11:03:31  field. 

11:03:32 They recover 
to the P5 plan
11:03:33  they like the idea 
in a they have a
11:03:37  plan where there's 
no disagreement.
11:03:38  So I think we can 
Pat ourselves in the
11:03:41  back about. 

11:03:42 That I think we have to

11:03:44  repeat it in 
the future. 
11:03:45 I even have other 
countries coming to me 
11:03:48 and asking me how dough 
do our planning
11:03:50  process now. 

11:03:51 So the word is out --

11:03:56  not just in the U.S. 

11:03:58 but around the

11:04:07  world. 

11:04:07 And our reputation 
as a field.
11:04:09  The is being Paul 
talks about it a
11:04:12  lot in his travels 
and I think a lot
11:04:15  of that again goes 
back to the P5 plan
11:04:18  and how well it's 
been received by the
11:04:21  administration of 
so I just encourage
11:04:23  everybody to have 
a good meeting and
11:04:26  keep in mind what 
they are trying to
11:04:29  do is have a good plan 
and get on the same page 
11:04:33 and work tock for 
the next one. 
11:04:35 Thank you very much.

11:04:37  

11:04:37 >> Thank you very 
much, Nigel for the
11:04:40  words of encouragement. 

11:04:41 We will take them 
to heart. 
11:04:43 At this moment I would

11:04:47  like to turn over 
the session to our
11:04:52  stallword local 
organizers. 
11:04:53 Bo in and

11:05:00  Brenda Taggart. 

11:05:01 >> Krista Young-Kee

11:05:04  is next. 

11:05:05 >> Okay. 

11:05:06 >> Let me

11:05:07  introduce. 

11:05:08 Young-kee who is our

11:05:09  current chair of 
the division of
11:05:11  particles and field.

11:05:15  

11:05:16 >> Thank you, Priesca. 

11:05:17 You can hear

11:05:20  me okay? 

11:05:21 I assume So it's 
not muted.
11:05:23  So I will briefly 
discussion goals of
11:05:27  the community planning 
meeting CPM.
11:05:30  And preliminary known 
as timeline and
11:05:42  report structure. 

11:05:43 Just a reminder --

11:05:45  You heard from Nigel 
but I want to
11:05:48  give you an example 
of strategic
11:05:51  planning. 

11:05:52 It start with a

11:05:54  community-wide 
science study. 
11:05:55 We

11:05:56  define the most 
exciting and important
11:05:58  questions for the 
field and identify
11:06:03  promising opportunity 
to address them.
11:06:08  Organized by DPS, 
division particles
11:06:11  and fielding to with 
other division,
11:06:13  physicallics and 
nuclear physical I
11:06:15  objects and physics 
of beams and this
11:06:17  is followed by another 
process called
11:06:23  the P5 project panel, 
that formulates
11:06:25  the exclusion plan 
in a vision of 20
11:06:28  years in a global 
context. 
11:06:30 Last one

11:06:32  took place in 2012 
and 2013 followed
11:06:39  by P5 in 2014, we 
are doing 2020 and
11:06:47  2021. 

11:06:48 And next year there 
will be P5.
11:06:50  Particle physics 
is global. 
11:06:52 And now involves 
community strong 
11:06:54 engagement

11:06:55  and use our plans 
Ann input to
11:06:57  analysis and we 
are not isolated. 
11:06:59 As

11:07:01  I said earlier we 
will be working
11:07:03  together with -- hour 
colleagues from
11:07:05  other divisions.

11:07:21  And as accomplish 
Canada mentioned,
11:07:24  -- as priss Canada 
mentioned I would
11:07:33  like to thank priss 
Canada that
11:07:35  chaired -- Prisca 
prepared it. 
11:07:37 It's

11:07:37  not one team does all. 

11:07:39 It's the team

11:07:40  working together 
to do our Snowmass
11:07:42  process. 

11:07:43 Again together with the

11:07:45  other divisions. 

11:07:46 There are

11:07:48  leaderships 
shown there. 
11:07:49 So this is

11:07:53  the snow mass steering. 

11:07:54 And we have

11:07:55  an advisory group 
and in addition to
11:07:58  steering group members 
we have the members from 
11:08:01 the executive committee 
and editor and 
11:08:03 communication and also

11:08:04  in addition 
we have seven
11:08:06  representatives 
from international
11:08:07  communities. 

11:08:07 I would like to take

11:08:10  this opportunity 
to give our special
11:08:18  thanks to international

11:08:27  representatives. 

11:08:28 They have been

11:08:30  important to 
our process. 
11:08:32 We have

11:08:36  large leaderships. 

11:08:37 Conveners and

11:08:38  career liaisons 
and early career
11:08:40  liaisons and this 
is all thank to the
11:08:43  community for your 
nominations and
11:08:45  these people -- sorry.

11:08:48  (phone ringing) And 
chosen primarily
11:08:52  on the outcome 
of nominations
11:08:55  nominations nominations 
and outcomes.
11:08:58  And today we have 
30 enter developers
11:09:01  you will hear from 
them the key
11:09:03  questions in their 
frontier so far.
11:09:05  Outbreaks of sessions 
and the plans
11:09:08  and steps between 
now and summer study
11:09:11  next year. 

11:09:12 There's a weekly page

11:09:15  known as 21.org which 
is a one-stop
11:09:17  shop. 

11:09:18 You have all the 
information
11:09:20  related to Snowmass. 

11:09:21 You can find that. 

11:09:23 And we hope to 
have you visit
11:09:25  as often as possible. 

11:09:27 We are also

11:09:31  very delighted that 
there is strong
11:09:34  engagement from the 
career process.
11:09:36  All community members 
should feel safe
11:09:38  and supported in 
exchanging ideas
11:09:40  through this process. 

11:09:41 So we formed

11:09:42  the ethics task force 
early this year
11:09:45  and they produced 
the four principals
11:09:50  and community 
guidelines and also was
11:09:53  a team for this 
week's meeting. 
11:09:55 We

11:09:56  currently establishing 
an ethics
11:09:57  committee, that no 
real members will
11:10:02  be announced early 
November this year.
11:10:05  The Snowmass timeline, 
especially the
11:10:07  community-wide 
get together. 
11:10:08 We

11:10:09  started a meeting 
in April this year
11:10:12  at the APS April 
meeting. 
11:10:14 Now we have

11:10:17  four days of a planning 
meeting. 
11:10:19 And

11:10:20  we are planning to 
have another small
11:10:23  get together. 

11:10:24 April meeting neck year

11:10:27  but finally a ten-day 
long workshop --
11:10:31  again involving all 
the community. 
11:10:33 So

11:10:36  to prepare this week's 
meeting, I have
11:10:39  received many -- 
in fact more than
11:10:44  1500 letters of 
interest from our
11:10:46  community. 

11:10:47 Our frontier communities

11:10:49  spend a lot of time 
understanding and
11:10:53  analyzing to prepare 
the bottom -- the
11:10:57  class shows that 
when they were
11:11:00  submitted -- Not 
surprisingly, 28
11:11:04  hours, also the day 
before, from the
11:11:06  deadline we have 
most otherwise
11:11:09  received and also 
you will notice that
11:11:11  there are many covering 
different
11:11:14  types of groups 
and different
11:11:15  frontiers. 

11:11:16 Showing really

11:11:19  interconnected the 
areas of research.
11:11:23  For this week's 
meeting, because they
11:11:25  have been already 
a popular group and
11:12:03  have been already 
a popular group and frontier groups having 
had their own meetings and workshops. 

11:12:03 Therefore,
 this week when 
we have this opportunity to bring 
together the
11:12:03  community across 
the field we would like to he to 
cuss on more interpreting 
discussions and also to
11:12:03  establish a cross-work 
group connections. 
At the same time, we

11:12:03  would like to identify 
gaps and areas to focus or for 
further studies. And

11:12:03  also to brainstorm 
new ideas. And
 planning sessions 
will hear about
11:12:03  excitement about 
the field and plans from other regions 
and related fields
11:12:04  and messages from 
funding agencies and
11:12:06  voices of community. 

11:12:07 So overall our

11:12:10  goal this week is 
to produce -- plan
11:12:13  the steps to take 
between now and the
11:12:16  Snowmass summer 
study next year.
11:12:20  Leading to a final 
report in October
11:12:22  of 2021. 

11:12:23 So after the -- this week

11:12:27  there will be 
a lot of effort
11:12:30  throughout the groups 
and frontier,
11:12:32  understanding what 
further studies are
11:12:34  to be done and what 
kinded of papers
11:12:37  could be produced. 

11:12:39 I saw a lot of

11:12:41  discussion happen. 

11:12:42 And between --

11:12:43  around the end 
of this year to
11:12:46  February/March we 
could like to have a
11:12:48  couple of rules 
developing key
11:12:50  questions and 
opportunities. 
11:12:51 And

11:12:53  February to March, 
April time, popular
11:12:56  groups producing 
outlines of their
11:13:00  reports. 

11:13:01 Finally April 
to June time,
11:13:03  preliminary matter 
frontier report.
11:13:05  You will see that 
each one we had a
11:13:09  range of a few months 
because group to
11:13:11  group, they may have 
decided different
11:13:15  plans and timeline. 

11:13:16 Also ways of

11:13:17  getting people from 
the community.
11:13:20  Solve there will be 
enough flexibility
11:13:24  in that. 

11:13:25 So for the summer study

11:13:27  time, our goal is 
to build a consensus
11:13:30  on key questions and 
opportunities of
11:13:32  the entire physics 
field and enabling
11:13:35  technologies and 
community engagements
11:13:38  engagements and 
to form late the
11:13:40  compliment of Snowmass 
executive
11:13:47  summary and after 
the CS weS we have a
11:13:50  report by the 
end of October. 
11:13:52 This is a starting point 
for discussion. 
11:13:55 We would like to get 
more feedback this
11:13:58  week. 

11:13:59 Concerning the 
core structure,
11:14:05  our thinking plan 
is to use the 2013
11:14:09  Snowmass with 
a summary. 
11:14:10 With a few pages from 
frontier summary. 
11:14:13 And then

11:14:15  we will have the 
frontier report, that
11:14:19  itself will start 
with the frontier
11:14:21  summary and popular 
report and they
11:14:23  will be used 
as references. 
11:14:25 Again

11:14:25  this is something 
we would like to get
11:14:28  feedback for 
you this week. 
11:14:30 Thank you

11:14:31  I would like to 
thank our program
11:14:35  committee for CPM. 

11:14:36 Presented to other

11:14:40  careers and chairs 
of the local
11:14:46  organizationing 
committee. 
11:14:47 In

11:14:47  particular all 
frontier has a
11:14:49  committee and members 
have done an
11:14:52  incredible job to 
organizing very
11:14:54  nontrivial breakout 
sessions. 
11:14:55 And of

11:14:57  course a special, 
special thanks has
11:15:00  to go to our local 
committee. 
11:15:02 Thank

11:15:04  you very much. 

11:15:05 And next one will be a

11:15:07  report from the 
local organizing
11:15:09  committee.

11:15:14  

11:15:15 >> Sorry for reversing 
the order of
11:15:19  the two. 

11:15:20 But thank you, 
Young-Kee for
11:15:22  getting us on the 
path now and for
11:15:25  details of this week's 
festivities, if
11:15:28  you like. 

11:15:29 We will listen to 
Bo and Brendan.
11:15:33  

11:15:33 >> Thank you, Prisca.

11:15:39  So good morning, 
afternoon or
11:15:40  evening, depending 
on where you are in
11:15:45  the world my name 
is Bo Jayatilaka.
11:15:48  And I would like 
to welcome to you
11:15:51  Snowmass committee 
planning meeting.
11:15:53  You saw from Young-kee 
who we are.
11:15:57  But you may be 
wondering why this
11:15:58  meeting has a 
local organizing
11:16:00  committee. 

11:16:01 When we started this

11:16:02  process we were hoping 
to welcome you
11:16:04  in opinion person 
and we would be the
11:16:07  people you could ask 
about cookies at
11:16:10  the breaks but yet 
here we are at
11:16:12  another Zoom meeting 
which we are all
11:16:15  very used to 
at this point. 
11:16:17 Nonetheless we putting 
to a set of Zoom 
11:16:20 meetings that will be 
productive as a start to 
11:16:23 the main part of the 
Snowmass process. 
11:16:25 You can see on the

11:16:27  right the blocked 
schedule for the
11:16:30  meeting. 

11:16:31 The plan near sessions in

11:16:33  blue are all through 
today and
11:16:35  Wednesday. 

11:16:36 They will be held on the

11:16:38  Zoom webinar as 
this session is. 
11:16:40 So you will use the 
same information as
11:16:44  you used today. 

11:16:46 In the parallel

11:16:47  breakouts these will 
be held in the
11:16:49  regular Zoom meetings 
you are
11:16:51  accustomed to to year. 

11:16:53 We will be sending 
information for breakout
11:16:55  meetings later today 
likely after the
11:17:05  plane near sessions 
-- After the
11:17:07  plenary sessions end. 

11:17:09 They start at 5

11:17:13  p.m. 

11:17:13 on the west coast 
and 1 p.m. 
11:17:16 on east coast so to 
organizers please be
11:17:19  mindful of these 
constraints and
11:17:22  everybody's time. 

11:17:23 One advantage of

11:17:25  having this meeting 
be virtual is it
11:17:27  does lower the 
barrier for
11:17:29  participation because 
there isn't
11:17:31  travel involved. 

11:17:32 There's over 2500

11:17:34  participants and 
while there is a
11:17:36  heavy participation 
in the U.S. 
11:17:37 time zones you can see 
that we really do
11:17:41  have participation 
from around the
11:17:42  grown in this time 
zone and on the
11:17:45  right you can see 
a very diverse
11:17:48  reputation of frontier 
interests
11:17:49  amongst the ten 
frontiers in the
11:17:53  Snowmass 2021 process. 

11:17:54 Now this

11:18:00  differs of people 
drivers of people
11:18:02  dissers havity we 
are agreeing to take
11:18:05  part in this meeting. 

11:18:06 At its core we are 
agreeing and respect 
11:18:09 each others

11:18:12  the members of 
the community and
11:18:15  engage in constructive 
guidelines.
11:18:18  What is expected 
of you and what the
11:18:21  accountability 
procedures are in this
11:18:24  document linked in 
this snow masswiki.
11:18:26  Everyone is 
encouraged for
11:18:28  constructivity 
and supportive
11:18:29  collaboration. 

11:18:30 And your first point.

11:18:31  Contact for any time 
that you think
11:18:33  you see a violation 
of the core
11:18:36  principals and 
community guidelines
11:18:37  are the conveners 
and organizers of
11:18:41  this meetings and 
its sessions. 
11:18:43 Who

11:18:43  have all received 
training and its
11:18:48  handlers. 

11:18:48 That means the 
pron tear at
11:18:50  Snowmass. 

11:18:51 They are encouraged 
to have
11:18:53  early intervention 
and appropriate
11:18:54  enough to observe 
issues and don't
11:18:57  deviate from the 
task force as well
11:18:59  and you can find their 
contact information at 
11:19:02 the same link 
above here. 
11:19:04 And you should remember 
that show mass is most 
11:19:07 successful and 
everybody's voice -- 
11:19:08 Snowmass is most 
successful and 
11:19:10 everybody's voice 
can be heard. 
11:19:12 In terms of hearing your 
voice, since is this is 
11:19:15 a planning meeting we 
want to make it as 
11:19:19 conducive as possible to 
discussions that help 
11:19:21 with that planning 
process. 
11:19:22 One of the main points 
to make here is that the 
11:19:26 Snowmass slack will have 
a series of dedicated 
11:19:29 channels for the CPM. 

11:19:31 This he all start with 
CPM for the channel 
11:19:34 name. 

11:19:35 For example there is 
one for each plenary 
11:19:38 session. 

11:19:38 Where you can have 
discussions during the 
11:19:41 session and ask 
individual questions. 
11:19:42 The Zoom rooms for 
parallel breakouts were 
11:19:45 set up so everyone could 
take part and generally 
11:19:48 you will be able to 
share a video and speak 
11:19:52 in the audio and take 
part in those meetings 
11:19:55 and you can set up Zoom 
rooms for additional 
11:19:58 discussions. 

11:19:59 You can use the chat. 

11:20:01 >> One thing that is in 
line with the community
11:20:04  guidelines is you 
set your Zoom and
11:20:07  slack display names 
to your preferred
11:20:09  name. 

11:20:10 It doesn't have 
to be your
11:20:12  legal and birth name 
but we ask you
11:20:14  don't have an email 
address or user
11:20:18  name set so you can 
Tuesday on the tab
11:20:21  in the participants 
list ask you can
11:20:23  include your personal 
pronouns as well
11:20:25  there. 

11:20:26 One question in 
a comes up is
11:20:28  how you can ask 
questions in this
11:20:37  webinar forum. 

11:20:38 We prefer you use the

11:20:39  webinar link and the 
Zoom chat panels.
11:20:44  And if there is time 
they will choose
11:20:47  questions to ask 
and all questions
11:20:49  will be copied to 
slack afterwards and
11:20:53  encourage speakers 
to hang around and
11:20:56  ask questions. 

11:20:57 So that's it for us we

11:20:59  hope have you a 
productive meeting of
11:21:01  if you have questions 
or problems
11:21:03  first line is 
to look at the
11:21:06  participant guide. 

11:21:07 And if not feel

11:21:09  free to email or Canuck 
us at the CPM
11:21:12  underscore help 
channel on slack.
11:21:14  Thank you and I will 
hand things back
11:21:17  to Prisca. 

11:21:18 >> Thanks. 

11:21:19 Remarkably on time. 

11:21:20 Our next speaker 
is Joanne
11:21:23  Hewitt, who is the 
current chair of
11:21:26  Hpath and the 
lab director for
11:21:28  fundamental statistics. 

11:21:29 And she will

11:21:33  fire us up with the 
exists still ahead
11:21:36  for us.

11:21:36  

11:21:37 >> Thank you, Prisca. 

11:21:38 Good morning, everyone. 

11:21:40 I have to say I look 
forward to the day when 
11:21:44 we can all see each 
other again as three 
11:21:47 dimensional people. 

11:21:48 So I've been charged to 
talk about the exciting 
11:21:51 physics that 
is before us. 
11:21:53 I've taken this to mean 
during the next decade. 
11:21:56 And I would like to 
start with what was in 
11:21:59 the P5 report. 

11:22:01 So this chart 
on left is a
11:22:04  list of projects 
that was in the 5-5
11:22:07  plan. 

11:22:08 It's a long list. 

11:22:09 And as you know it's 
colored so that the green
11:22:13  bars are experiments in 
operation and analysis 
11:22:15 and the blue bars are 
under fabrication or 
11:22:18 discussion. 

11:22:19 And the yellow bars are 
conceptual and technical 
11:22:22 design. 

11:22:22 The white horizon line 
is where we are today. 
11:22:25 Almost at the end 
of calendar 2020. 
11:22:28 And you see that empty 
these projects are now in
11:22:31  the green or assumed 
-- soon to be in
11:22:39  the green. 

11:22:40 So that means all of our

11:22:42  hard years of labor 
are now turning
11:22:45  into project. 

11:22:46 The remainder will be 
operating by the end of 
11:22:49 the decade. 

11:22:50 So during this talk I 
will March down this 
11:22:53 list of projects and 
discuss the physics that 
11:22:56 we now be able to reason

11:23:02  from in republican 
from in decade of
11:23:06  reap. 

11:23:07 I will start with 
the moment of
11:23:10  the Muon. 

11:23:11 There's been 
discrepancies
11:23:12  of 15 years old, 
if not olderby now
11:23:16  between the standard 
and model
11:23:19  predictions. 

11:23:19 E821 achieves a

11:23:22  sensitivity of 540 
parts per billion
11:23:25  and the measurement 
has recently been
11:23:28  determined to be 
3.7 stigma with the
11:23:30  model. 

11:23:31 You will see why I said

11:23:34  recently in a minute. 

11:23:36 The -2

11:23:37  experiment at Fermilab 
started data
11:23:38  taking in 2018. 

11:23:40 They completed three

11:23:41  runs and they have 
two more to go as
11:23:44  you can see from that 
plan on the very
11:23:47  right. 

11:23:48 The target sensitivity 
is a
11:23:50  factor of four 
improvements but four
11:23:52  and a half improvement 
over that from
11:23:54  the brook haven run. 

11:23:56 The world is

11:23:57  holding its breath 
waiting for these
11:23:59  three results. 

11:24:00 Come on, guys. 

11:24:02 We want to see they. 

11:24:04 There's also an 
experiment, an 
11:24:06 independent experiment

11:24:06  in Japan at J-park 
that uses an
11:24:09  alternative technique. 

11:24:10 It's a

11:24:10  accelerated low 
emittance and
11:24:14  operations there 
planned for 2024 and
11:24:16  2026. 

11:24:17 This will serve 
as an important
11:24:21  cross-check to any 
results that Muon
11:24:24  G-2 will get in the 
case it disagrees
11:24:27  from the standard 
model. 
11:24:29 While we are waiting 
for the experimental 
11:24:31 results, the theory 
community has been
11:24:35  extremely active. 

11:24:36 There is a Muon

11:24:38  G-30 initiative that 
recently put out
11:24:40  a tone of 200 pages 
and about the same
11:24:47  number of Arthurs. 

11:24:49 authors. 

11:24:49 It's an impressive 
author list from around 
11:24:52 the

11:24:52  wore. 

11:24:53 They have made 
it notoriously
11:24:55  difficult to make 
contributions to the
11:25:02  G-2. 

11:25:03 The polarization 
vacuum and the
11:25:05  hydronic -- ask there's 
air decomb.
11:25:13  With this new 
determination that now
11:25:16  says the escapesy 
is with 3.7 sigma.
11:25:19  Of course we 
have the LHC. 
11:25:21 There's

11:25:24  much more data to come. 

11:25:26 Regardless of

11:25:27  anything you read 
in science magazine
11:25:29  there's much more 
dad to come ask much
11:25:32  more physics to come. 

11:25:34 Run 2 delivered

11:25:35  5% of the anticipated 
3AB that is
11:25:37  expected in the high 
Lumme no, sirrity
11:25:40  program for the LHC. 

11:25:42 As well as a run

11:25:53  3 upcoming. 

11:25:54 One of the most important

11:26:08  thing is the his 
coupling managements.
11:26:11  We got the his to 
-- as you can see
11:26:22  in the middle platform 
and limiting.
11:26:24  And the holy grail 
for Higgs which
11:26:27  will soon become 
available to the LHC
11:26:30  in the high luminosity 
era. 
11:26:32 In

11:26:32  addition to these 
very important Higgs
11:26:34  coupling measurements 
they will
11:26:36  continue to explore 
the unknown.
11:26:38  There's precision 
tests of the
11:26:40  standard model that 
will get even
11:26:43  better as the data 
accumulates. 
11:26:44 And

11:26:46  the seven for new 
physics and dark
11:26:49  matter is not over. 

11:26:51 There are many

11:26:52  increasing channels 
in order to tease
11:26:55  the small for new 
physics in the
11:26:57  background. 

11:26:58 Most notably is from

11:27:02  super Sim symmetry. 

11:27:03 The precise 
interpretation of this 
11:27:05 data is of

11:27:06  course made possible 
by theory. 
11:27:08 The

11:27:08  one stop impossible 
has now become
11:27:11  state-of-the-art 
for calculation and
11:27:13  standard model 
processes and that's
11:27:15  next to next to 
leading order. 
11:27:17 As you

11:27:18  can see from the 
plot on the bottom
11:27:21  right, the level 
of precision that
11:27:23  these cross sections 
-- This is the
11:27:31  cross section for 
Higgs production
11:27:36  from fusion is next. 

11:27:37 So what is next?

11:27:39  What's the next 
collider? 
11:27:40 This can be the topic 
of discussion over the
11:27:43  Snowmass process and 
has already been
11:27:46  over the summer. 

11:27:47 There's many 
differenting ons to 
11:27:49 study and some designs 
more mature than others 
11:27:51 and IOC is the most 
mature, having had a
11:27:55  TDR for almost 
a decade now. 
11:27:57 The 2020 update in the 
European particle
11:28:01  physics strategy 
recommended an
11:28:03  electric Ron physics 
factory as the
11:28:05  highest priority 
next collider. 
11:28:07 They made this 
recommendation because of
11:28:10  the percent level 
determination of
11:28:18  Higgs coupling field. 

11:28:20 In addition the

11:28:23  coupling really comes 
into play at an
11:28:27  E plus, E minus 
Higgs factory. 
11:28:29 This chart at the bottom 
left hand corner
11:28:32  of the screen is yet 
another study of
11:28:35  the degree of accuracy 
of measurements
11:28:37  of all of the Higgs 
Cummingss of all
11:28:40  the various types 
of Higgs machines.
11:28:45  You can see in most 
wayses percent
11:28:50  level or subpercent 
level precision is
11:28:53  achievable and decays 
continue limited
11:28:55  at the 10% level. 

11:28:57 The bottom right

11:28:59  chart shows the 
precision that is
11:29:01  available for the 
cuppings at the
11:29:03  various machines. 

11:29:04 If you look at the

11:29:06  solid bars, those 
are the ones that
11:29:08  are are the for 
production, so it
11:29:11  shows the cupping. 

11:29:12 The figures of

11:29:13  merit to keep 
in mind is a 50%
11:29:16  precision which is 
achievable at the
11:29:26  high luminosity LHC 
removes the 935%
11:29:30  coupling level. 

11:29:31 And 20% precision

11:29:34  existence at 5 sigma 
and 5 to 10%
11:29:37  precision that becomes 
possible at
11:29:39  20EVE is what is 
they'ded for quantum
11:29:42  level corrects. 

11:29:43 This is what is

11:29:45  needed to really 
study the shame of
11:29:47  the Higgs potential.

11:29:52  Back to exploring 
the unknown, rare
11:29:55  processes are also 
going to have a
11:29:59  significant role to 
play over the next
11:30:08  decade. 

11:30:09 Rare B Meson 
decays in the
11:30:12  announce I wills 
persist in various
11:30:14  districts. 

11:30:15 20 to 30 types of

11:30:16  distributions and 
at various levels of
11:30:19  discrepancies 
from the level. 
11:30:21 All

11:30:25  around 3 sigma. 

11:30:26 Here is one on the

11:30:30  right. 

11:30:31 Starting at +/minus which

11:30:33  shows the data better 
than that of a
11:30:36  standard model 
prediction at a 3 sigma
11:30:38  level. 

11:30:39 Players in the 
future to watch
11:30:43  for there are bell, 
bell 2 has turned
11:30:45  on. 

11:30:46 They go achieve 
5 B by the end
11:30:49  of their run and 
they have now since
11:30:52  this past summer 
reclaimed the world
11:30:58  luminosity record. 

11:30:59 Atlas/CMS do 3AB

11:31:02  and LHCb at the end 
of a high looming
11:31:05  run. 

11:31:06 So watch this space. 

11:31:08 This is another area 
where discrepancy from
11:31:10  the standard model 
could go from the 3
11:31:13  sigma to a 5 sigma. 

11:31:15 Another exciting 
experiment that will 
11:31:17 come online

11:31:22  during the next decade 
is mute E which
11:31:26  will test charged 
Lepton flavor
11:31:31  violation. 

11:31:31 It will have Lepton

11:31:36  violations it measures 
aluminum nuclei
11:31:41  to a sensitivity 
of 3 x 10 -17 over
11:31:44  orders of magnitude 
over previous
11:31:46  measures. 

11:31:46 They go start taking data

11:31:48  (n)2024. 

11:31:49 Reaching their full 
sensitivity by the end 
11:31:51 of the decade and will 
be able to probe new 
11:31:55 physics

11:32:00  up to 10 of the 4VEV 
and interactions
11:32:03  and of course a 
flagship of our
11:32:09  domestic program is 
in the nutri know
11:32:21  program in the 
Fermilab. 
11:32:22 There is a

11:32:24  process summed 
over Neutrino and
11:32:26  anti-Neutrino 
modes from the
11:32:27  collaboration alone. 

11:32:28 This is shown on

11:32:29  the chart in the 
right where you see
11:32:33  particularly Loewen 
gives in the
11:32:35  Neutrino energy 
distribution. 
11:32:36 The

11:32:37  data is quite a bit 
higher than the
11:32:39  standard background 
prediction. 
11:32:41 If

11:32:41  you include the LSND 
results in the
11:32:44  analysis the access 
grows from 4.8
11:32:49  sigma to 6.1. 

11:32:50 Timing information at

11:32:52  miniboo shows it's 
timed with the
11:32:55  interacting in 
the volume. 
11:32:56 So it is

11:33:05  not due to the entering 
the detector.
11:33:07  Microboo has begin 
displays with the
11:33:09  promise that results 
will be coming
11:33:16  very soon. 

11:33:17 Again the word is holding

11:33:19  its breath. 

11:33:20 Waiting for the results.

11:33:22  And another independent 
check of these
11:33:24  anomalies anomalies 
and the detector
11:33:25  is under construction 
and will be
11:33:28  operating in a 
couple of years. 
11:33:30 So by mid-decade, 
we will have many
11:33:32  different experiments 
in the short
11:33:34  baseline Neutrino 
program. 
11:33:35 Checking

11:33:36  for these anomalies 
and seeing if they
11:33:40  persist or not. 

11:33:41 And that will give us

11:33:43  plenty of Neutrino 
physics while the
11:33:45  construction of 
the long baseline
11:33:51  Neutrino facility, 
the detector doom
11:33:54  and the accelerator 
upgrade 2 are
11:33:58  underway. 

11:33:58 The scientific program of

11:34:03  dune has grown since 
it was first
11:34:12  perceived by Q5 
to include nuke I
11:34:23  don't know decay 
and now includes
11:34:26  includes dark 
matter displays.
11:34:28  There's a multivolume 
DTR that came
11:34:32  out earlier by the 
collaboration dune.
11:34:35  And you can see 
the sensitivity on
11:34:39  the charts on right. 

11:34:41 Without the range. 

11:34:42 And possible value of 
the phase you can 
11:34:45 measure the level that

11:34:47  can be determined 
of CP violation is
11:34:49  given by these 
purple and orange
11:34:51  curves with the staged 
approach with
11:34:53  the purple going 
for seven years in
11:34:56  the staged approach. 

11:34:57 Stage approach

11:34:58  is when the different 
detector modules
11:35:01  at the far side 
start to turn on. 
11:35:04 And then ten years 
within the orange. 
11:35:07 The chart on the very 
right shows the
11:35:09  rescission at which 
the angle Delta
11:35:12  can be measured 
for each different
11:35:14  value. 

11:35:15 And you can see 
that it ranges
11:35:17  basically from 5 to 
16% with 15 years
11:35:22  of data taking in 
the staged approach.
11:35:24  Meanwhile construction 
of the project
11:35:27  is underway. 

11:35:28 We can see the beautiful

11:35:30  pictures on the bottom. 

11:35:31 Vet excavation on 
the far side. 
11:35:33 I have to say the first 
time I saw that it
11:35:37  reminded me when I 
saw the digging of
11:35:40  the SSC tunnel. 

11:35:41 It's nice to see 
excavating unground 
11:35:43 again. 

11:35:44 There's preparation 
of the near site. 
11:35:46 The first steps are 
clearing out the stuff
11:35:51  that is already there. 

11:35:53 And last

11:35:58  summer there was 
a ground for the
11:36:00  caregenic plant. 

11:36:01 Moving on to the

11:36:02  dark side universe 
there is tension in
11:36:05  the model measurements 
that persist at
11:36:08  the 2 to 3 sigma level. 

11:36:10 I borrowed

11:36:13  this set of plots 
by David Kirkby at
11:36:17  Irving which shows 
recent results from
11:36:20  the complete digital 
sky survey of bar
11:36:33  I don't know isolation. 

11:36:35 You can see

11:36:36  the measurements of 
the parameters we
11:36:38  have the distance 
ladder versus the
11:36:46  hubbell on the left. 

11:36:48 In the In the

11:36:52  center the city -- 
and on the left A
11:36:55  is related to the 
red shift distance
11:36:57  of the galaxy. 

11:36:59 And you see in each 
cases there's a slight 
11:37:02 discrepancy between the 
different types of
11:37:04  measurements. 

11:37:05 We are looking forward

11:37:06  to the new data that 
will be coming
11:37:09  out in the next 
decade, which will
11:37:12  hopefully resolve 
this tension between
11:37:13  these different types 
of measurements
11:37:16  or not. 

11:37:17 DES is poised 
to release the
11:37:19  analysis of its 
three-year dataset
11:37:22  very soon. 

11:37:23 Daisy, the dark energy

11:37:25  survey has completed 
a construction.
11:37:27  Commissioning is 
underway and we will
11:37:29  start taking 
data in 2021. 
11:37:31 You see

11:37:38  the forecast for 
Dacey here in the
11:37:40  Dacey in the 
middle plot. 
11:37:42 The survey

11:37:54  was able to do 
is remarkable. 
11:37:56 You get another factor 
in which you combine
11:38:04  all the measurement 
techniques. 
11:38:05 So the Vera Rubin 
observatory will
11:38:07  conduct the legacy 
service of space
11:38:10  and time, and it 
will turn somewhere
11:38:13  between 2023 and 
2024, depending on
11:38:15  how long this pandemic 
lasts twill
11:38:17  record images of 
10 billion galaxies
11:38:19  to observe the nature 
of dark energy
11:38:24  and the DUE piece 
of the telescope,
11:38:27  the 3.4 mega Pixel 
camera is now
11:38:31  complete it. 

11:38:32 Took this world famous 
photo of broccoli shown 
11:38:35 in the chart

11:38:36  on the right. 

11:38:37 This photo got about 10 
million hits already on 
11:38:40 the web in the

11:38:42  first week it was 
up last month.
11:38:44  Commissions and 
preparations for
11:38:46  operations is underway. 

11:38:47 One thing

11:38:48  that is different 
in this facility
11:38:51  from what is normal 
in the community
11:38:54  is that the facility 
will serve ago
11:38:56  different science 
collaborations so
11:38:58  there is no Vera 
Rubin collaboration
11:39:02  or an LSST 
collaboration. 
11:39:03 The

11:39:04  collaboration that 
will study dark
11:39:07  energy is the dark 
energy design
11:39:09  collaboration ask 
they have been busy
11:39:12  preparing themselves 
for the onslaught
11:39:15  of data that will 
be coming their way
11:39:21  with ALSD. 

11:39:22 They have been looking at

11:39:23  challenges and will 
sharpen tools in
11:39:26  preparation for start 
of organizes and
11:39:29  you can see the 
simulated on the
11:39:31  right. 

11:39:32 I see I need to 
speed up just
11:39:35  a little bit. 

11:39:36 I think I can do. 

11:39:39 That

11:39:39  moving on to cosmic 
microwave
11:39:45  background organizes 
we have the
11:39:47  bicep/Keck array 
and south pole
11:39:50  telescope they have 
merged to form the
11:39:52  south pole observatory. 

11:39:54 And they will

11:39:57  be measuring the 
error on tensor so
11:39:59  scale measure are 
at the level of .00
11:40:02  about by the end 
of 2023 when they
11:40:05  finished data intaking. 

11:40:07 This is of

11:40:11  course on the way 
to C NMB stage 4.
11:40:15  It has a number 
of primary science
11:40:19  drivers you can 
see where they fit
11:40:22  here in the power 
spectrum from low
11:40:26  values. 

11:40:26 You measure the 
gravitational
11:40:30  waves from inflation. 

11:40:31 Up to the light

11:40:32  constraints as 
well as many
11:40:35  astrophysical and 
Astro particle
11:40:39  measurements. 

11:40:39 We looking forward to

11:40:41  this. 

11:40:42 It is just now starting. 

11:40:44 The

11:40:44  project has passed 
CD0 and going for
11:40:53  CD1 sometime next 
year and it will
11:40:57  start taking matter 
at the end of this
11:41:00  decade. 

11:41:01 Dark matter generation 2

11:41:02  experiments. 

11:41:03 There are two. 

11:41:04 LZ is

11:41:07  the higher mass 
range from 10Tev.
11:41:11  Operations will be 
starting in 2021 as
11:41:17  soon as slack finishes 
purifying the
11:41:28  liquid Xeon. 

11:41:29 And Scdms from .5-5Ge V

11:41:31  and will start 
operations in 2022.
11:41:33  This is another 
occasion of watch this
11:41:35  space for new physics 
that will occur
11:41:37  very soon. 

11:41:39 Starting in the next year

11:41:48  or two. 

11:41:49 The third experiment AVMS

11:41:50  recently started 
approving a new
11:41:52  model. 

11:41:53 They had continue 
to operate
11:41:56  and improve 
their search. 
11:41:57 Briefly at

11:41:59  the end, what is 
new since P5? 
11:42:01 That's

11:42:02  the set of P5 projects. 

11:42:04 What is new since them? 

11:42:06 Well the community has 
been very imaginative 
11:42:09 and realized

11:42:10  that there's more 
to dark matter than
11:42:13  wimps. 

11:42:14 Or Axons. 

11:42:15 In fact there's a

11:42:17  whole range that 
composes 36 of
11:42:19  magnitude ask 
there's been an
11:42:22  explosion of ideas 
for the searches.
11:42:29  I've listed picture 
here of five of
11:42:34  these pro jokes who 
are in defunds in
11:42:36  order to prepare 
themselves. 
11:42:38 For

11:42:38  construction as Des 
tornado by a bake
11:42:41  needs workshop that 
was held a couple
11:42:45  of years ago. 

11:42:46 Quantum information

11:42:48  science is another 
area that is new
11:42:52  since the P5. 

11:42:53 This has been

11:43:03  investments in AGP 
with the quantityd
11:43:06  SED program. 

11:43:07 There has been a range

11:43:10  from quantum techniques 
to algorithms
11:43:15  to data analysis 
to table-top
11:43:17  holograms.

11:43:17  

11:43:17 >> One of the 
applications for
11:43:19  physics is that in 
the compassion and
11:43:22  the ability to look 
for dark matter in
11:43:26  new ways. 

11:43:27 So this is taking many

11:43:29  different techniques 
I quantum sensing
11:43:31  which provides the 
sensitivity to
11:43:33  search for dark matter 
in new regions
11:43:36  that we would not 
be able to before.
11:43:39  Last but not least, 
of course, can
11:43:42  gravitational wave 
science is what
11:43:44  brought us a noble 
prize quite
11:43:46  recently. 

11:43:47 They provide 
information on
11:43:50  ther I will universe 
back to
11:43:52  inflation. 

11:43:53 But it's difficult or

11:43:54  impossible to assess 
by other methods
11:43:58  and provides a new 
way to probe the
11:44:02  cosmos and implore 
fundamental
11:44:05  physics. 

11:44:06 It provides cos moll give

11:44:07  and particle physics 
and even theory
11:44:10  has gotten into 
the realm here of
11:44:12  making predictions 
of much more
11:44:14  accurate. 

11:44:15 They are now doing higher

11:44:19  order calculations 
in the inn spiral
11:44:22  velocity and Newton's 
constant in
11:44:28  order to look for 
massive scale binary
11:44:30  systems. 

11:44:31 There's the future of

11:44:32  gravitational wave 
measurement which
11:44:34  can benefit from 
particle physics
11:44:45  expertise. 

11:44:46 There's generation laser

11:44:47  interferometer. 

11:44:48 It will increase the

11:44:51  sensitivity in 
frequency range from 10
11:44:55  to 1,000 hertz. 

11:44:56 And there's also a

11:45:00  possibility of an 
atom interferometer.
11:45:02  A prototype that 
is being built now
11:45:05  where they act as 
waves between two
11:45:09  atom sources while 
they are in
11:45:12  freefall. 

11:45:13 This probes gravitational

11:45:16  waves in a different 
frequency range
11:45:22  in the different 
interferometers and
11:45:24  puttings them 
back together. 
11:45:25 So putting this August 
together this is a
11:45:28  remarkable achievement 
the community
11:45:30  has done and continues 
to built as
11:45:32  part of the P5 plan 
and we should all
11:45:35  be proud of ourselves. 

11:45:37 There's been a sacrifice 
for us to do. 
11:45:40 That but we should be 
proud of ourselves for
11:45:43  having accomplished 
that. 
11:45:44 And over

11:45:47  the next decade as 
we do finish all of
11:45:52  these construction 
projects the
11:45:55  community will wait 
for the science
11:45:59  experiments. 

11:46:00 There are several

11:46:01  sciences addressing 
these anomalies.
11:46:04  There are discoveries 
of new
11:46:07  properties and 
interactions waiting to
11:46:10  be made by the 
experiments and
11:46:12  theorists will 
be kept very busy
11:46:14  interpreting the data. 

11:46:15 So in conclusion the 
next decade will be a
11:46:19  very exciting time 
for particle
11:46:22  physics. 

11:46:22 Thank you. 

11:46:23 >> Thank you so

11:46:25  much. 

11:46:25 That was a wonderful 
description of the 
11:46:28 landscape before

11:46:29  us. 

11:46:30 And I'm excited, 
in any case we
11:46:33  actually don't have 
I in questions on
11:46:35  the Q&A and we are 
out of time any
11:46:38  way. 

11:46:39 So I think I will 
just remind
11:46:41  you that you can put 
your questions on
11:46:46  slack. 

11:46:47 And they will be 
answered when
11:46:55  shellac is back up. 

11:46:57 We do know that

11:46:58  Slack is having 
service-wide shortages
11:47:00  this morning. 

11:47:01 So feel free when

11:47:02  everything is available 
again to ask
11:47:04  your questions in the 
Slack channel to Joanne.
11:47:07  So at this point, 
I would like to
11:47:10  move on to our 
next session. 
11:47:12 And hand

11:47:13  it over to the chair 
of that session.
11:47:22  Grande Glenys who 
is the chair.
11:47:25  

11:47:26 >> Thanks a lot Joanne. 

11:47:28 Thanks for that 
wonderful talk. 
11:47:30 I'm originally a

11:47:31  particle theorist. 

11:47:32 I'm from NYU. 

11:47:33 So it's a real honor 
and pleasure to be
11:47:36  moderating this 
session. 
11:47:37 Our first

11:47:39  speaker is Jurgen 
from the university
11:47:42  in Brussels. 

11:47:43 He's a member of CMS and

11:47:46  is currently the chair 
of the European
11:47:48  committee for future 
accelerators and
11:47:50  has been one of the 
participants in
11:47:52  the European strategy. 

11:47:54 So we will

11:47:56  hear from him about 
European plans.
11:47:58  Thank you very much. 

11:48:00 I hope we can make this 
transition properly.
11:48:03  

11:48:03 >> Thank you very much. 

11:48:05 And thank you as well 
for the opportunity to
11:48:09  present the plans 
for particle physics
11:48:11  in Europe. 

11:48:12 In a moment you 
should see
11:48:14  my screen. 

11:48:15 If that will not be the 
case please shout.
11:48:18  And now we should 
be able to move
11:48:24  forward with this.

11:48:30  

11:48:31 >> I see your screen 
fine, Jorgen but
11:48:37  not you. 

11:48:38 Start your video. 

11:48:40 Had

11:48:40  

11:48:40 >> I can do that. 

11:48:42 But it's not

11:48:43  optimal for doing 
everything. 
11:48:45 So

11:48:48  maybe we throw 
in like this. 
11:48:50 And I

11:48:54  put on the video 
during the session.
11:48:57  Understanding the 
particle of physics
11:48:58  and we do know.

11:49:00  (Audio Difficulties)

11:49:15  Partle physic can 
provide a wonderful
11:49:17  description. 

11:49:18 But we have histories as

11:49:22  well and they come 
along with a list
11:49:25  of questions and 
mental questions in
11:49:27  our feel. 

11:49:28 So cheerly we 
on the search
11:49:30  for new knowledge 
to appear and that
11:49:32  new knowledge will 
guide us to get to
11:49:35  a better understanding 
of particle
11:49:37  physic but it came 
along in Europe,
11:49:40  three strategies 
on the small side.
11:49:43  Particle physics on 
the large side and
11:49:46  Astro particle physics 
and if you
11:49:49  want, in the middle, 
physics. 
11:49:51 So

11:49:53  these are 
community-driven 
11:49:54 strategies

11:49:55  to address these 
open questions and
11:50:03  there after they 
serve as a guidance
11:50:06  (Audio Difficulties)

11:50:11  The research programs. 

11:50:13 Obviously

11:50:14  there are synergies 
between the three
11:50:16  corner. 

11:50:17 And we are exploring this

11:50:19  synergies and we 
strength end the
11:50:21  synergies. 

11:50:21 An example is through

11:50:29  joint seminars between 
-- organized by
11:50:37  those connect the 
field -- physics and
11:50:41  in these seminars 
came along several
11:50:43  examples, for 
example machine
11:50:47  lettering tools and 
dark matter and on
11:50:53  the computer side, 
with the EU escape
11:50:57  project. 

11:50:57 Note that the European

11:51:02  strategy for Bart 
call physics
11:51:05  particle experiments 
in the boundaries
11:51:07  through disciplines 
and through
11:51:08  scientific changes 
and through
11:51:15  technological 
corporations. 
11:51:15 The

11:51:18  accelerator is to 
be upgraded for
11:51:21  that. 

11:51:22 Connected links 
and magnets.
11:51:28  And as we speak...

11:51:33  (Audio Difficulties)

11:51:44  The investment in 
the Spehr meant
11:51:46  enter mental techniques.

11:51:49  

11:51:49 >> Jorgen.

11:51:54  

11:51:55 >> If you put them 
here in the
11:51:59  framework, you can 
achieve with them.
11:52:01  (Audio Difficulties)

11:52:14  In Green what is 
expected to be
11:52:25  achievable -- Jorgegen. 

11:52:27 We are having

11:52:28  a problem. 

11:52:29 People here are 
willing to
11:52:30  run your slide for you. 

11:52:33 If that would help. 

11:52:34 >> I do not hear you.

11:52:36  

11:52:37 >> We have lost 
your slides.
11:52:39  

11:52:39 >> You can still hear me.

11:52:41  

11:52:42 >> Barely it's 
breaking up. 
11:52:43 Maybe if

11:52:44  you quit trying to 
transmit the slides
11:52:47  and let Bo run them 
for you it would
11:52:50  work better. 

11:52:51 >> He can do that. 

11:52:53 You have slide numbers 
and we are on slide
11:52:56  number 10.

11:52:57  I hope you can 
still hear me.
11:53:02  So slide number 10 
-- I can point to
11:53:10  the -- I cannot 
point to the slide
11:53:18  now. 

11:53:19 (Audio Difficulties) Ize

11:53:20  mentioned -- it's 
very difficult. 
11:53:22 I

11:53:23  do not see slide 
number 11 now. 
11:53:26 On

11:53:29  slide number 11 let 
me Zoom into one
11:53:32  particular coupling. 

11:53:33 A year after the

11:53:35  Higgs discovery 
it was estimated a
11:53:37  precision of 7 
to 10% would be
11:53:39  achievable. 

11:53:40 And now a value of better

11:53:42  than 4% seems to 
be reachable. 
11:53:44 And

11:53:44  with only 6 years 
of innovations and
11:53:51  yet we are 20 years 
with that program.
11:53:54  Slide 12, please. 

11:53:55 So that clearly

11:53:56  means and this is 
a very important
11:53:58  sentence in European 
strategy for
11:54:00  particle physics that 
we have explore
11:54:03  the key sector. 

11:54:04 The division is to

11:54:05  prepare for a Higgs 
factory which will
11:54:11  be followed by a 
future head room
11:54:14  collider. 

11:54:14 Sensitivity to energy.

11:54:21  (Audio Difficulties)

11:54:24  An order of magnitude 
higher than
11:54:27  those of the LHC.

11:54:43  You can still hear me?

11:54:45  

11:54:46 >> It's going 
in and out. 
11:54:48 But we can

11:54:49  sort of make out what 
you are saying.
11:54:53  Slide number 13. 

11:54:54 So obviously what

11:54:56  the program that 
is fully embracing
11:54:59  that ambition is kind 
of a big system
11:55:04  program of the LHC. 

11:55:06 It is the FCC

11:55:07  which provides 
a exhibition of
11:55:09  precision with the 
Higgs factory and
11:55:11  there after the 
energy would have
11:55:13  their own collisions. 

11:55:15 Obviously this

11:55:15  is a phenomenal 
ambition and we have
11:55:18  to be prudent of 
course.By have to
11:55:20  plan for success 
and therefore it
11:55:22  means that by around 
2026, which will
11:55:26  be the next update 
of the European
11:55:28  strategy we would 
like to identify if
11:55:31  it is feasible to 
plan for success.
11:55:33  That means on the 
technical side, and
11:55:36  financially 
and the global
11:55:38  governments. 

11:55:39 On the next slide. 

11:55:41 You see what is written 
in the European
11:55:44  strategy that 
Europe should
11:55:45  investigate technical 
and financial
11:55:52  feasibility of such 
a future with a
11:55:55  Higgs factory and 
that it's a possible
11:55:59  first stage. 

11:56:00 And as well, discussions

11:56:03  with potential 
major planners. 
11:56:04 Next

11:56:05  slide, please. 

11:56:06 Obviously you know to

11:56:08  make that happen we 
have to advance or
11:56:10  accelerator the 
technologies. 
11:56:12 And highlighted here 
are four avenues to
11:56:14  make that happen. 

11:56:15 Obviously field

11:56:19  magnets we have Tesla 
and for the high
11:56:24  volume no, sirrity. 

11:56:25 That will be in

11:56:35  310 and on an 
industrial scale. 
11:56:37 And

11:56:37  also in this decade 
nEurope we
11:56:40  continue to strengthen 
our research in
11:56:42  plasma, be it laser 
driven and beam
11:56:45  driven and a 
collaboration for design
11:56:48  studies for the neuron 
collider that
11:56:55  high energies has 
been put together.
11:56:58  We received strong 
regulators in the
11:57:05  EU and the maybe 
from Europe. 
11:57:07 Next

11:57:07  lied. 

11:57:08 This is win in 
the strategy
11:57:11  that the community 
should ramp up with
11:57:18  a focus on advanced 
accelerator
11:57:20  technologies. 

11:57:20 Next slide, please. 

11:57:22 Of

11:57:22  course Europeans are 
and will continue
11:57:24  to remain active 
at the future
11:57:26  colliders elsewhere 
and outside of
11:57:29  Europe. 

11:57:30 Super KEKB is 
an example with
11:57:35  the bell 2 experiment 
but as well the
11:57:41  learn tron-ion 
collider EIC user
11:57:44  community and in 
Japan, the ILC. 
11:57:46 If

11:57:47  there will be a timely 
resignation,
11:57:52  the physics community 
physic community
11:57:54  would wish to 
community. 
11:57:56 You have as

11:57:57  well the density 
frontier where you
11:57:59  see on the left page, 
the temperature
11:58:01  for the energy. 

11:58:03 The chemical

11:58:04  potential or 
the dencity. 
11:58:06 And in that

11:58:09  same space are 
you studying
11:58:13  transition. 

11:58:14 You can do that can

11:58:16  collider experiments 
and mixed
11:58:19  experiment experiments 
and facilities
11:58:22  which will join in 
Russia and as well
11:58:25  as in Germany. 

11:58:27 You see that these 
facilities are being 
11:58:29 built. 

11:58:30 And over the years to 
come -- and certainly in
11:58:33  this decade, 
experiments will be 
11:58:35 taking data and 
analyzing this data. 
11:58:37 Next slide.

11:58:38  Of course you can 
put your detector
11:58:41  very close to the 
region at the LHC
11:58:44  but also put these 
detectors further
11:58:47  away. 

11:58:48 Look for particles 
which is
11:58:52  typically light and 
weekly coupling
11:58:54  particles the 
phase is being
11:58:56  reinstalled and they 
have a variety of
11:58:58  other proposals 
which are being
11:59:01  explored. 

11:59:02 Next slide, please. 

11:59:03 You

11:59:04  can see between the 
collider as well
11:59:07  as these other 
experiments is a clear
11:59:10  Glen tarty which 
is shown here in a
11:59:19  portal reputation. 

11:59:20 Mitigate it

11:59:21  between the 
advancements in the 
11:59:23 hidden

11:59:24  sector. 

11:59:24 You see as well the Axon

11:59:27  arena. 

11:59:27 And on the next 
slide you see
11:59:30  of course that for 
Axxion physics you
11:59:32  can use the structures 
and in
11:59:42  particular older. 

11:59:43 If you want new

11:59:45  magnets and Zooming 
into the space of
11:59:47  models and up to 
the left you see a
11:59:50  lineup of experiments 
put together at
11:59:53  daisy and helps. 

11:59:54 And all of them look

11:59:56  for the contraction 
in a high magnetic
12:00:00  field and the photons 
that will
12:00:02  immerge from that 
will be available.
12:00:04  Next slide. 

12:00:05 Of course there is

12:00:07  physics beyond 
colliders and here you
12:00:11  see a picture of the 
CERN accelerator
12:00:15  complex. 

12:00:16 You see the particles 
go to
12:00:21  the PS and LHCS support 
experiments.
12:00:24  All of the other 
protons are going to
12:00:29  a vast. 

12:00:30 A other Bs. 

12:00:32 Next slide. 

12:00:33 And

12:00:33  if you look on the 
high energy front.
12:00:39  The so problem is 
calling for an SCS.
12:00:41  The lineup for 
dedicated experiments.
12:00:43  They are all reported 
on the collider
12:00:46  studies and I would 
like to highlight
12:00:48  just a few of them. 

12:00:50 Next slide. 

12:00:51 So,

12:00:52  for example in 
the realm of Kaon
12:00:54  physics today we 
have NA62 running.
12:00:59  Look for a charge. 

12:01:01 And in the high 
luminosity, another 
12:01:03 similar,

12:01:04  nevertheless new 
detector would come
12:01:05  online which is clever. 

12:01:07 Which is at

12:01:09  the proposal stage 
as we speak to look
12:01:12  for neutral. 

12:01:13 And on the plot on the

12:01:16  upper front you 
clearly see if you
12:01:23  have new physics 
that is comply men
12:01:25  tridepending 
on the slide. 
12:01:27 Next

12:01:27  slide. 

12:01:28 You can use the 
protons from
12:01:36  the SPS which comes 
at 400Ge V and
12:01:40  after that you put 
an absorber which
12:01:42  you remove the full 
cascades and what
12:01:45  is left are own the 
hidden particles
12:01:48  and if you created 
it you might
12:01:51  capture the decay 
in dedicated
12:01:58  experiments like 
ship or Tau Fv. 
12:02:00 Next

12:02:01  slide. 

12:02:02 These proposals 
are very much
12:02:04  meantry on the Loewen 
give side and
12:02:08  the high energy slide 
with comparative
12:02:10  experiments. 

12:02:10 Neck slide, please. 

12:02:12 So what is mentioned 
in the strategy,
12:02:14  that these experiments 
that offer
12:02:19  potentially impact 
for physics at the
12:02:22  laboratory. 

12:02:22 But as well such

12:02:25  experiments is also 
to be than area
12:02:28  mind. 

12:02:29 Next slide, please. 

12:02:30 An example

12:02:36  is the surge for 
electroparticles like
12:02:39  a proton. 

12:02:40 There's an opportunity in

12:02:43  Germany that you 
can adapt that
12:02:45  storage to demonstrate 
the technology
12:02:47  which will be required 
for that. 
12:02:49 And

12:02:53  the ultimate goal 
would be a dedicated
12:02:56  storage ring. 

12:02:57 So that would have

12:02:58  sensitivity for the 
three orders of
12:03:01  magnitude of what 
we have today. 
12:03:03 Next

12:03:04  slide. 

12:03:05 As well in the 
realm of flavor
12:03:07  physics we can 
look for flavor
12:03:16  violation at 
Switzerland you have the
12:03:25  Meg-II and MU3e 
experiments so you can
12:03:28  cop instruct 3 
electric Rones. 
12:03:30 With

12:03:34  that experiment you 
can improve the
12:03:36  race

12:03:37  Next slide. 

12:03:38 Today we are

12:03:41  accelerating problems 
in the SPS but
12:03:46  we also have problems 
in the ESPS.
12:03:49  You have to have new 
electric cons in
12:03:52  the ESPS and for 
that you can have
12:03:54  accelerated technology 
and after the
12:03:56  acceleration of the 
electric Rones you
12:04:00  can have experiments 
which are
12:04:05  dedicated to dark 
ask light matter.
12:04:08  Next slide. 

12:04:09 So this was at the level.

12:04:12  At the Loewen give 
side which means
12:04:14  pro tones you can 
do great physics.
12:04:17  Next slide. 

12:04:18 You see that you can --

12:04:21  for example do 
precision physics with
12:04:23  antimatter. 

12:04:24 You can decelerate the

12:04:26  protons and the 
antiprotons from the
12:04:29  MEV level to 
the KEV level. 
12:04:31 And you

12:04:32  can measure the 
properties of
12:04:34  antiprotons and 
anti-hydrogen. 
12:04:35 And

12:04:36  the facility that 
will make this
12:04:38  happen in the next 
decade is the
12:04:40  variety of B lines 
to a various active
12:04:45  experiments. 

12:04:46 Next slide. 

12:04:47 As well as

12:04:48  the European source 
in Sweden problems
12:04:52  will be accelerated 
to 2GEV. 
12:04:54 A very high powered beam 
and that will go to
12:04:58  a target. 

12:04:59 Beyond that you will 
have neutrons and with 
12:05:02 these neutrons you can 
do fundamental physics. 
12:05:05 For example you can 
measure or search for
12:05:07  antineutron at scales 
up to 300 meters
12:05:14  and that will help 
you with three
12:05:17  improvements. 

12:05:18 Next slide. 

12:05:19 Of course

12:05:19  with accelerators 
you can also create
12:05:21  the Neutrino Beams 
and this is being
12:05:24  done as you know in 
Japan and the U.S.
12:05:27  and through the 
Neutrino platform.
12:05:36  And Europe is involved 
in LBNF and
12:05:41  dune. 

12:05:42 And RL BC in dune and a

12:05:44  detector or a 
near detector. 
12:05:46 The strategy says we 
have to continue to
12:05:49  support the baseline 
experiments in Japan and 
12:05:51 in the U.S. 

12:05:53 and in particular 
towards the success
12:05:58  implementation 
of LBNF and DUNE.
12:06:00  Slide. 

12:06:01 The three can come with a

12:06:03  variety of energies 
and you can study
12:06:05  them with the a variety 
of distances
12:06:08  and at lower energies 
they typically
12:06:10  come from reactors 
and at short
12:06:12  distances you have 
a reality of
12:06:15  running it this Europe 
and Russia that
12:06:18  will Zoom into what 
existing as a
12:06:20  short baseline and 
they will also
12:06:22  provide us with results 
in the years
12:06:25  to come. 

12:06:26 Next slide.

12:06:30  The Neutrino 
film as well. 
12:06:32 It's

12:06:32  important and the 
KATRIN experiment is
12:06:41  looking for the Trithum 
display, you
12:06:43  see the en pointe 
is very sensitive to
12:06:46  the mouse. 

12:06:47 So by count the number of

12:06:49  electric Rones at 
the end of that
12:06:52  spectrum, you basically 
have a handle
12:06:58  of the Neutrino. 

12:07:00 So you need a vast

12:07:03  spectrometer which 
is being shown here
12:07:05  and being select. 

12:07:07 Don't forget this

12:07:09  is setting up the 
right neutrons.
12:07:11  Next slide. 

12:07:12 There are major 
underground facilities 
12:07:14 in Euro. 

12:07:15 You

12:07:16  see them here 
on the map. 
12:07:18 On the next

12:07:20  slide. 

12:07:21 The first thing 
you can do at
12:07:25  these facilities 
is Neutrino with a
12:07:27  bit of decay. 

12:07:28 We have had a variety

12:07:30  of experiments up 
until now but in the
12:07:33  future we have 
legends and cupid
12:07:35  coming along. 

12:07:36 They all use different

12:07:38  technologies and all 
together they can
12:07:42  March on to halftimes 
of that of '0 to
12:07:45  28 years and that's 
the scientific
12:07:47  discovery. 

12:07:48 The next slide. 

12:07:50 Of course with these 
underground facilities 
12:07:52 you

12:07:52  can put there as 
well dark matter
12:07:58  experiments. 

12:07:59 So on the side of Argo.

12:08:08  Volume with Argo 
and with -- a 200
12:08:11  tonight experiment 
Darwin experiment
12:08:15  and this will provide 
the astrophysics
12:08:19  observatories to reach 
that platform.
12:08:22  So those tend to 
come up in the neck
12:08:25  decade. 

12:08:25 Next slide.

12:08:26  

12:08:27 >> Jorgen you have 
about 1 minute left.
12:08:29  

12:08:30 >> In cosmic particles 
you can
12:08:35  observe them in 
orbit and on the
12:08:37  surface and with 
GTA in the next few
12:08:40  years and on the 
water any are
12:08:42  partially operational 
for high energy
12:08:44  at the next stage. 

12:08:46 Next slide. 

12:08:47 I will be very brief on. 

12:08:50 Thissing of 
gravitational waves were 
12:08:51 mentioned.

12:08:52  Very go in Europe. 

12:08:54 And the flagship

12:08:55  for a decade and a 
decade and a half.
12:08:58  And beyond that 
we have thes a
12:09:01  irrational have the 
aspirations to go
12:09:07  underground in 
a tunnel with
12:09:16  criergenics. 

12:09:16 The fats are being put

12:09:29  together.

12:09:33  Next slide, theory 
is of course a
12:09:36  almost in the backbone 
of particle
12:09:38  physic. 

12:09:39 Of course if you are 
looking for new physics 
12:09:42 will you see emerging

12:09:50  in this decade the 
Wolfe gangpauli
12:09:52  center. 

12:09:53 They stress that 
obviously we
12:09:55  have to continue 
to support the
12:10:01  program of theory 
from the be a track
12:10:03  to fill solve call 
targets and in the
12:10:06  last slide let me 
conclude I presented
12:10:09  in previous 
presentation the vast
12:10:10  portfolio to unlock 
new avenues to
12:10:13  address these open 
questions in
12:10:14  fundamental physics 
and the key
12:10:16  motivation is of 
course to leave no
12:10:18  stone unturned in 
this endeavor. 
12:10:20 And of course as I 
mentioned before.
12:10:23  These strategies 
are now a coherent
12:10:38  basis for funding 
bodies for resource
12:10:40  programs. 

12:10:41 I thank you for 
your attention.
12:10:43  

12:10:43 >> Thank you so 
much, Jorgen. 
12:10:45 That

12:10:46  was wonderful. 

12:10:47 It's an impressive

12:10:48  program. 

12:10:48 I think due to 
the technical
12:10:51  issues we are running 
a tiny bit
12:10:53  behind we started 
late from the last
12:10:55  session. 

12:10:56 So let's jump right into 
the next talk ask we 
12:11:00 will have time for Q&A 
hopefulliful the next 
12:11:02 speaker is Jeffrey 
Taylor at the University 
12:11:05 of Melbourne. 

12:11:06 He is the current 
chair of
12:11:08  Ekfa and a member 
of the atlas bellle
12:11:11  and saber 
collaborations and he 
12:11:13 will tell us about 
the strategy and
12:11:15  planning in Asia 
and the Pacific.
12:11:17  Welcome, Jeffrey. 

12:11:18 Thank you very much

12:11:20  for being here in 
spite of the time.
12:11:25  

12:11:25 >> Thank you. 

12:11:27 Let me just bring you up.

12:11:51  I hope that is 
coming through. 
12:11:53 >>

12:11:53  Yes, it looks great.

12:11:58  

12:11:58 >> Thank you very 
much for this
12:12:01  opportunity to discuss 
the Asia view
12:12:05  of where we are. 

12:12:07 I would like to

12:12:08  start by being perhaps 
a limb bit
12:12:10  controversial by 
really saying that
12:12:12  particle physics 
is not regional. 
12:12:14 So

12:12:14  regional road maps 
are as we know very
12:12:20  highly correlated. 

12:12:22 And the facilities

12:12:23  -- the reason being 
of course is the
12:12:25  large scale facilities 
must be
12:12:27  international and 
interregional. 
12:12:28 So

12:12:29  the facilities are 
chosen and designed
12:12:35  to meet priorities 
of the field. 
12:12:37 So the correlation 
between these road
12:12:41  maps is very, 
very strong. 
12:12:43 So we also

12:12:45  look to what is 
going on in other
12:12:48  regions. 

12:12:49 All funding strategies 
make
12:12:50  references to 
international plans
12:12:52  which is what ties 
theming to. 
12:12:54 It's

12:12:54  true in the Asia 
Pacific too. 
12:12:56 But I

12:12:57  guess the big 
thing -- the big
12:13:01  difference between 
Asia and Europe or
12:13:03  the United States 
is that there is no
12:13:11  unifying structure 
in Asia. 
12:13:13 There is

12:13:15  no union. 

12:13:17 So China and 
Japan with the
12:13:19  dominant players 
with international
12:13:21  scale behind 
the geo physics
12:13:22  facilities but 
there are other
12:13:25  countries, Korea, 
and India, Taiwan
12:13:29  and Australian that 
are clever on the
12:13:31  international program 
and maintain
12:13:33  much smaller national 
programs. 
12:13:34 So we

12:13:38  don't have an 
overriding DOE to run
12:13:43  things and we don't 
have a central
12:13:45  concern to give 
coherence. 
12:13:47 Let's see what happens. 

12:13:48 So the -- first of all

12:13:50  I would like to go 
through some of the
12:13:54  strength of Asian 
particle physics.
12:13:56  And one thing which 
is very clear is
12:13:59  that the Asian 
institutes from across
12:14:01  the board and across 
the countries in
12:14:04  Asia are very good 
participants. 
12:14:06 Very

12:14:07  good collaborators 
on a global
12:14:08  activities. 

12:14:09 And they are

12:14:10  collaborating 
in all the major
12:14:12  particle physics 
experiments. 
12:14:13 But if

12:14:15  we pick out two areas 
where there's
12:14:18  perhaps more 
significance than others
12:14:21  within the Asian 
region I would
12:14:25  highlight flavour 
physics and Neutrino
12:14:27  physics and learn 
more about them
12:14:31  through this talk. 

12:14:33 In Japan, KKB and

12:14:35  bell -- which was 
strongly motivated
12:14:39  and strong competition 
with the U.S.
12:14:42  through baba. 

12:14:43 Has moved on to bill 2.

12:14:46  Which is really 
a leading beef
12:14:49  factory. 

12:14:49 And in China there is --

12:14:56  what start the 
off as BES. 
12:14:58 The

12:15:02  Beijing spectrometer. 

12:15:03 It's now best

12:15:15  of 3 and BEPCII 
and BESII. 
12:15:17 So

12:15:19  Neutrino is rashable 
in Asia. 
12:15:20 There

12:15:22  are remarkable 
experiments where
12:15:27  significant results 
have been
12:15:32  obtained. 

12:15:32 The Daya bay and Reno. 

12:15:35 And

12:15:35  the Neutrino mixes 
with great
12:15:37  precision and aiming 
to do better with
12:15:44  juno in China. 

12:15:45 Of course we will know

12:15:48  about Kamland and 
it's gone to hiker K
12:15:53  and with a much larger 
volume and in
12:15:57  parallel with that 
is the J-Park
12:16:00  extension into a 
high-power proton
12:16:04  source, aiming for 
750 kilowatts. 
12:16:06 And

12:16:10  of course we have 
geoneutrino knows as
12:16:15  well. 

12:16:16 So sorting out 
Neutrinos from
12:16:18  nuclear decays from 
the background
12:16:22  which is also a very, 
very interesting
12:16:24  experiment. 

12:16:25 There are many, this

12:16:28  activity which I 
won't have time to
12:16:32  cover here. 

12:16:33 And there are many

12:16:35  underground experiments 
largely
12:16:38  dominated by dark 
matter researches
12:16:43  but also looking 
for other -- rare
12:16:49  processes. 

12:16:50 So in Japan there's 
XMASS.
12:16:57  China has Panda-X 
and Korea KIMS and
12:17:09  Australia has 
the Za Samier. 
12:17:10 And Look

12:17:13  Telling Underground 
Facilities. 
12:17:14 In

12:17:16  Asian a Couple of 
Laboratories in
12:17:21  Korea. 

12:17:22 The Laboratory 
in China, and
12:17:26  in the Region Several 
Laboratories
12:17:31  Within the Kamioka 
Mine. 
12:17:32 And Down in

12:17:33  Australia Just a 
Few Hours from Here
12:17:35  Is the New SUPL 
Facility Which Should
12:17:41  Be Finished in a 
Year or So just to
12:17:47  broaden it out 
a little bit, the
12:17:50  LHAASO. 

12:17:51 The large high 
at duty air
12:17:53  shower observatory 
in southwest China
12:17:56  is up at 4,000 metres 
and is a massive
12:18:00  array of detectors 
so cosmic rays
12:18:03  clearly being a 
focus as well. 
12:18:05 Just

12:18:08  to look at the 
precision run here.
12:18:15  More about the 
factories in Japan and
12:18:18  China. 

12:18:19 So what started as a very

12:18:21  healthy competition 
again the U.S. 
12:18:23 and

12:18:28  Japan and driven 
by largly trying to
12:18:33  improve the CKM metrics 
to look for
12:18:36  physics beyond the 
standard model, the
12:18:41  precision over the 
years has really
12:18:47  got to incredibly 
high degree of
12:18:51  development. 

12:18:52 And the kick has been

12:18:57  upgraded to super-kick 
and kick B.
12:19:05  And the belle 2 
experiment has been
12:19:10  quickly upgraded 
to handle that. 
12:19:12 So

12:19:13  from Lumme no, 
sirsy from KEKB. 
12:19:15 The

12:19:15  plans were to go by 
another factor of
12:19:19  almost 40 times higher. 

12:19:21 And 50 in

12:19:22  integrated luminosity 
over the next
12:19:25  ten years or So 
so this gives you
12:19:29  some idea of where 
we expect this
12:19:32  integrated luminosity 
it occur.
12:19:34  There's a program 
that stretches out
12:19:37  for the next decade 
or So and you can
12:19:40  see down at the bottom 
in red, it's
12:19:43  going to be -- which 
was already a
12:19:45  significant dataset 
is going to be
12:19:47  multiplied by 50 or 
so which is really
12:19:54  quite a remarkable 
change. 
12:19:56 Of course

12:19:57  the parameters would 
have to be met by
12:20:00  high precision 
so this jump in
12:20:02  luminosity is an 
essential step. 
12:20:03 And

12:20:11  as was mentioned, 
the pack has passed
12:20:18  the record of KEK 
reaching I think
12:20:27  1.22, some weeks ago. 

12:20:29 In BEPC. 

12:20:30 The

12:20:32  BEPC II and BES III 
facility will be
12:20:34  operating for another 
decade and they
12:20:43  will be around 
4Ge -- V where
12:20:46  luminosity will be 
increased by 10.
12:20:49  And the measurements 
will be reduced
12:20:52  considerably. 

12:20:52 So that's going to be a

12:20:59  rather interesting 
area for QCD
12:21:04  contributions. 

12:21:05 So BES III is a major

12:21:07  experiment and it 
has collaborated
12:21:09  across the world. 

12:21:10 And 500 or so

12:21:20  members. 

12:21:21 So it is a major 
facility.
12:21:23  Bell III has nearly 
1,000 rarities
12:21:26  from across the world. 

12:21:27 Just an aside,

12:21:29  the BEPC facility 
was a very
12:21:31  interesting example 
of U.S. 
12:21:32 /China collaboration. 

12:21:33 The machine was large

12:21:39  I will inspired 
by SLAC. 
12:21:41 Wilson suggest they 
had did not go to
12:21:44  Australia to a high 
energy proton beam
12:21:47  at the time because 
it was too
12:21:53  expensive and too 
hard to basically
12:21:57  working with SLAC 
and with the
12:22:06  personal interactions 
of China early
12:22:10  on. 

12:22:11 The development 
of the early
12:22:13  years of BEPC shows 
even between
12:22:15  countries that you 
may not expect too
12:22:18  much collaboration 
to go on, the
12:22:23  scientists can 
breakthrough these
12:22:28  barriers. 

12:22:29 And the BEPC and BEPC III

12:22:31  is a rule of what 
would now seem to be
12:22:35  unlikely collaboration. 

12:22:36 I don't think we would 
like to keep that theme
12:22:39  going. 

12:22:40 So Neutrino physics. 

12:22:41 Of

12:22:43  course there is hyper 
"K" and almost
12:22:52  in Japan. 

12:22:53 China has Daya Bay and

12:22:57  moving into JUNO 
in coming years and
12:23:00  Korea has important 
results out of
12:23:06  RENO and NEOS looking 
at an anomaly
12:23:11  from another sector. 

12:23:13 India has an INO

12:23:14  observatory. 

12:23:15 It's been through a few

12:23:17  numbers over 
the years with
12:23:18  environmental issues 
I think they are
12:23:20  through that now but 
progress is still
12:23:24  being hell up a bit. 

12:23:26 This a magazine tidessed 
ion spectrometer.
12:23:28  And it's an interesting 
idea. 
12:23:30 I

12:23:31  should say Neutrino 
is Japan's
12:23:32  national particle. 

12:23:33 I don't know if

12:23:35  you have a national 
particle. 
12:23:37 So just

12:23:39  a few pictures. 

12:23:41 RENO, again using

12:23:43  these reactors. 

12:23:44 And the results

12:23:53  showed a very nice 
electron with the
12:23:56  Neutrino disappearances 
and consistent
12:24:01  with the well 
measured value. 
12:24:03 And the experiment right 
near the reactor
12:24:07  trying to understand 
the anomaly of
12:24:10  the anti-Neutrino 
spectrum coming out
12:24:19  of the reactors. 

12:24:20 The Daya Bay clap

12:24:26  race is collaboration 
is by China but
12:24:30  has European 
collaborators but looked
12:24:33  for collaborations 
with good precision
12:24:38  and JUNO will step 
up with a major
12:24:41  increase in volume. 

12:24:42 Ask it will have

12:24:46  the capacity of looking 
for Neutrino
12:24:50  hierarchy and can 
good precision. 
12:24:51 The JUNO collaboration 
is also dominated
12:24:55  by China of course 
but it has members
12:24:57  institutes in Europe 
and in the
12:25:02  Americas as well. 

12:25:04 And the JUNO

12:25:06  experiment has an 
unusual choice of
12:25:11  sitting on the absolute 
minimum of
12:25:15  electric Ron and 
Neutrino evens. 
12:25:17 I'm

12:25:19  sure they will be 
most sensitive of
12:25:22  the disappears apps. 

12:25:23 This is a sketch

12:25:30  of what they 
hope to do. 
12:25:32 T2K -- it's been a very, 
very successful
12:25:35  experiment. 

12:25:36 And it's been boosted by

12:25:40  the development of 
the proton machine
12:25:44  and it was recently 
reported that they
12:25:49  are aiming for 750 
kilowatts in the
12:25:51  future. 

12:25:52 When hyper K 
comes in there
12:25:56  will be two massive 
detectors in the
12:25:58  KAMIOKANDE region 
but not exactly the
12:26:01  same as where 
KAMIOKANDE is right now.
12:26:04  And this will improve 
the event rate
12:26:06  quite considerably. 

12:26:07 We will also be

12:26:10  looking at super NOVA 
and proton decay
12:26:13  and other thing as 
all of these big
12:26:16  detectors do. 

12:26:17 There's also the idea

12:26:22  -- I'm not sure where 
it is exactly
12:26:25  right now but putting 
a detector in
12:26:28  Korea and having 
a second detector
12:26:30  underground in Korea 
which will be
12:26:32  very interesting in a

12:26:34  multinational%live 
as well as from a
12:26:36  physics perspective. 

12:26:37 Just to mention

12:26:39  a couple of thing 
in terse of
12:26:42  technology. 

12:26:42 Asia has good technology.

12:26:45  It has technology 
in super conducting
12:26:51  magnets and technology 
obviously in
12:26:55  exercise conducting 
RF but China is
12:26:59  also doing something 
in that region.
12:27:03  Magnets for -- they 
have been provided
12:27:10  to CERN in some 
numbers. 
12:27:12 Including

12:27:14  the D2 correct for 
magnet which the
12:27:18  first prototype has 
painted as being
12:27:24  approved. 

12:27:24 It got through its test.

12:27:28  Also as we all know 
proton detectors
12:27:30  and lots of things 
going on in terms
12:27:34  of technology. 

12:27:35 [ Please Stand By ]

12:30:00  In nonmember states 
with you see that
12:30:03  the big green one 
in the middle is the
12:30:08  U.S. 

12:30:08 is the dominant 
one but there are
12:30:11  Asian members as well. 

12:30:13 Asian users

12:30:14  which are relatively 
significant.
12:30:20  We get on to the 
-- I guess what is
12:30:23  driving in the 
big facilities,
12:30:25  interest in Asia. 

12:30:27 And it was

12:30:29  highlighted in the 
European strategy
12:31:07  highlighted in the 
European strategy update. 
Not only wanting 
to maintain
12:31:07  its strength in 
high-field magnets to push into the energy 
frontier of the future, but the 
idea at least is a
12:31:07  possibility of going 
100 kilometre scale machine and 
using a first stage as a plus or minus 
machine to satisfy
12:31:07  this idea that the 
electron-positive
12:31:10  tron Higgs factory 
is the next
12:31:16  collider. 

12:31:16 The ILC in Japan would be

12:31:18  combatable with 
this strategy and
12:31:22  timely. 

12:31:22 And they would wish 
to clap rate. 
12:31:25 >> Jeff are you close to 
the end of your time.
12:31:29  

12:31:29 >> Of course just a 
couple minutes of this. 
12:31:32 I will push ahead. 

12:31:34 So this is

12:31:35  the dominant 
characteristic of cross
12:31:41  seconds which may 
make a 250Ge V Higgs
12:31:46  factory so exciting. 

12:31:48 Plus to minus

12:31:49  Higgs, plus or example 
the specific
12:31:53  energy on the Z gives 
us the capacity
12:31:56  to generate Higgs 
without being biased
12:32:01  by the trigger 
on the Higgs. 
12:32:03 Why an

12:32:03  Asian Higgs factory? 

12:32:05 Experience with

12:32:11  the plus or minus. 

12:32:13 The KEK and IHEP.

12:32:19  But with that. 

12:32:20 The cost up to 1Tev is

12:32:23  a cleatly different 
beast from 100Te
12:32:27  VPP collider. 

12:32:28 Only being about 1/400

12:32:32  of the energy. 

12:32:34 So it's a much more

12:32:36  manageable machine 
and the footprint
12:32:38  is much reduced 
and its new
12:32:42  technology. 

12:32:42 CEPC. 

12:32:43 The 100-kilometer 
Terwillegar ton sell not 
12:32:45 such an

12:32:49  issue. 

12:32:50 So these things 
both require
12:32:52  international 
collaboration but
12:32:54  neither would drive 
the frontier
12:32:56  threshold and I think 
that's rather
12:32:58  important. 

12:32:59 But no outcomes are

12:33:01  assured so we need 
to develop various
12:33:04  options when you 
support multiple
12:33:05  expertise. 

12:33:06 We need to push where we

12:33:08  can to look for 
additional source of 
12:33:11 funding.

12:33:13  This gives us a plot 
of where we are.
12:33:18  And cheerly the GDP 
in Asia is very
12:33:20  large. 

12:33:21 We must remember 
that a lot of
12:33:23  these countries are 
still developing.
12:33:27  But this is a growing 
portion. 
12:33:29 And

12:33:33  the economic forum 
says by 2030, 6% of
12:33:35  global growth will 
come from Asia.
12:33:37  The point is that 
we shouldn't let
12:33:40  commercial and industry 
drive science.
12:33:42  Particle physics 
has been very
12:33:44  efficient in innovation 
and we must
12:33:46  provide our governments 
-- we must
12:33:48  persuade our 
governments that our
12:33:51  field is much 
more ahead. 
12:33:53 You all

12:33:53  know the two circular 
machines. 
12:33:55 The

12:33:59  FCC in Europe and CPC. 

12:34:01 100 kilometre

12:34:06  scale machines. 

12:34:07 And China is

12:34:09  proposing that it 
builds one itself
12:34:11  but with the machine 
which is chosest
12:34:14  to being approved 
is the ILC. 
12:34:16 The

12:34:18  250ers have of the ILC. 

12:34:20 So I look at

12:34:22  the economies to see -- 

12:34:24 >> Sorry? 

12:34:25 I'm almost finished.

12:34:27  The relative 
size of Japan. 
12:34:28 We

12:34:29  should remember 
is considerably
12:34:31  smaller than Europe 
and general and in
12:34:40  the U.S. 

12:34:41 So that's part 
of the reason
12:34:43  for Japan being 
very, have very
12:34:45  careful about 
its decision. 
12:34:47 The same

12:34:48  number of population. 

12:34:49 126 million

12:34:53  compared with 238 
million in the U.S.
12:34:57  and 700 also in Europe. 

12:34:59 The ILC is a 
multimillion dollars 
12:35:01 machine. 

12:35:02 It's not just a new 
facility in the well
12:35:05  established laboratory. 

12:35:06 It's a well oiled 
machine. 
12:35:08 The community must 
not unestimate the 
12:35:10 significance of the 
undertaking and we must 
12:35:12 have unwavering and 
dominant support for
12:35:14  our feel for these 
to be taken
12:35:17  seriously. 

12:35:17 Is it affordable we

12:35:21  looking at the 
big mac index. 
12:35:23 A $5

12:35:24  billion LHC when 
approved in nine 5
12:35:31  and the big magazine 
big mac. 
12:35:34 I think

12:35:34  it would cost 10 
billion today so a 6
12:35:37  billion price tag 
on the LHC isn't too
12:35:40  bad as long as it 
isn't being shared I
12:35:46  should point out 
that Big Macs cost
12:35:50  less in Japan in 1995. 

12:35:52 So I will be careful. 

12:35:54 This points out -- I will

12:35:57  move straight on. 

12:35:58 I will go to this

12:36:00  quickly. 

12:36:01 ICFA has recently started

12:36:02  the international 
development team to
12:36:04  make preperations 
for the prelab of
12:36:08  the ILC. 

12:36:09 We are aim fog get that

12:36:11  started in 2022. 

12:36:12 In April the

12:36:13  Japanese financial 
year. 
12:36:14 There's an

12:36:18  executive board shared 
by NAKATA with
12:36:21  reputation and in 
conclusion, many
12:36:23  opportunity for 
world-wide particle
12:36:27  physics in Asia exist. 

12:36:29 Conversely Asia science 
contributes greatly to
12:36:31  the international 
field in Europe and
12:36:34  the U.S.A.. 

12:36:35 And the U.S. 

12:36:36 shows that the 
scientific collaboration 
12:36:38 is remarkably resilient 
even in times
12:36:40  when international 
policies are stressing 
12:36:42 and particle physical I

12:36:43  objects must not miss 
the opportunity
12:36:46  presented by the 
Asian century. 
12:36:47 And I

12:36:48  hope that Snowmass 
2020 and the
12:36:51  following P5 will 
reflect on these
12:36:53  opportunities. 

12:36:54 Thank you. 

12:36:55 Sorry I ran out of time.

12:36:57  

12:36:57 >> Thank you very 
much, Jeffrey. 
12:37:00 I

12:37:00  have to be the clapper 
for everybody I
12:37:03  think. 

12:37:03 Because of the time 
we will move on
12:37:06  but I'm sure there will 
be lots of interesting 
12:37:09 questions so 
people please
12:37:11  put in their questions 
in the Q& Our
12:37:14  physical Q&A will 
get shortened to
12:37:16  make up for the 
overage but we can
12:37:21  carry it on 
in the Slack. 
12:37:23 And it's a

12:37:30  real pleasure to 
introduce a member of
12:37:32  atlas and co-chair 
of the physics
12:37:35  long-range planning 
committee. 
12:37:36 Go ahead, Bridget.

12:37:39  

12:37:39 >> Thank you. 

12:37:41 I was just waiting for

12:37:42  the ability to share. 

12:37:44 So you should 
see my slide.
12:37:50  So thank you first 
of all for -- to
12:37:53  the organizer for 
the opportunity to
12:37:55  summarize the ongoing 
activity as was
12:37:57  said for the verifiment 
of the
12:37:59  Canadian sub atomic 
physics long-range
12:38:04  plan covering the 
period 2022-2026.
12:38:06  Indeed I'm presenting 
today in my
12:38:09  capacity as co-chair 
of the long-range
12:38:11  plan committee. 

12:38:12 A responsibility I

12:38:13  share with my colleague 
Adam Ritz from
12:38:24  the University 
of University of
12:38:26  British Columbia

12:38:29  What we mean 
by sub atomic
12:38:31  physicallic in Canada 
means a wide
12:38:35  variety of energy 
skills and
12:38:38  techniques. 

12:38:39 As you can see on these

12:38:41  diagrams on nuclear 
structure to
12:38:43  Neutrino property, 
which in this
12:38:48  particular case, does 
include Neutrino
12:38:50  experiments. 

12:38:51 Collider physics,

12:38:54  particle astrophysics. 

12:38:55 Dark matter

12:38:56  surges, et cetera. 

12:38:58 Now these activities 
-- there's two
12:39:00  organizations that 
promotes and
12:39:02  advocates for these 
facilities. 
12:39:04 The

12:39:04  Canadian research 
of nuclear
12:39:07  physicking. 

12:39:08 And the Canadian

12:39:09  institute of particle 
physics or the
12:39:11  IPP. 

12:39:12 So also provide a bit of

12:39:14  additional context, 
let me also
12:39:18  mention that the 
Canadian sub
12:39:21  community which was 
last surveyed in
12:39:24  2015 consisted at 
the time of 233
12:39:27  grant eligible 
researchers working at
12:39:29  31 different 
universities across the
12:39:33  count interest. 

12:39:34 And at the time, in

12:39:37  2015 approximately 
12% of the
12:39:40  researchers identified 
as women.
12:39:42  Canada is also 
of course host of
12:39:45  world leading 
centers and
12:39:48  infrastructures such 
as triumph and
12:39:52  snow lab and perimeter 
institute. 
12:39:53 Now

12:39:54  the Canadian SAP 
long-range plan is a
12:39:57  plan that is updated 
every five years.
12:40:02  And it's a plan that 
communicates the
12:40:05  sub atomics' community 
inspiration and
12:40:07  identifies promising 
research
12:40:13  opportunities of 
course for Canada.
12:40:15  The overall goal 
of this exercise is
12:40:18  of course to come 
up with a plan that
12:40:25  maximizes the 
Canadian pact. 
12:40:27 We all

12:40:28  know -- and otherwise 
global field has
12:40:32  to do with given 
limited finite
12:40:34  resources. 

12:40:35 To do that the idea is to

12:40:37  build on Canada's 
established strength
12:40:41  and expertise. 

12:40:42 And also we typically

12:40:43  maintain -- and even 
further develop
12:40:46  our worldclass 
domestic research
12:40:48  programs and 
infrastructures. 
12:40:49 The

12:40:52  plan itself has 
historically been
12:40:54  articulated in the 
form that read a
12:40:57  little bit between 
a strategy and a
12:40:59  road map. 

12:41:00 And I thought it was

12:41:02  important to mention 
that unlike in
12:41:07  the U.S., while the 
long-range plan
12:41:09  report presenting 
the community's
12:41:10  priorities it does 
not actually
12:41:13  dictate what gets 
funded or not. 
12:41:15 Our

12:41:16  funding agency still 
traditionally
12:41:23  holds broad funding 
competition. 
12:41:25 The

12:41:27  record is also used 
to communicate to
12:41:32  national stakeholders 
and our own
12:41:33  makers. 

12:41:34 And the plans in the

12:41:36  community and as 
you can imagine the
12:41:38  resources requirement. 

12:41:39 The one additional part 
I wanted to mention is
12:41:43  also -- even for us 
in Canada, beside
12:41:46  the actual final report 
and the final
12:41:49  product, the actual 
planning process
12:41:50  is an extremely 
valuable exercise for
12:41:53  the community to 
essentially take
12:41:54  stock of where it 
stands and to help
12:41:58  further -- I would 
argue, develop ties
12:42:00  among various 
researchers.
12:42:07  So on flag 5 I'm 
presenting here
12:42:10  Some background 
information for the
12:42:13  LRP process but the 
long-range plan is
12:42:16  commit commissioned 
by Canada's
12:42:21  planning agency 
NSERC and the
12:42:28  institute for particle 
physics physics
12:42:31  and CINP and the 
scope is to look at
12:42:34  the horizon of 15 
years or So but the
12:42:38  plan itself would 
be active for a
12:42:40  period of five years, 
starting in
12:42:42  2022. 

12:42:43 Now needless to 
say that given
12:42:46  the global nature 
of sub atomic
12:42:48  physics, of course 
this Canadian
12:42:50  planning process is 
informed by other
12:42:52  similar planning 
processes around the
12:42:54  world. 

12:42:55 Most of which 
actually we are
12:42:57  hearing about today, 
which is nice.
12:43:01  On slide 6 I present 
here some
12:43:05  additional information 
about the
12:43:07  organization. 

12:43:08 The planning process is

12:43:12  actually organized 
and coordinated by
12:43:13  the long-range plan 
committee which is
12:43:16  made up of 12 members 
as you can see
12:43:19  on the left table. 

12:43:20 Four of which are

12:43:22  international members. 

12:43:23 We also have a

12:43:25  number of exofficial 
and observer
12:43:27  members who represent 
-- for example
12:43:30  funding agencies 
and national
12:43:31  institute. 

12:43:32 I thought I would also

12:43:36  mention s a an aside 
that -- as part
12:43:42  of the U.S. 

12:43:43 NOMAS process and Canada

12:43:50  has one advisory 
on the group.
12:43:54  Heather Yolten provides 
us with the
12:43:56  U.S. 

12:43:57 process. 

12:43:58 So while given the time

12:43:59  I wasn't planning 
to go into the
12:44:02  details of the mandate 
of the LRP
12:44:04  committee. 

12:44:05 I wanted to, however,

12:44:06  point out that the 
mandate is broader
12:44:09  than just addressing 
the scientific
12:44:11  opportunities and 
resources needed to
12:44:14  follow up on these 
opportunities. 
12:44:16 The

12:44:17  mandate also includes 
reporting on
12:44:27  issues of equity, 
different and
12:44:31  diversity and 
inclusion. 
12:44:32 Topics that

12:44:33  are of primary 
importance for our
12:44:38  community to thrive. 

12:44:40 On slide ago I'm

12:44:41  showing here the 
timeline and a bit
12:44:43  more detail about 
the actual process.
12:44:47  Is the So the Canadian 
planning
12:44:49  process is a community 
driven process.
12:44:57  And it take place 
in a year. 
12:45:00 The current planning 
process was this past
12:45:02  June. 

12:45:03 At which point the June

12:45:05  timeline parked a 
point in which the
12:45:09  IPP and CINP have 
been busy working on
12:45:11  the preparation of 
the brief due to be
12:45:14  submitted to the LRP 
committee at the
12:45:17  beginning of December. 

12:45:18 Meanwhile this

12:45:19  fall the LRP committee 
has become
12:45:23  busy. 

12:45:23 In particular 
in preparing a
12:45:25  community-wide survey. 

12:45:26 And also

12:45:27  gathering various 
types of data that
12:45:30  will be valuable 
for the formulation
12:45:35  of its recommendation. 

12:45:36 The plan is

12:45:38  that at the beginning 
of the new year,
12:45:41  probably around 
February, we plan to
12:45:46  hold approximately 
six topical mini
12:45:48  town meetings to 
further gather inputs
12:45:50  from the community 
but those will be
12:45:53  topical meetings to 
gather information
12:45:55  and discussion very 
speck topics that
12:45:59  will have bubbled 
up and come up with
12:46:03  the activities ongoing 
since June.
12:46:05  Final general town 
hall meeting is
12:46:08  then planned around 
April next year.
12:46:11  Followed by men 
a presentation of
12:46:20  draft recommendations 
in June of the
12:46:23  actual report will 
be completed next
12:46:27  year and you can see 
there is various
12:46:30  opportunities for the 
committee to participate 
12:46:32 in this planning 
process. 
12:46:34 Now throughout this 
process, one of
12:46:36  the things that I 
want to emphasize is
12:46:39  we also want to 
make sure to reach
12:46:41  tout to young 
physicists and really 
12:46:43 hear their voices 
and their opinion
12:46:46  and their thoughts 
and their
12:46:47  suggestions. 

12:46:48 So if you are interested

12:46:50  in general in keeping 
informed about
12:46:52  the Canadian planning 
process and in
12:46:54  particular how to 
participate in the
12:46:57  upcoming events 
such as those I
12:46:59  highlighted I encourage 
you to go to
12:47:03  the web page that 
is listed here. 
12:47:05 And we can add your 
name to the mailing
12:47:11  list in order 
to keep and stay
12:47:14  informed. 

12:47:14 So in summary 
Canada is in
12:47:17  the mid-of a long-range 
planning
12:47:19  exercise that will 
culminate in a
12:47:21  final report available 
September of
12:47:23  next year. 

12:47:24 As I mentioned earlier

12:47:26  this is a 
community-driven process 
12:47:27 and

12:47:28  there are several 
ways through which
12:47:31  you can participate. 

12:47:32 And in

12:47:40  particular we invite 
all interested
12:47:42  individuals to join 
the list and stay
12:47:45  informed about the 
upcoming events so
12:47:47  thank you for 
your attention.
12:47:49  

12:47:49 >> Thank you so 
much, Bridget and
12:47:51  being very precise 
and take making
12:47:53  time to come talk 
to us today. 
12:47:56 We will move on right 
away to the next
12:47:59  talk sky understand 
you will be
12:48:01  available for Q&A 
on the Slack after.
12:48:04  

12:48:04 >> Yes. 

12:48:05 >> Thank you 
so much again.
12:48:07  Our next -- it's 
a pleasure to
12:48:11  introduce Rosario 
Rosenfelt from the
12:48:22  University of Somfhalo. 

12:48:24 He is from

12:48:25  the group of Latin 
infrastructure in
12:48:27  America. 

12:48:28 And he will be tenning 
you about the plans in 
12:48:31 Latin measure. 

12:48:32 >> Thank you so much 
for the opportunity.
12:48:35  To talk about this 
community planning
12:48:37  meeting. 

12:48:38 I'm talking on 
behalf of the
12:48:40  group of this Latin 
American forum for
12:48:48  research and 
infrastructure. 
12:48:49 Which we

12:48:52  call EHCAP. 

12:48:53 So this the web page you 
can find most of the 
12:48:57 information regarding 
this process. 
12:48:58 And you are welcome 
to visit this page. 
12:49:01 And I just want to 
stress that this is the
12:49:05  first time that 
a strategy process
12:49:07  like that is conducted 
in Latin
12:49:09  America. 

12:49:10 And we are planning this

12:49:11  time frame for the 
strategy from 3 to
12:49:14  5 years. 

12:49:15 That's the first time 
we want to revise it. 
12:49:18 So brief timeline

12:49:21  for this effort. 

12:49:23 Which we call

12:49:24  LASF4RI. 

12:49:24 Research for structures.

12:49:28  Under the HECAP part. 

12:49:30 We started with

12:49:32  brainstorming in 
the community.
12:49:37  SILAFAE. 

12:49:37 It's a binary 
symposium for
12:49:39  binary physics that 
actually is the
12:49:42  thing that bringing 
to our community
12:49:47  in Latin America so 
the general is in
12:49:54  November 2016. 

12:49:55 And the year 2017 and

12:49:57  2018 was brief 
experiments and also
12:49:59  gathering support 
from national
12:50:01  communities. 

12:50:01 In October 2018

12:50:03  something very 
important happened
12:50:07  which was the Irb 
aboutero-American
12:50:09  ministerial science 
and technology
12:50:11  meeting in Guatemala. 

12:50:12 That's where we

12:50:15  have a mandate. 

12:50:16 We have a mandate

12:50:21  from here in order 
to plan -- make the
12:50:24  strategy planning. 

12:50:25 So it comes from

12:50:26  this institution. 

12:50:27 In November 2018 we

12:50:30  had a town hall open 
to everybody at
12:50:37  the -- again at X 
III SILAFAE in Peru
12:50:41  to discuss the next 
steps and in 2019
12:50:44  we had preparatory 
group. 
12:50:45 We

12:50:46  established a 
preparatory group that
12:50:48  celebrates from ten 
countries in Latin
12:50:53  America. 

12:50:54 And we hell our first

12:50:58  workshop and also 
the first meeting.
12:51:05  And I say safer 
in -- for south
12:51:08  Americans doing 
fundamental research
12:51:09  and I want to also 
stress in this
12:51:12  meeting some members 
of the global
12:51:14  research council 
participated. 
12:51:15 And

12:51:17  then in may, June 
2019 we had the
12:51:21  meeting of the high 
level strategy
12:51:23  group. 

12:51:24 Sorry the definition 
of the
12:51:25  high level strategy 
group which I'm
12:51:28  going to talk 
about later. 
12:51:29 And then

12:51:30  we issued a call 
for white papers to
12:51:33  contribute to 
this effort. 
12:51:35 And the

12:51:35  deadline for the 
submission of the
12:51:39  white papers was 
December 2019. 
12:51:41 We

12:51:43  have almost 40 papers 
submitted. 
12:51:45 And

12:51:46  July of this year 
we held an open
12:51:53  virtual symposium. 

12:51:54 It was supposed to

12:51:57  be with ICTP-SAIFR. 

12:51:59 In March it was

12:52:00  delayed due to 
the pandemic. 
12:52:02 And now

12:52:04  we are doing a writeup 
of the physics
12:52:06  briefing book 
and the strategy
12:52:08  document that will 
be submitted to
12:52:10  high level strategy. 

12:52:12 So in this

12:52:13  process we have 
an idea now of the
12:52:16  landscape in high 
energy cosmology
12:52:18  Astro particles 
in Latin America. 
12:52:20 So

12:52:22  we estimate roughly 
at around 1,000
12:52:27  physicists HECAP 
in the region. 
12:52:29 I

12:52:30  will show you now 
a figure of the
12:52:33  landscape. 

12:52:33 So I started 
the countries
12:52:35  that we mapped out 
so those are the
12:52:38  countries that are 
involved in this
12:52:41  initiative. 

12:52:42 And here you can see the

12:52:45  high energy nuclear 
experiments that
12:52:48  the community is 
involved with. 
12:52:50 So

12:52:53  mostly LHC but future 
colliders here
12:52:55  are the Neutrinos 
and dark matter
12:52:57  experiments that 
communities involved
12:53:03  with. 

12:53:04 So there are 
many of these
12:53:11  experiments. 

12:53:12 Some are located in the

12:53:17  region. 

12:53:17 Also in the region. 

12:53:19 So these

12:53:20  are the three main 
areas that we are
12:53:23  focusing on now. 

12:53:25 So high energy and

12:53:26  Astro particles 
and cosmology. 
12:53:28 And

12:53:28  now the connections 
are kind of messy.
12:53:30  So these are the 
connections that
12:53:33  each country has 
groups working with
12:53:35  different experiments 
so this is
12:53:36  depend in the high 
energy nuclear
12:53:39  Neutrinos. 

12:53:40 So the type for the

12:53:42  organization so 
these are the
12:53:44  connections of 
each country with
12:53:49  different experiments 
and also in
12:53:51  cosmology and Astro 
particles so as
12:53:53  you can see it's 
a very rich and
12:53:57  complex landscape. 

12:53:58 And I think some

12:53:59  coordination 
can be useful. 
12:54:01 So we are

12:54:02  finishing up the 
writing of this
12:54:04  physics briefing book. 

12:54:05 It's based on

12:54:06  40 submitted white 
papers and these
12:54:12  are the members 
of the preparatory
12:54:14  group, as you 
can see here. 
12:54:16 And when

12:54:19  this is final we will 
put this in the
12:54:30  archives and. 

12:54:31 Just an idea. 

12:54:32 Astro

12:54:35  Ass trophies idea. 

12:54:36 astrophysics. 

12:54:37 So

12:54:37  those are the main 
chapters in this
12:54:40  briefing and just 
a few highlights of
12:54:42  what I learned 
at least. 
12:54:44 So those are

12:54:45  my personal picks. 

12:54:47 It has nothing to do 
with the preparatory 
12:54:50 groups my personal picks 
so we have of course in
12:54:56  the region the Auger 
Observatory. 
12:54:58 The success story 
in the region. 
12:55:00 We have

12:55:07  developed new 
technology for the
12:55:10  liquid Aragon 
scintilation Ariapuca
12:55:13  adopted in DUNE and 
full development
12:55:19  for new 
front-enread-out. 
12:55:20 And a lot

12:55:23  of things in the 
region Neutrino/DM
12:55:27  detectors and there 
is a southern
12:55:29  wide-field view 
gamma-ray answer
12:55:31  sorry. 

12:55:32 So this is built 
on the hot
12:55:35  experience in Mexico 
for MRAs and also
12:55:37  the possibility 
-- this is very
12:55:39  exciting of an 
underground facility in
12:55:43  the region called 
ANDES in the slides
12:55:46  with give but this 
is not approved
12:55:48  yet. 

12:55:49 So it's a very exciting

12:55:57  possibility. 

12:55:58 Finally, we are

12:55:59  developing a strategy 
document. 
12:56:01 In

12:56:01  this document 
we have ten
12:56:05  recommendations that 
are going to be
12:56:07  submitted -- were 
submitted to the
12:56:09  high level strategy 
group. 
12:56:11 Here you can see the 
members of the high level
12:56:14  strategy group. 

12:56:15 This group is chaired

12:56:24  by Luciano Miani and 
Fernando Quevedo.
12:56:28  And representatives 
from around the
12:56:32  worm. 

12:56:33 And a representative 
of the
12:56:35  advisory group. 

12:56:36 Next steps October

12:56:37  20th a meeting 
of the high level
12:56:40  strategy group. 

12:56:41 And they are going to

12:56:43  go through the document 
-- strategy
12:56:45  document that was 
submitted to them.
12:56:47  And October 27th there 
is going to be
12:56:50  this meeting of 
the Ibero-American
12:56:52  ministers of science, 
technology and
12:56:54  innovation. 

12:56:54 This meeting here and

12:56:56  again we have a mandate 
interest them.
12:56:58  So we have to report 
our progress to
12:57:01  this meeting. 

12:57:02 So this is all I have

12:57:04  to say. 

12:57:05 Thank you very much.

12:57:14  

12:57:14 >> Thank you very 
much, that was very
12:57:17  interesting and keeping 
us on time.
12:57:19  So we will save 
questions to the end
12:57:22  and move right awatt 
to last talk
12:57:25  which is professor 
Shavanka. 
12:57:27 The

12:57:33  Center for Fundamental 
Physics Zewaii
12:57:35  City of Science 
Ask Technology in
12:57:40  Europe. 

12:57:41 A member of the African

12:57:45  strategy and I can 
say he is both a
12:57:50  theorist and 
fundamentalist at IRF.
12:57:52  Thanks for being 
with us.
12:57:53  

12:57:54 >> Thank you very 
much and thank you
12:57:57  very much for the 
opportunity. 
12:57:58 I will discuss -- in 
fact Africa and the
12:58:02  middle east we do 
not really have a
12:58:04  strategy yet. 

12:58:05 We started in this --

12:58:07  as I will mention 
but at least I will
12:58:10  show you the activity 
that we have in
12:58:13  our region and all 
through the country
12:58:17  involved and I will 
give you overview
12:58:25  about this. 

12:58:26 So essentially Africa and

12:58:28  the middle east they 
have several high
12:58:31  energy physics 
activities. 
12:58:32 In

12:58:33  particular with LHC. 

12:58:35 There is

12:58:38  involvement in CMS 
collaboration and
12:58:41  ATLAS collaborations 
and ALICE and
12:58:43  other experiments 
and collaborator
12:58:45  experiments and of 
course theory for
12:58:47  particle physicallics 
and cosmology
12:58:50  and astrophysics 
as you will
12:58:57  -- as you will see.

12:59:00  As we said we don't 
have the strategy
12:59:03  for the countriesing 
to and in fact it
12:59:06  is initiated by a 
group of citizens to
12:59:11  set some strategy 
for Africa. 
12:59:13 For

12:59:13  physics and high 
energy physics in
12:59:16  particular. 

12:59:16 And it started to do so

12:59:18  under the umbrella 
of African fiscal
12:59:25  society. 

12:59:26 And I hope that 
by June or
12:59:29  October 2021 we 
will have some
12:59:32  documents for 
this strategy.
13:01:33 Machine learning,

13:01:36  which is quite a hot

13:01:37  topic

13:01:39  nowadays,

13:01:47 Secondly country involved

13:01:48  is turkey.

13:01:53  Turkey has been 
involved in this
13:01:55  business

13:01:55  since

13:01:57  1961 as an observer 
country
13:02:04  and then in 2015, 
became one of the member 
13:02:06 states. 

13:02:07 They have large 
numbers of
13:02:08  members involved 
in certain
13:02:11  -- concern

13:02:14  C

13:02:14 ER

13:02:15 N

13:02:20 . 

13:02:20 Again, they are 
also involved
13:02:22  with

13:02:23  Argonaut physics 
analysis
13:02:26  and also

13:02:29  B physics and so on.

13:02:35  And also in addition to 
this, they are involved
13:02:40  in the technical physics

13:02:41  at

13:02:44  Hg Cal and the 
prototypes systems.
13:02:50  This is also

13:02:52  a big country 
involved in CMS.
13:02:56  Another big country 
involved in CMS is 
13:02:58 around.

13:02:59  They joined since 2002

13:03:03  -- Iran. 

13:03:04 They joined since 2002

13:03:06  and they are 
also involved
13:03:08  in an

13:03:10  RBC group

13:03:11  like

13:03:12  Egypt

13:03:13 .

13:03:17  Like other groups, 
they are doing
13:03:19  organ metaphysics

13:03:23  -- (unknown term) 
metaphysics
13:03:24  analysis

13:03:25 .

13:03:32  We have another 
country, Cyprus in CMS.
13:03:36  It is not Africa, 
it is Middle East.
13:03:39  They

13:03:39  are a member

13:03:41  in CMS

13:03:43  and they are

13:03:44  involved

13:03:45  in collaborating

13:03:46  in different aspects

13:03:49  and also different 
subjects of physics.
13:03:51  Physics analysis

13:03:54  and (inaudible) physics

13:03:57  LS GC.

13:04:01  Small countries 
recently joined like 
13:04:02 Lebanon for example.

13:04:03  They just joined

13:04:04  a couple of years ago

13:04:09  and they are 
starting with
13:04:13  a few numbers of

13:04:16  students and supporting 
engineering and so on
13:04:18  and I think we 
are encouraging
13:04:22  all the big and 
small countries
13:04:24  to be involved

13:04:25  in this collaboration

13:04:28  and this has created a 
kind of match work in 
13:04:31 fact collaboration

13:04:32  between the regions.

13:04:34  Now we move

13:04:37  to the ATLAS 
collaboration
13:04:42  which is one of the big

13:04:44  experiments

13:04:44  at

13:04:46  (inaudible).

13:04:47  At ATLAS

13:04:48 , we have

13:04:49  turkey.

13:04:54  Turkey is also involved 
in the ATLAS experiments
13:04:58  and

13:05:00  during the data taking 
of the detectors
13:05:03  and

13:05:06  Turkey was involved 
with even 100 institutes
13:05:09  so they are really doing

13:05:10  a good job

13:05:12 .

13:05:18  From the Arabic region,

13:05:20  Egypt

13:05:21  and

13:05:24  CMS and

13:05:26  ATLAS.

13:05:29  (unknown term) has 
about 22 physicists
13:05:31 ,

13:05:35  22 PhD students 
and 10 Masters.
13:05:41  It includes physics 
as usual, detector or 
13:05:43 operation, commuting, 
detector performance
13:05:45 , machine learning 
and so on
13:05:49  and also updates 
for the machines. 
13:05:51 This is the typical 
involvement
13:05:54  of all reasonable 
big institutes
13:05:56 .

13:05:58  Israel is also in ATLAS

13:06:00  and in fact

13:06:01 ,

13:06:03  they are the first 
non-European
13:06:05  CERN

13:06:09  member states and they 
have four ATLAS groups
13:06:12  and they provided me 
with this information
13:06:14 . 

13:06:15 About 15 staff members

13:06:19  as well as postdocs, 
engineers and 
13:06:21 technicians are involved.

13:06:22  They are also involved

13:06:23  in different aspects

13:06:24  of physics

13:06:25  analysis

13:06:26  and machine learning

13:06:31 . 

13:06:32 So this is

13:06:35  South Africa. 

13:06:36 They are a big country 
involved in
13:06:38  ATLAS

13:06:39  and ALICE.

13:06:44  Again, this is quite 
big and strong groups 
13:06:46 involved in this 
collaboration.
13:06:49  Other activities like

13:06:50  ALICE

13:06:51  and

13:06:52  AMS

13:06:53  02

13:06:57 , Turkey is involved 
in this experiment.
13:07:01  And also more important 
now, Turkey is involved 
13:07:04 within FCC

13:07:04 , which is the

13:07:06  future circular collider

13:07:08  which we hope

13:07:12  will give us a large 
scale for detecting 
13:07:14 (inaudible). 

13:07:15 Israel is also involved

13:07:16  with other experiments 
like
13:07:18  Bell to

13:07:23  and

13:07:26  (inaudible) for 
neutrinos and so on.
13:07:31  We also have 
(inaudible) involved in 
13:07:33 (inaudible) physics.

13:07:36  Then Egypt has 
a large group
13:07:37  of involvements

13:07:41  in different aspects 
of particle physics
13:07:43  and also quantum 
gravities
13:07:46  and astrophysics.

13:07:49  The same for (unknown 
term). 
13:07:51 I think Turkey 
is also the same
13:07:53 .

13:07:54  -- The same for Morocco 
and I think
13:07:56  Turkey is also the same.

13:07:59  Big countries like 
Egypt, Morocco, Turkey
13:08:02  and South Africa.

13:08:05  And that's it

13:08:09  for this virtual time. 

13:08:11 And as I said,

13:08:12  I will bind your 
will really have
13:08:18  a well-defined strategy

13:08:22  for building 
collaborations
13:08:24 . 

13:08:25 Thank you very much.

13:08:30  

13:08:31 >> Thank you very much. 

13:08:33 That was wonderful. 

13:08:34 I'm happy to know about 
all that activity
13:08:36  which I hadn't really 
appreciated before. 
13:08:38 There's only a couple 
of minutes and I was 
13:08:40 looking at the questions 
that came in on the Q&A.
13:08:43  There were several 
about the ILC.
13:08:45  One of them got answered

13:08:48  by Joanne on Slack

13:08:49  but

13:08:50  I wanted to ask

13:08:53  if Taylor would 
like to come in
13:08:55  on that

13:08:56  summer couple of them.

13:08:57  Another question

13:09:00 , while he's getting 
organized
13:09:01 , that came up

13:09:02  was for South America

13:09:04 .

13:09:05  What is the end days

13:09:07  and tell us more 
about Andy's
13:09:11  and what is the 
prospects for the 
13:09:13 funding.

13:09:17  

13:09:18 >> This is Geoff

13:09:21  and I can't see the 
question though.
13:09:23  

13:09:24 >>

13:09:25  They were just 
generally, what's the 
13:09:27 status?

13:09:31  There a couple of 
variance on it, but why 
13:09:34 don't you just give 
us a run-down. 
13:09:36 >> Sure. 

13:09:37 So one slide which I 
went to rather quickly
13:09:39  which shows 
some progress
13:09:41  is that

13:09:43  (unknown term) has 
established what's called
13:09:46  the ILC international 
development team.
13:09:47  And like team

13:09:49  is charged

13:09:54  with preparing for 
the ILC pre-lap
13:09:57  which is a four-year 
period
13:10:00  before construction 
starts
13:10:02  where final questions

13:10:04  are being sorted out

13:10:06  on R&D

13:10:08  and some of the 
technical work.
13:10:11  And also governance 
structures are set up
13:10:16  and there's time to get 
international funding 
13:10:18 and so forth.

13:10:20  So IDT, this 
international 
13:10:21 development team that has

13:10:23  taken about a year and 
1/2 or so to work,
13:10:26  there is no guarantee

13:10:27  that the work of the IDT

13:10:29  will result in funding 
for the prenup.
13:10:31  But we are somewhat 
encouraged right now
13:10:35  that we will continue 
to make progress.
13:10:40  

13:10:40 >>

13:10:43  OK, thank you 
very much. 
13:10:45 We are able to 
end on time.
13:10:47  There is now 15 minute 
break and we will resume
13:10:51  at 1:25 central time

13:10:52  with

13:10:53  Fiona Harris

13:10:57  in talking about the 
(unknown term) 2020.
13:10:59  Thanks to all the 
people in the session.
13:11:06  

13:11:06 >>

13:11:09  I can answer the 
question about Andy's
13:11:11  if you want. 

13:11:13 >> Sorry?

13:11:13  

13:11:14 >> I can answer 
the question
13:11:15  about Andy's later

13:11:16  if you want.

13:11:17  

13:11:18 >>

13:11:20  Right, right. 

13:11:21 Sorry about that.

13:11:25  

13:11:25 >> The broadcast 
is still going.
13:11:34  

13:11:35 >> Do I do anything? 

13:11:37 I guess I should 
stop my video.