field.
They recover to the P5 plan
they like the idea in a they have a
plan where there's no disagreement.
So I think we can Pat ourselves in the
back about.
That I think we have to
repeat it in the future.
I even have other countries coming to me
and asking me how dough do our planning
process now.
So the word is out --
not just in the U.S.
but around the
world.
And our reputation as a field.
The is being Paul talks about it a
lot in his travels and I think a lot
of that again goes back to the P5 plan
and how well it's been received by the
administration of so I just encourage
everybody to have a good meeting and
keep in mind what they are trying to
do is have a good plan and get on the same page
and work tock for the next one.
Thank you very much.
>> Thank you very much, Nigel for the
words of encouragement.
We will take them to heart.
At this moment I would
like to turn over the session to our
stallword local organizers.
Bo in and
Brenda Taggart.
>> Krista Young-Kee
is next.
>> Okay.
>> Let me
introduce.
Young-kee who is our
current chair of the division of
particles and field.
>> Thank you, Priesca.
You can hear
me okay?
I assume So it's not muted.
So I will briefly discussion goals of
the community planning meeting CPM.
And preliminary known as timeline and
report structure.
Just a reminder --
You heard from Nigel but I want to
give you an example of strategic
planning.
It start with a
community-wide science study.
We
define the most exciting and important
questions for the field and identify
promising opportunity to address them.
Organized by DPS, division particles
and fielding to with other division,
physicallics and nuclear physical I
objects and physics of beams and this
is followed by another process called
the P5 project panel, that formulates
the exclusion plan in a vision of 20
years in a global context.
Last one
took place in 2012 and 2013 followed
by P5 in 2014, we are doing 2020 and
2021.
And next year there will be P5.
Particle physics is global.
And now involves community strong
engagement
and use our plans Ann input to
analysis and we are not isolated.
As
I said earlier we will be working
together with -- hour colleagues from
other divisions.
And as accomplish Canada mentioned,
-- as priss Canada mentioned I would
like to thank priss Canada that
chaired -- Prisca prepared it.
It's
not one team does all.
It's the team
working together to do our Snowmass
process.
Again together with the
other divisions.
There are
leaderships shown there.
So this is
the snow mass steering.
And we have
an advisory group and in addition to
steering group members we have the members from
the executive committee and editor and
communication and also
in addition we have seven
representatives from international
communities.
I would like to take
this opportunity to give our special
thanks to international
representatives.
They have been
important to our process.
We have
large leaderships.
Conveners and
career liaisons and early career
liaisons and this is all thank to the
community for your nominations and
these people -- sorry.
(phone ringing) And chosen primarily
on the outcome of nominations
nominations nominations and outcomes.
And today we have 30 enter developers
you will hear from them the key
questions in their frontier so far.
Outbreaks of sessions and the plans
and steps between now and summer study
next year.
There's a weekly page
known as 21.org which is a one-stop
shop.
You have all the information
related to Snowmass.
You can find that.
And we hope to have you visit
as often as possible.
We are also
very delighted that there is strong
engagement from the career process.
All community members should feel safe
and supported in exchanging ideas
through this process.
So we formed
the ethics task force early this year
and they produced the four principals
and community guidelines and also was
a team for this week's meeting.
We
currently establishing an ethics
committee, that no real members will
be announced early November this year.
The Snowmass timeline, especially the
community-wide get together.
We
started a meeting in April this year
at the APS April meeting.
Now we have
four days of a planning meeting.
And
we are planning to have another small
get together.
April meeting neck year
but finally a ten-day long workshop --
again involving all the community.
So
to prepare this week's meeting, I have
received many -- in fact more than
1500 letters of interest from our
community.
Our frontier communities
spend a lot of time understanding and
analyzing to prepare the bottom -- the
class shows that when they were
submitted -- Not surprisingly, 28
hours, also the day before, from the
deadline we have most otherwise
received and also you will notice that
there are many covering different
types of groups and different
frontiers.
Showing really
interconnected the areas of research.
For this week's meeting, because they
have been already a popular group and
have been already a popular group and frontier groups having had their own meetings and workshops.
Therefore, this week when we have this opportunity to bring together the
community across the field we would like to he to cuss on more interpreting discussions and also to
establish a cross-work group connections. At the same time, we
would like to identify gaps and areas to focus or for further studies. And
also to brainstorm new ideas. And planning sessions will hear about
excitement about the field and plans from other regions and related fields
and messages from funding agencies and
voices of community.
So overall our
goal this week is to produce -- plan
the steps to take between now and the
Snowmass summer study next year.
Leading to a final report in October
of 2021.
So after the -- this week
there will be a lot of effort
throughout the groups and frontier,
understanding what further studies are
to be done and what kinded of papers
could be produced.
I saw a lot of
discussion happen.
And between --
around the end of this year to
February/March we could like to have a
couple of rules developing key
questions and opportunities.
And
February to March, April time, popular
groups producing outlines of their
reports.
Finally April to June time,
preliminary matter frontier report.
You will see that each one we had a
range of a few months because group to
group, they may have decided different
plans and timeline.
Also ways of
getting people from the community.
Solve there will be enough flexibility
in that.
So for the summer study
time, our goal is to build a consensus
on key questions and opportunities of
the entire physics field and enabling
technologies and community engagements
engagements and to form late the
compliment of Snowmass executive
summary and after the CS weS we have a
report by the end of October.
This is a starting point for discussion.
We would like to get more feedback this
week.
Concerning the core structure,
our thinking plan is to use the 2013
Snowmass with a summary.
With a few pages from frontier summary.
And then
we will have the frontier report, that
itself will start with the frontier
summary and popular report and they
will be used as references.
Again
this is something we would like to get
feedback for you this week.
Thank you
I would like to thank our program
committee for CPM.
Presented to other
careers and chairs of the local
organizationing committee.
In
particular all frontier has a
committee and members have done an
incredible job to organizing very
nontrivial breakout sessions.
And of
course a special, special thanks has
to go to our local committee.
Thank
you very much.
And next one will be a
report from the local organizing
committee.
>> Sorry for reversing the order of
the two.
But thank you, Young-Kee for
getting us on the path now and for
details of this week's festivities, if
you like.
We will listen to Bo and Brendan.
>> Thank you, Prisca.
So good morning, afternoon or
evening, depending on where you are in
the world my name is Bo Jayatilaka.
And I would like to welcome to you
Snowmass committee planning meeting.
You saw from Young-kee who we are.
But you may be wondering why this
meeting has a local organizing
committee.
When we started this
process we were hoping to welcome you
in opinion person and we would be the
people you could ask about cookies at
the breaks but yet here we are at
another Zoom meeting which we are all
very used to at this point.
Nonetheless we putting to a set of Zoom
meetings that will be productive as a start to
the main part of the Snowmass process.
You can see on the
right the blocked schedule for the
meeting.
The plan near sessions in
blue are all through today and
Wednesday.
They will be held on the
Zoom webinar as this session is.
So you will use the same information as
you used today.
In the parallel
breakouts these will be held in the
regular Zoom meetings you are
accustomed to to year.
We will be sending information for breakout
meetings later today likely after the
plane near sessions -- After the
plenary sessions end.
They start at 5
p.m.
on the west coast and 1 p.m.
on east coast so to organizers please be
mindful of these constraints and
everybody's time.
One advantage of
having this meeting be virtual is it
does lower the barrier for
participation because there isn't
travel involved.
There's over 2500
participants and while there is a
heavy participation in the U.S.
time zones you can see that we really do
have participation from around the
grown in this time zone and on the
right you can see a very diverse
reputation of frontier interests
amongst the ten frontiers in the
Snowmass 2021 process.
Now this
differs of people drivers of people
dissers havity we are agreeing to take
part in this meeting.
At its core we are agreeing and respect
each others
the members of the community and
engage in constructive guidelines.
What is expected of you and what the
accountability procedures are in this
document linked in this snow masswiki.
Everyone is encouraged for
constructivity and supportive
collaboration.
And your first point.
Contact for any time that you think
you see a violation of the core
principals and community guidelines
are the conveners and organizers of
this meetings and its sessions.
Who
have all received training and its
handlers.
That means the pron tear at
Snowmass.
They are encouraged to have
early intervention and appropriate
enough to observe issues and don't
deviate from the task force as well
and you can find their contact information at
the same link above here.
And you should remember that show mass is most
successful and everybody's voice --
Snowmass is most successful and
everybody's voice can be heard.
In terms of hearing your voice, since is this is
a planning meeting we want to make it as
conducive as possible to discussions that help
with that planning process.
One of the main points to make here is that the
Snowmass slack will have a series of dedicated
channels for the CPM.
This he all start with CPM for the channel
name.
For example there is one for each plenary
session.
Where you can have discussions during the
session and ask individual questions.
The Zoom rooms for parallel breakouts were
set up so everyone could take part and generally
you will be able to share a video and speak
in the audio and take part in those meetings
and you can set up Zoom rooms for additional
discussions.
You can use the chat.
>> One thing that is in line with the community
guidelines is you set your Zoom and
slack display names to your preferred
name.
It doesn't have to be your
legal and birth name but we ask you
don't have an email address or user
name set so you can Tuesday on the tab
in the participants list ask you can
include your personal pronouns as well
there.
One question in a comes up is
how you can ask questions in this
webinar forum.
We prefer you use the
webinar link and the Zoom chat panels.
And if there is time they will choose
questions to ask and all questions
will be copied to slack afterwards and
encourage speakers to hang around and
ask questions.
So that's it for us we
hope have you a productive meeting of
if you have questions or problems
first line is to look at the
participant guide.
And if not feel
free to email or Canuck us at the CPM
underscore help channel on slack.
Thank you and I will hand things back
to Prisca.
>> Thanks.
Remarkably on time.
Our next speaker is Joanne
Hewitt, who is the current chair of
Hpath and the lab director for
fundamental statistics.
And she will
fire us up with the exists still ahead
for us.
>> Thank you, Prisca.
Good morning, everyone.
I have to say I look forward to the day when
we can all see each other again as three
dimensional people.
So I've been charged to talk about the exciting
physics that is before us.
I've taken this to mean during the next decade.
And I would like to start with what was in
the P5 report.
So this chart on left is a
list of projects that was in the 5-5
plan.
It's a long list.
And as you know it's colored so that the green
bars are experiments in operation and analysis
and the blue bars are under fabrication or
discussion.
And the yellow bars are conceptual and technical
design.
The white horizon line is where we are today.
Almost at the end of calendar 2020.
And you see that empty these projects are now in
the green or assumed -- soon to be in
the green.
So that means all of our
hard years of labor are now turning
into project.
The remainder will be operating by the end of
the decade.
So during this talk I will March down this
list of projects and discuss the physics that
we now be able to reason
from in republican from in decade of
reap.
I will start with the moment of
the Muon.
There's been discrepancies
of 15 years old, if not olderby now
between the standard and model
predictions.
E821 achieves a
sensitivity of 540 parts per billion
and the measurement has recently been
determined to be 3.7 stigma with the
model.
You will see why I said
recently in a minute.
The -2
experiment at Fermilab started data
taking in 2018.
They completed three
runs and they have two more to go as
you can see from that plan on the very
right.
The target sensitivity is a
factor of four improvements but four
and a half improvement over that from
the brook haven run.
The world is
holding its breath waiting for these
three results.
Come on, guys.
We want to see they.
There's also an experiment, an
independent experiment
in Japan at J-park that uses an
alternative technique.
It's a
accelerated low emittance and
operations there planned for 2024 and
2026.
This will serve as an important
cross-check to any results that Muon
G-2 will get in the case it disagrees
from the standard model.
While we are waiting for the experimental
results, the theory community has been
extremely active.
There is a Muon
G-30 initiative that recently put out
a tone of 200 pages and about the same
number of Arthurs.
authors.
It's an impressive author list from around
the
wore.
They have made it notoriously
difficult to make contributions to the
G-2.
The polarization vacuum and the
hydronic -- ask there's air decomb.
With this new determination that now
says the escapesy is with 3.7 sigma.
Of course we have the LHC.
There's
much more data to come.
Regardless of
anything you read in science magazine
there's much more dad to come ask much
more physics to come.
Run 2 delivered
5% of the anticipated 3AB that is
expected in the high Lumme no, sirrity
program for the LHC.
As well as a run
3 upcoming.
One of the most important
thing is the his coupling managements.
We got the his to -- as you can see
in the middle platform and limiting.
And the holy grail for Higgs which
will soon become available to the LHC
in the high luminosity era.
In
addition to these very important Higgs
coupling measurements they will
continue to explore the unknown.
There's precision tests of the
standard model that will get even
better as the data accumulates.
And
the seven for new physics and dark
matter is not over.
There are many
increasing channels in order to tease
the small for new physics in the
background.
Most notably is from
super Sim symmetry.
The precise interpretation of this
data is of
course made possible by theory.
The
one stop impossible has now become
state-of-the-art for calculation and
standard model processes and that's
next to next to leading order.
As you
can see from the plot on the bottom
right, the level of precision that
these cross sections -- This is the
cross section for Higgs production
from fusion is next.
So what is next?
What's the next collider?
This can be the topic of discussion over the
Snowmass process and has already been
over the summer.
There's many differenting ons to
study and some designs more mature than others
and IOC is the most mature, having had a
TDR for almost a decade now.
The 2020 update in the European particle
physics strategy recommended an
electric Ron physics factory as the
highest priority next collider.
They made this recommendation because of
the percent level determination of
Higgs coupling field.
In addition the
coupling really comes into play at an
E plus, E minus Higgs factory.
This chart at the bottom left hand corner
of the screen is yet another study of
the degree of accuracy of measurements
of all of the Higgs Cummingss of all
the various types of Higgs machines.
You can see in most wayses percent
level or subpercent level precision is
achievable and decays continue limited
at the 10% level.
The bottom right
chart shows the precision that is
available for the cuppings at the
various machines.
If you look at the
solid bars, those are the ones that
are are the for production, so it
shows the cupping.
The figures of
merit to keep in mind is a 50%
precision which is achievable at the
high luminosity LHC removes the 935%
coupling level.
And 20% precision
existence at 5 sigma and 5 to 10%
precision that becomes possible at
20EVE is what is they'ded for quantum
level corrects.
This is what is
needed to really study the shame of
the Higgs potential.
Back to exploring the unknown, rare
processes are also going to have a
significant role to play over the next
decade.
Rare B Meson decays in the
announce I wills persist in various
districts.
20 to 30 types of
distributions and at various levels of
discrepancies from the level.
All
around 3 sigma.
Here is one on the
right.
Starting at +/minus which
shows the data better than that of a
standard model prediction at a 3 sigma
level.
Players in the future to watch
for there are bell, bell 2 has turned
on.
They go achieve 5 B by the end
of their run and they have now since
this past summer reclaimed the world
luminosity record.
Atlas/CMS do 3AB
and LHCb at the end of a high looming
run.
So watch this space.
This is another area where discrepancy from
the standard model could go from the 3
sigma to a 5 sigma.
Another exciting experiment that will
come online
during the next decade is mute E which
will test charged Lepton flavor
violation.
It will have Lepton
violations it measures aluminum nuclei
to a sensitivity of 3 x 10 -17 over
orders of magnitude over previous
measures.
They go start taking data
(n)2024.
Reaching their full sensitivity by the end
of the decade and will be able to probe new
physics
up to 10 of the 4VEV and interactions
and of course a flagship of our
domestic program is in the nutri know
program in the Fermilab.
There is a
process summed over Neutrino and
anti-Neutrino modes from the
collaboration alone.
This is shown on
the chart in the right where you see
particularly Loewen gives in the
Neutrino energy distribution.
The
data is quite a bit higher than the
standard background prediction.
If
you include the LSND results in the
analysis the access grows from 4.8
sigma to 6.1.
Timing information at
miniboo shows it's timed with the
interacting in the volume.
So it is
not due to the entering the detector.
Microboo has begin displays with the
promise that results will be coming
very soon.
Again the word is holding
its breath.
Waiting for the results.
And another independent check of these
anomalies anomalies and the detector
is under construction and will be
operating in a couple of years.
So by mid-decade, we will have many
different experiments in the short
baseline Neutrino program.
Checking
for these anomalies and seeing if they
persist or not.
And that will give us
plenty of Neutrino physics while the
construction of the long baseline
Neutrino facility, the detector doom
and the accelerator upgrade 2 are
underway.
The scientific program of
dune has grown since it was first
perceived by Q5 to include nuke I
don't know decay and now includes
includes dark matter displays.
There's a multivolume DTR that came
out earlier by the collaboration dune.
And you can see the sensitivity on
the charts on right.
Without the range.
And possible value of the phase you can
measure the level that
can be determined of CP violation is
given by these purple and orange
curves with the staged approach with
the purple going for seven years in
the staged approach.
Stage approach
is when the different detector modules
at the far side start to turn on.
And then ten years within the orange.
The chart on the very right shows the
rescission at which the angle Delta
can be measured for each different
value.
And you can see that it ranges
basically from 5 to 16% with 15 years
of data taking in the staged approach.
Meanwhile construction of the project
is underway.
We can see the beautiful
pictures on the bottom.
Vet excavation on the far side.
I have to say the first time I saw that it
reminded me when I saw the digging of
the SSC tunnel.
It's nice to see excavating unground
again.
There's preparation of the near site.
The first steps are clearing out the stuff
that is already there.
And last
summer there was a ground for the
caregenic plant.
Moving on to the
dark side universe there is tension in
the model measurements that persist at
the 2 to 3 sigma level.
I borrowed
this set of plots by David Kirkby at
Irving which shows recent results from
the complete digital sky survey of bar
I don't know isolation.
You can see
the measurements of the parameters we
have the distance ladder versus the
hubbell on the left.
In the In the
center the city -- and on the left A
is related to the red shift distance
of the galaxy.
And you see in each cases there's a slight
discrepancy between the different types of
measurements.
We are looking forward
to the new data that will be coming
out in the next decade, which will
hopefully resolve this tension between
these different types of measurements
or not.
DES is poised to release the
analysis of its three-year dataset
very soon.
Daisy, the dark energy
survey has completed a construction.
Commissioning is underway and we will
start taking data in 2021.
You see
the forecast for Dacey here in the
Dacey in the middle plot.
The survey
was able to do is remarkable.
You get another factor in which you combine
all the measurement techniques.
So the Vera Rubin observatory will
conduct the legacy service of space
and time, and it will turn somewhere
between 2023 and 2024, depending on
how long this pandemic lasts twill
record images of 10 billion galaxies
to observe the nature of dark energy
and the DUE piece of the telescope,
the 3.4 mega Pixel camera is now
complete it.
Took this world famous photo of broccoli shown
in the chart
on the right.
This photo got about 10 million hits already on
the web in the
first week it was up last month.
Commissions and preparations for
operations is underway.
One thing
that is different in this facility
from what is normal in the community
is that the facility will serve ago
different science collaborations so
there is no Vera Rubin collaboration
or an LSST collaboration.
The
collaboration that will study dark
energy is the dark energy design
collaboration ask they have been busy
preparing themselves for the onslaught
of data that will be coming their way
with ALSD.
They have been looking at
challenges and will sharpen tools in
preparation for start of organizes and
you can see the simulated on the
right.
I see I need to speed up just
a little bit.
I think I can do.
That
moving on to cosmic microwave
background organizes we have the
bicep/Keck array and south pole
telescope they have merged to form the
south pole observatory.
And they will
be measuring the error on tensor so
scale measure are at the level of .00
about by the end of 2023 when they
finished data intaking.
This is of
course on the way to C NMB stage 4.
It has a number of primary science
drivers you can see where they fit
here in the power spectrum from low
values.
You measure the gravitational
waves from inflation.
Up to the light
constraints as well as many
astrophysical and Astro particle
measurements.
We looking forward to
this.
It is just now starting.
The
project has passed CD0 and going for
CD1 sometime next year and it will
start taking matter at the end of this
decade.
Dark matter generation 2
experiments.
There are two.
LZ is
the higher mass range from 10Tev.
Operations will be starting in 2021 as
soon as slack finishes purifying the
liquid Xeon.
And Scdms from .5-5Ge V
and will start operations in 2022.
This is another occasion of watch this
space for new physics that will occur
very soon.
Starting in the next year
or two.
The third experiment AVMS
recently started approving a new
model.
They had continue to operate
and improve their search.
Briefly at
the end, what is new since P5?
That's
the set of P5 projects.
What is new since them?
Well the community has been very imaginative
and realized
that there's more to dark matter than
wimps.
Or Axons.
In fact there's a
whole range that composes 36 of
magnitude ask there's been an
explosion of ideas for the searches.
I've listed picture here of five of
these pro jokes who are in defunds in
order to prepare themselves.
For
construction as Des tornado by a bake
needs workshop that was held a couple
of years ago.
Quantum information
science is another area that is new
since the P5.
This has been
investments in AGP with the quantityd
SED program.
There has been a range
from quantum techniques to algorithms
to data analysis to table-top
holograms.
>> One of the applications for
physics is that in the compassion and
the ability to look for dark matter in
new ways.
So this is taking many
different techniques I quantum sensing
which provides the sensitivity to
search for dark matter in new regions
that we would not be able to before.
Last but not least, of course, can
gravitational wave science is what
brought us a noble prize quite
recently.
They provide information on
ther I will universe back to
inflation.
But it's difficult or
impossible to assess by other methods
and provides a new way to probe the
cosmos and implore fundamental
physics.
It provides cos moll give
and particle physics and even theory
has gotten into the realm here of
making predictions of much more
accurate.
They are now doing higher
order calculations in the inn spiral
velocity and Newton's constant in
order to look for massive scale binary
systems.
There's the future of
gravitational wave measurement which
can benefit from particle physics
expertise.
There's generation laser
interferometer.
It will increase the
sensitivity in frequency range from 10
to 1,000 hertz.
And there's also a
possibility of an atom interferometer.
A prototype that is being built now
where they act as waves between two
atom sources while they are in
freefall.
This probes gravitational
waves in a different frequency range
in the different interferometers and
puttings them back together.
So putting this August together this is a
remarkable achievement the community
has done and continues to built as
part of the P5 plan and we should all
be proud of ourselves.
There's been a sacrifice for us to do.
That but we should be proud of ourselves for
having accomplished that.
And over
the next decade as we do finish all of
these construction projects the
community will wait for the science
experiments.
There are several
sciences addressing these anomalies.
There are discoveries of new
properties and interactions waiting to
be made by the experiments and
theorists will be kept very busy
interpreting the data.
So in conclusion the next decade will be a
very exciting time for particle
physics.
Thank you.
>> Thank you so
much.
That was a wonderful description of the
landscape before
us.
And I'm excited, in any case we
actually don't have I in questions on
the Q&A and we are out of time any
way.
So I think I will just remind
you that you can put your questions on
slack.
And they will be answered when
shellac is back up.
We do know that
Slack is having service-wide shortages
this morning.
So feel free when
everything is available again to ask
your questions in the Slack channel to Joanne.
So at this point, I would like to
move on to our next session.
And hand
it over to the chair of that session.
Grande Glenys who is the chair.
>> Thanks a lot Joanne.
Thanks for that wonderful talk.
I'm originally a
particle theorist.
I'm from NYU.
So it's a real honor and pleasure to be
moderating this session.
Our first
speaker is Jurgen from the university
in Brussels.
He's a member of CMS and
is currently the chair of the European
committee for future accelerators and
has been one of the participants in
the European strategy.
So we will
hear from him about European plans.
Thank you very much.
I hope we can make this transition properly.
>> Thank you very much.
And thank you as well for the opportunity to
present the plans for particle physics
in Europe.
In a moment you should see
my screen.
If that will not be the case please shout.
And now we should be able to move
forward with this.
>> I see your screen fine, Jorgen but
not you.
Start your video.
Had
>> I can do that.
But it's not
optimal for doing everything.
So
maybe we throw in like this.
And I
put on the video during the session.
Understanding the particle of physics
and we do know.
(Audio Difficulties)
Partle physic can provide a wonderful
description.
But we have histories as
well and they come along with a list
of questions and mental questions in
our feel.
So cheerly we on the search
for new knowledge to appear and that
new knowledge will guide us to get to
a better understanding of particle
physic but it came along in Europe,
three strategies on the small side.
Particle physics on the large side and
Astro particle physics and if you
want, in the middle, physics.
So
these are community-driven
strategies
to address these open questions and
there after they serve as a guidance
(Audio Difficulties)
The research programs.
Obviously
there are synergies between the three
corner.
And we are exploring this
synergies and we strength end the
synergies.
An example is through
joint seminars between -- organized by
those connect the field -- physics and
in these seminars came along several
examples, for example machine
lettering tools and dark matter and on
the computer side, with the EU escape
project.
Note that the European
strategy for Bart call physics
particle experiments in the boundaries
through disciplines and through
scientific changes and through
technological corporations.
The
accelerator is to be upgraded for
that.
Connected links and magnets.
And as we speak...
(Audio Difficulties)
The investment in the Spehr meant
enter mental techniques.
>> Jorgen.
>> If you put them here in the
framework, you can achieve with them.
(Audio Difficulties)
In Green what is expected to be
achievable -- Jorgegen.
We are having
a problem.
People here are willing to
run your slide for you.
If that would help.
>> I do not hear you.
>> We have lost your slides.
>> You can still hear me.
>> Barely it's breaking up.
Maybe if
you quit trying to transmit the slides
and let Bo run them for you it would
work better.
>> He can do that.
You have slide numbers and we are on slide
number 10.
I hope you can still hear me.
So slide number 10 -- I can point to
the -- I cannot point to the slide
now.
(Audio Difficulties) Ize
mentioned -- it's very difficult.
I
do not see slide number 11 now.
On
slide number 11 let me Zoom into one
particular coupling.
A year after the
Higgs discovery it was estimated a
precision of 7 to 10% would be
achievable.
And now a value of better
than 4% seems to be reachable.
And
with only 6 years of innovations and
yet we are 20 years with that program.
Slide 12, please.
So that clearly
means and this is a very important
sentence in European strategy for
particle physics that we have explore
the key sector.
The division is to
prepare for a Higgs factory which will
be followed by a future head room
collider.
Sensitivity to energy.
(Audio Difficulties)
An order of magnitude higher than
those of the LHC.
You can still hear me?
>> It's going in and out.
But we can
sort of make out what you are saying.
Slide number 13.
So obviously what
the program that is fully embracing
that ambition is kind of a big system
program of the LHC.
It is the FCC
which provides a exhibition of
precision with the Higgs factory and
there after the energy would have
their own collisions.
Obviously this
is a phenomenal ambition and we have
to be prudent of course.By have to
plan for success and therefore it
means that by around 2026, which will
be the next update of the European
strategy we would like to identify if
it is feasible to plan for success.
That means on the technical side, and
financially and the global
governments.
On the next slide.
You see what is written in the European
strategy that Europe should
investigate technical and financial
feasibility of such a future with a
Higgs factory and that it's a possible
first stage.
And as well, discussions
with potential major planners.
Next
slide, please.
Obviously you know to
make that happen we have to advance or
accelerator the technologies.
And highlighted here are four avenues to
make that happen.
Obviously field
magnets we have Tesla and for the high
volume no, sirrity.
That will be in
310 and on an industrial scale.
And
also in this decade nEurope we
continue to strengthen our research in
plasma, be it laser driven and beam
driven and a collaboration for design
studies for the neuron collider that
high energies has been put together.
We received strong regulators in the
EU and the maybe from Europe.
Next
lied.
This is win in the strategy
that the community should ramp up with
a focus on advanced accelerator
technologies.
Next slide, please.
Of
course Europeans are and will continue
to remain active at the future
colliders elsewhere and outside of
Europe.
Super KEKB is an example with
the bell 2 experiment but as well the
learn tron-ion collider EIC user
community and in Japan, the ILC.
If
there will be a timely resignation,
the physics community physic community
would wish to community.
You have as
well the density frontier where you
see on the left page, the temperature
for the energy.
The chemical
potential or the dencity.
And in that
same space are you studying
transition.
You can do that can
collider experiments and mixed
experiment experiments and facilities
which will join in Russia and as well
as in Germany.
You see that these facilities are being
built.
And over the years to come -- and certainly in
this decade, experiments will be
taking data and analyzing this data.
Next slide.
Of course you can put your detector
very close to the region at the LHC
but also put these detectors further
away.
Look for particles which is
typically light and weekly coupling
particles the phase is being
reinstalled and they have a variety of
other proposals which are being
explored.
Next slide, please.
You
can see between the collider as well
as these other experiments is a clear
Glen tarty which is shown here in a
portal reputation.
Mitigate it
between the advancements in the
hidden
sector.
You see as well the Axon
arena.
And on the next slide you see
of course that for Axxion physics you
can use the structures and in
particular older.
If you want new
magnets and Zooming into the space of
models and up to the left you see a
lineup of experiments put together at
daisy and helps.
And all of them look
for the contraction in a high magnetic
field and the photons that will
immerge from that will be available.
Next slide.
Of course there is
physics beyond colliders and here you
see a picture of the CERN accelerator
complex.
You see the particles go to
the PS and LHCS support experiments.
All of the other protons are going to
a vast.
A other Bs.
Next slide.
And
if you look on the high energy front.
The so problem is calling for an SCS.
The lineup for dedicated experiments.
They are all reported on the collider
studies and I would like to highlight
just a few of them.
Next slide.
So,
for example in the realm of Kaon
physics today we have NA62 running.
Look for a charge.
And in the high luminosity, another
similar,
nevertheless new detector would come
online which is clever.
Which is at
the proposal stage as we speak to look
for neutral.
And on the plot on the
upper front you clearly see if you
have new physics that is comply men
tridepending on the slide.
Next
slide.
You can use the protons from
the SPS which comes at 400Ge V and
after that you put an absorber which
you remove the full cascades and what
is left are own the hidden particles
and if you created it you might
capture the decay in dedicated
experiments like ship or Tau Fv.
Next
slide.
These proposals are very much
meantry on the Loewen give side and
the high energy slide with comparative
experiments.
Neck slide, please.
So what is mentioned in the strategy,
that these experiments that offer
potentially impact for physics at the
laboratory.
But as well such
experiments is also to be than area
mind.
Next slide, please.
An example
is the surge for electroparticles like
a proton.
There's an opportunity in
Germany that you can adapt that
storage to demonstrate the technology
which will be required for that.
And
the ultimate goal would be a dedicated
storage ring.
So that would have
sensitivity for the three orders of
magnitude of what we have today.
Next
slide.
As well in the realm of flavor
physics we can look for flavor
violation at Switzerland you have the
Meg-II and MU3e experiments so you can
cop instruct 3 electric Rones.
With
that experiment you can improve the
race
Next slide.
Today we are
accelerating problems in the SPS but
we also have problems in the ESPS.
You have to have new electric cons in
the ESPS and for that you can have
accelerated technology and after the
acceleration of the electric Rones you
can have experiments which are
dedicated to dark ask light matter.
Next slide.
So this was at the level.
At the Loewen give side which means
pro tones you can do great physics.
Next slide.
You see that you can --
for example do precision physics with
antimatter.
You can decelerate the
protons and the antiprotons from the
MEV level to the KEV level.
And you
can measure the properties of
antiprotons and anti-hydrogen.
And
the facility that will make this
happen in the next decade is the
variety of B lines to a various active
experiments.
Next slide.
As well as
the European source in Sweden problems
will be accelerated to 2GEV.
A very high powered beam and that will go to
a target.
Beyond that you will have neutrons and with
these neutrons you can do fundamental physics.
For example you can measure or search for
antineutron at scales up to 300 meters
and that will help you with three
improvements.
Next slide.
Of course
with accelerators you can also create
the Neutrino Beams and this is being
done as you know in Japan and the U.S.
and through the Neutrino platform.
And Europe is involved in LBNF and
dune.
And RL BC in dune and a
detector or a near detector.
The strategy says we have to continue to
support the baseline experiments in Japan and
in the U.S.
and in particular towards the success
implementation of LBNF and DUNE.
Slide.
The three can come with a
variety of energies and you can study
them with the a variety of distances
and at lower energies they typically
come from reactors and at short
distances you have a reality of
running it this Europe and Russia that
will Zoom into what existing as a
short baseline and they will also
provide us with results in the years
to come.
Next slide.
The Neutrino film as well.
It's
important and the KATRIN experiment is
looking for the Trithum display, you
see the en pointe is very sensitive to
the mouse.
So by count the number of
electric Rones at the end of that
spectrum, you basically have a handle
of the Neutrino.
So you need a vast
spectrometer which is being shown here
and being select.
Don't forget this
is setting up the right neutrons.
Next slide.
There are major underground facilities
in Euro.
You
see them here on the map.
On the next
slide.
The first thing you can do at
these facilities is Neutrino with a
bit of decay.
We have had a variety
of experiments up until now but in the
future we have legends and cupid
coming along.
They all use different
technologies and all together they can
March on to halftimes of that of '0 to
28 years and that's the scientific
discovery.
The next slide.
Of course with these underground facilities
you
can put there as well dark matter
experiments.
So on the side of Argo.
Volume with Argo and with -- a 200
tonight experiment Darwin experiment
and this will provide the astrophysics
observatories to reach that platform.
So those tend to come up in the neck
decade.
Next slide.
>> Jorgen you have about 1 minute left.
>> In cosmic particles you can
observe them in orbit and on the
surface and with GTA in the next few
years and on the water any are
partially operational for high energy
at the next stage.
Next slide.
I will be very brief on.
Thissing of gravitational waves were
mentioned.
Very go in Europe.
And the flagship
for a decade and a decade and a half.
And beyond that we have thes a
irrational have the aspirations to go
underground in a tunnel with
criergenics.
The fats are being put
together.
Next slide, theory is of course a
almost in the backbone of particle
physic.
Of course if you are looking for new physics
will you see emerging
in this decade the Wolfe gangpauli
center.
They stress that obviously we
have to continue to support the
program of theory from the be a track
to fill solve call targets and in the
last slide let me conclude I presented
in previous presentation the vast
portfolio to unlock new avenues to
address these open questions in
fundamental physics and the key
motivation is of course to leave no
stone unturned in this endeavor.
And of course as I mentioned before.
These strategies are now a coherent
basis for funding bodies for resource
programs.
I thank you for your attention.
>> Thank you so much, Jorgen.
That
was wonderful.
It's an impressive
program.
I think due to the technical
issues we are running a tiny bit
behind we started late from the last
session.
So let's jump right into the next talk ask we
will have time for Q&A hopefulliful the next
speaker is Jeffrey Taylor at the University
of Melbourne.
He is the current chair of
Ekfa and a member of the atlas bellle
and saber collaborations and he
will tell us about the strategy and
planning in Asia and the Pacific.
Welcome, Jeffrey.
Thank you very much
for being here in spite of the time.
>> Thank you.
Let me just bring you up.
I hope that is coming through.
>>
Yes, it looks great.
>> Thank you very much for this
opportunity to discuss the Asia view
of where we are.
I would like to
start by being perhaps a limb bit
controversial by really saying that
particle physics is not regional.
So
regional road maps are as we know very
highly correlated.
And the facilities
-- the reason being of course is the
large scale facilities must be
international and interregional.
So
the facilities are chosen and designed
to meet priorities of the field.
So the correlation between these road
maps is very, very strong.
So we also
look to what is going on in other
regions.
All funding strategies make
references to international plans
which is what ties theming to.
It's
true in the Asia Pacific too.
But I
guess the big thing -- the big
difference between Asia and Europe or
the United States is that there is no
unifying structure in Asia.
There is
no union.
So China and Japan with the
dominant players with international
scale behind the geo physics
facilities but there are other
countries, Korea, and India, Taiwan
and Australian that are clever on the
international program and maintain
much smaller national programs.
So we
don't have an overriding DOE to run
things and we don't have a central
concern to give coherence.
Let's see what happens.
So the -- first of all
I would like to go through some of the
strength of Asian particle physics.
And one thing which is very clear is
that the Asian institutes from across
the board and across the countries in
Asia are very good participants.
Very
good collaborators on a global
activities.
And they are
collaborating in all the major
particle physics experiments.
But if
we pick out two areas where there's
perhaps more significance than others
within the Asian region I would
highlight flavour physics and Neutrino
physics and learn more about them
through this talk.
In Japan, KKB and
bell -- which was strongly motivated
and strong competition with the U.S.
through baba.
Has moved on to bill 2.
Which is really a leading beef
factory.
And in China there is --
what start the off as BES.
The
Beijing spectrometer.
It's now best
of 3 and BEPCII and BESII.
So
Neutrino is rashable in Asia.
There
are remarkable experiments where
significant results have been
obtained.
The Daya bay and Reno.
And
the Neutrino mixes with great
precision and aiming to do better with
juno in China.
Of course we will know
about Kamland and it's gone to hiker K
and with a much larger volume and in
parallel with that is the J-Park
extension into a high-power proton
source, aiming for 750 kilowatts.
And
of course we have geoneutrino knows as
well.
So sorting out Neutrinos from
nuclear decays from the background
which is also a very, very interesting
experiment.
There are many, this
activity which I won't have time to
cover here.
And there are many
underground experiments largely
dominated by dark matter researches
but also looking for other -- rare
processes.
So in Japan there's XMASS.
China has Panda-X and Korea KIMS and
Australia has the Za Samier.
And Look
Telling Underground Facilities.
In
Asian a Couple of Laboratories in
Korea.
The Laboratory in China, and
in the Region Several Laboratories
Within the Kamioka Mine.
And Down in
Australia Just a Few Hours from Here
Is the New SUPL Facility Which Should
Be Finished in a Year or So just to
broaden it out a little bit, the
LHAASO.
The large high at duty air
shower observatory in southwest China
is up at 4,000 metres and is a massive
array of detectors so cosmic rays
clearly being a focus as well.
Just
to look at the precision run here.
More about the factories in Japan and
China.
So what started as a very
healthy competition again the U.S.
and
Japan and driven by largly trying to
improve the CKM metrics to look for
physics beyond the standard model, the
precision over the years has really
got to incredibly high degree of
development.
And the kick has been
upgraded to super-kick and kick B.
And the belle 2 experiment has been
quickly upgraded to handle that.
So
from Lumme no, sirsy from KEKB.
The
plans were to go by another factor of
almost 40 times higher.
And 50 in
integrated luminosity over the next
ten years or So so this gives you
some idea of where we expect this
integrated luminosity it occur.
There's a program that stretches out
for the next decade or So and you can
see down at the bottom in red, it's
going to be -- which was already a
significant dataset is going to be
multiplied by 50 or so which is really
quite a remarkable change.
Of course
the parameters would have to be met by
high precision so this jump in
luminosity is an essential step.
And
as was mentioned, the pack has passed
the record of KEK reaching I think
1.22, some weeks ago.
In BEPC.
The
BEPC II and BES III facility will be
operating for another decade and they
will be around 4Ge -- V where
luminosity will be increased by 10.
And the measurements will be reduced
considerably.
So that's going to be a
rather interesting area for QCD
contributions.
So BES III is a major
experiment and it has collaborated
across the world.
And 500 or so
members.
So it is a major facility.
Bell III has nearly 1,000 rarities
from across the world.
Just an aside,
the BEPC facility was a very
interesting example of U.S.
/China collaboration.
The machine was large
I will inspired by SLAC.
Wilson suggest they had did not go to
Australia to a high energy proton beam
at the time because it was too
expensive and too hard to basically
working with SLAC and with the
personal interactions of China early
on.
The development of the early
years of BEPC shows even between
countries that you may not expect too
much collaboration to go on, the
scientists can breakthrough these
barriers.
And the BEPC and BEPC III
is a rule of what would now seem to be
unlikely collaboration.
I don't think we would like to keep that theme
going.
So Neutrino physics.
Of
course there is hyper "K" and almost
in Japan.
China has Daya Bay and
moving into JUNO in coming years and
Korea has important results out of
RENO and NEOS looking at an anomaly
from another sector.
India has an INO
observatory.
It's been through a few
numbers over the years with
environmental issues I think they are
through that now but progress is still
being hell up a bit.
This a magazine tidessed ion spectrometer.
And it's an interesting idea.
I
should say Neutrino is Japan's
national particle.
I don't know if
you have a national particle.
So just
a few pictures.
RENO, again using
these reactors.
And the results
showed a very nice electron with the
Neutrino disappearances and consistent
with the well measured value.
And the experiment right near the reactor
trying to understand the anomaly of
the anti-Neutrino spectrum coming out
of the reactors.
The Daya Bay clap
race is collaboration is by China but
has European collaborators but looked
for collaborations with good precision
and JUNO will step up with a major
increase in volume.
Ask it will have
the capacity of looking for Neutrino
hierarchy and can good precision.
The JUNO collaboration is also dominated
by China of course but it has members
institutes in Europe and in the
Americas as well.
And the JUNO
experiment has an unusual choice of
sitting on the absolute minimum of
electric Ron and Neutrino evens.
I'm
sure they will be most sensitive of
the disappears apps.
This is a sketch
of what they hope to do.
T2K -- it's been a very, very successful
experiment.
And it's been boosted by
the development of the proton machine
and it was recently reported that they
are aiming for 750 kilowatts in the
future.
When hyper K comes in there
will be two massive detectors in the
KAMIOKANDE region but not exactly the
same as where KAMIOKANDE is right now.
And this will improve the event rate
quite considerably.
We will also be
looking at super NOVA and proton decay
and other thing as all of these big
detectors do.
There's also the idea
-- I'm not sure where it is exactly
right now but putting a detector in
Korea and having a second detector
underground in Korea which will be
very interesting in a
multinational%live as well as from a
physics perspective.
Just to mention
a couple of thing in terse of
technology.
Asia has good technology.
It has technology in super conducting
magnets and technology obviously in
exercise conducting RF but China is
also doing something in that region.
Magnets for -- they have been provided
to CERN in some numbers.
Including
the D2 correct for magnet which the
first prototype has painted as being
approved.
It got through its test.
Also as we all know proton detectors
and lots of things going on in terms
of technology.
[ Please Stand By ]
In nonmember states with you see that
the big green one in the middle is the
U.S.
is the dominant one but there are
Asian members as well.
Asian users
which are relatively significant.
We get on to the -- I guess what is
driving in the big facilities,
interest in Asia.
And it was
highlighted in the European strategy
highlighted in the European strategy update. Not only wanting to maintain
its strength in high-field magnets to push into the energy frontier of the future, but the idea at least is a
possibility of going 100 kilometre scale machine and using a first stage as a plus or minus machine to satisfy
this idea that the electron-positive
tron Higgs factory is the next
collider.
The ILC in Japan would be
combatable with this strategy and
timely.
And they would wish to clap rate.
>> Jeff are you close to the end of your time.
>> Of course just a couple minutes of this.
I will push ahead.
So this is
the dominant characteristic of cross
seconds which may make a 250Ge V Higgs
factory so exciting.
Plus to minus
Higgs, plus or example the specific
energy on the Z gives us the capacity
to generate Higgs without being biased
by the trigger on the Higgs.
Why an
Asian Higgs factory?
Experience with
the plus or minus.
The KEK and IHEP.
But with that.
The cost up to 1Tev is
a cleatly different beast from 100Te
VPP collider.
Only being about 1/400
of the energy.
So it's a much more
manageable machine and the footprint
is much reduced and its new
technology.
CEPC.
The 100-kilometer Terwillegar ton sell not
such an
issue.
So these things both require
international collaboration but
neither would drive the frontier
threshold and I think that's rather
important.
But no outcomes are
assured so we need to develop various
options when you support multiple
expertise.
We need to push where we
can to look for additional source of
funding.
This gives us a plot of where we are.
And cheerly the GDP in Asia is very
large.
We must remember that a lot of
these countries are still developing.
But this is a growing portion.
And
the economic forum says by 2030, 6% of
global growth will come from Asia.
The point is that we shouldn't let
commercial and industry drive science.
Particle physics has been very
efficient in innovation and we must
provide our governments -- we must
persuade our governments that our
field is much more ahead.
You all
know the two circular machines.
The
FCC in Europe and CPC.
100 kilometre
scale machines.
And China is
proposing that it builds one itself
but with the machine which is chosest
to being approved is the ILC.
The
250ers have of the ILC.
So I look at
the economies to see --
>> Sorry?
I'm almost finished.
The relative size of Japan.
We
should remember is considerably
smaller than Europe and general and in
the U.S.
So that's part of the reason
for Japan being very, have very
careful about its decision.
The same
number of population.
126 million
compared with 238 million in the U.S.
and 700 also in Europe.
The ILC is a multimillion dollars
machine.
It's not just a new facility in the well
established laboratory.
It's a well oiled machine.
The community must not unestimate the
significance of the undertaking and we must
have unwavering and dominant support for
our feel for these to be taken
seriously.
Is it affordable we
looking at the big mac index.
A $5
billion LHC when approved in nine 5
and the big magazine big mac.
I think
it would cost 10 billion today so a 6
billion price tag on the LHC isn't too
bad as long as it isn't being shared I
should point out that Big Macs cost
less in Japan in 1995.
So I will be careful.
This points out -- I will
move straight on.
I will go to this
quickly.
ICFA has recently started
the international development team to
make preperations for the prelab of
the ILC.
We are aim fog get that
started in 2022.
In April the
Japanese financial year.
There's an
executive board shared by NAKATA with
reputation and in conclusion, many
opportunity for world-wide particle
physics in Asia exist.
Conversely Asia science contributes greatly to
the international field in Europe and
the U.S.A..
And the U.S.
shows that the scientific collaboration
is remarkably resilient even in times
when international policies are stressing
and particle physical I
objects must not miss the opportunity
presented by the Asian century.
And I
hope that Snowmass 2020 and the
following P5 will reflect on these
opportunities.
Thank you.
Sorry I ran out of time.
>> Thank you very much, Jeffrey.
I
have to be the clapper for everybody I
think.
Because of the time we will move on
but I'm sure there will be lots of interesting
questions so people please
put in their questions in the Q& Our
physical Q&A will get shortened to
make up for the overage but we can
carry it on in the Slack.
And it's a
real pleasure to introduce a member of
atlas and co-chair of the physics
long-range planning committee.
Go ahead, Bridget.
>> Thank you.
I was just waiting for
the ability to share.
So you should see my slide.
So thank you first of all for -- to
the organizer for the opportunity to
summarize the ongoing activity as was
said for the verifiment of the
Canadian sub atomic physics long-range
plan covering the period 2022-2026.
Indeed I'm presenting today in my
capacity as co-chair of the long-range
plan committee.
A responsibility I
share with my colleague Adam Ritz from
the University of University of
British Columbia
What we mean by sub atomic
physicallic in Canada means a wide
variety of energy skills and
techniques.
As you can see on these
diagrams on nuclear structure to
Neutrino property, which in this
particular case, does include Neutrino
experiments.
Collider physics,
particle astrophysics.
Dark matter
surges, et cetera.
Now these activities -- there's two
organizations that promotes and
advocates for these facilities.
The
Canadian research of nuclear
physicking.
And the Canadian
institute of particle physics or the
IPP.
So also provide a bit of
additional context, let me also
mention that the Canadian sub
community which was last surveyed in
2015 consisted at the time of 233
grant eligible researchers working at
31 different universities across the
count interest.
And at the time, in
2015 approximately 12% of the
researchers identified as women.
Canada is also of course host of
world leading centers and
infrastructures such as triumph and
snow lab and perimeter institute.
Now
the Canadian SAP long-range plan is a
plan that is updated every five years.
And it's a plan that communicates the
sub atomics' community inspiration and
identifies promising research
opportunities of course for Canada.
The overall goal of this exercise is
of course to come up with a plan that
maximizes the Canadian pact.
We all
know -- and otherwise global field has
to do with given limited finite
resources.
To do that the idea is to
build on Canada's established strength
and expertise.
And also we typically
maintain -- and even further develop
our worldclass domestic research
programs and infrastructures.
The
plan itself has historically been
articulated in the form that read a
little bit between a strategy and a
road map.
And I thought it was
important to mention that unlike in
the U.S., while the long-range plan
report presenting the community's
priorities it does not actually
dictate what gets funded or not.
Our
funding agency still traditionally
holds broad funding competition.
The
record is also used to communicate to
national stakeholders and our own
makers.
And the plans in the
community and as you can imagine the
resources requirement.
The one additional part I wanted to mention is
also -- even for us in Canada, beside
the actual final report and the final
product, the actual planning process
is an extremely valuable exercise for
the community to essentially take
stock of where it stands and to help
further -- I would argue, develop ties
among various researchers.
So on flag 5 I'm presenting here
Some background information for the
LRP process but the long-range plan is
commit commissioned by Canada's
planning agency NSERC and the
institute for particle physics physics
and CINP and the scope is to look at
the horizon of 15 years or So but the
plan itself would be active for a
period of five years, starting in
2022.
Now needless to say that given
the global nature of sub atomic
physics, of course this Canadian
planning process is informed by other
similar planning processes around the
world.
Most of which actually we are
hearing about today, which is nice.
On slide 6 I present here some
additional information about the
organization.
The planning process is
actually organized and coordinated by
the long-range plan committee which is
made up of 12 members as you can see
on the left table.
Four of which are
international members.
We also have a
number of exofficial and observer
members who represent -- for example
funding agencies and national
institute.
I thought I would also
mention s a an aside that -- as part
of the U.S.
NOMAS process and Canada
has one advisory on the group.
Heather Yolten provides us with the
U.S.
process.
So while given the time
I wasn't planning to go into the
details of the mandate of the LRP
committee.
I wanted to, however,
point out that the mandate is broader
than just addressing the scientific
opportunities and resources needed to
follow up on these opportunities.
The
mandate also includes reporting on
issues of equity, different and
diversity and inclusion.
Topics that
are of primary importance for our
community to thrive.
On slide ago I'm
showing here the timeline and a bit
more detail about the actual process.
Is the So the Canadian planning
process is a community driven process.
And it take place in a year.
The current planning process was this past
June.
At which point the June
timeline parked a point in which the
IPP and CINP have been busy working on
the preparation of the brief due to be
submitted to the LRP committee at the
beginning of December.
Meanwhile this
fall the LRP committee has become
busy.
In particular in preparing a
community-wide survey.
And also
gathering various types of data that
will be valuable for the formulation
of its recommendation.
The plan is
that at the beginning of the new year,
probably around February, we plan to
hold approximately six topical mini
town meetings to further gather inputs
from the community but those will be
topical meetings to gather information
and discussion very speck topics that
will have bubbled up and come up with
the activities ongoing since June.
Final general town hall meeting is
then planned around April next year.
Followed by men a presentation of
draft recommendations in June of the
actual report will be completed next
year and you can see there is various
opportunities for the committee to participate
in this planning process.
Now throughout this process, one of
the things that I want to emphasize is
we also want to make sure to reach
tout to young physicists and really
hear their voices and their opinion
and their thoughts and their
suggestions.
So if you are interested
in general in keeping informed about
the Canadian planning process and in
particular how to participate in the
upcoming events such as those I
highlighted I encourage you to go to
the web page that is listed here.
And we can add your name to the mailing
list in order to keep and stay
informed.
So in summary Canada is in
the mid-of a long-range planning
exercise that will culminate in a
final report available September of
next year.
As I mentioned earlier
this is a community-driven process
and
there are several ways through which
you can participate.
And in
particular we invite all interested
individuals to join the list and stay
informed about the upcoming events so
thank you for your attention.
>> Thank you so much, Bridget and
being very precise and take making
time to come talk to us today.
We will move on right away to the next
talk sky understand you will be
available for Q&A on the Slack after.
>> Yes.
>> Thank you so much again.
Our next -- it's a pleasure to
introduce Rosario Rosenfelt from the
University of Somfhalo.
He is from
the group of Latin infrastructure in
America.
And he will be tenning you about the plans in
Latin measure.
>> Thank you so much for the opportunity.
To talk about this community planning
meeting.
I'm talking on behalf of the
group of this Latin American forum for
research and infrastructure.
Which we
call EHCAP.
So this the web page you can find most of the
information regarding this process.
And you are welcome to visit this page.
And I just want to stress that this is the
first time that a strategy process
like that is conducted in Latin
America.
And we are planning this
time frame for the strategy from 3 to
5 years.
That's the first time we want to revise it.
So brief timeline
for this effort.
Which we call
LASF4RI.
Research for structures.
Under the HECAP part.
We started with
brainstorming in the community.
SILAFAE.
It's a binary symposium for
binary physics that actually is the
thing that bringing to our community
in Latin America so the general is in
November 2016.
And the year 2017 and
2018 was brief experiments and also
gathering support from national
communities.
In October 2018
something very important happened
which was the Irb aboutero-American
ministerial science and technology
meeting in Guatemala.
That's where we
have a mandate.
We have a mandate
from here in order to plan -- make the
strategy planning.
So it comes from
this institution.
In November 2018 we
had a town hall open to everybody at
the -- again at X III SILAFAE in Peru
to discuss the next steps and in 2019
we had preparatory group.
We
established a preparatory group that
celebrates from ten countries in Latin
America.
And we hell our first
workshop and also the first meeting.
And I say safer in -- for south
Americans doing fundamental research
and I want to also stress in this
meeting some members of the global
research council participated.
And
then in may, June 2019 we had the
meeting of the high level strategy
group.
Sorry the definition of the
high level strategy group which I'm
going to talk about later.
And then
we issued a call for white papers to
contribute to this effort.
And the
deadline for the submission of the
white papers was December 2019.
We
have almost 40 papers submitted.
And
July of this year we held an open
virtual symposium.
It was supposed to
be with ICTP-SAIFR.
In March it was
delayed due to the pandemic.
And now
we are doing a writeup of the physics
briefing book and the strategy
document that will be submitted to
high level strategy.
So in this
process we have an idea now of the
landscape in high energy cosmology
Astro particles in Latin America.
So
we estimate roughly at around 1,000
physicists HECAP in the region.
I
will show you now a figure of the
landscape.
So I started the countries
that we mapped out so those are the
countries that are involved in this
initiative.
And here you can see the
high energy nuclear experiments that
the community is involved with.
So
mostly LHC but future colliders here
are the Neutrinos and dark matter
experiments that communities involved
with.
So there are many of these
experiments.
Some are located in the
region.
Also in the region.
So these
are the three main areas that we are
focusing on now.
So high energy and
Astro particles and cosmology.
And
now the connections are kind of messy.
So these are the connections that
each country has groups working with
different experiments so this is
depend in the high energy nuclear
Neutrinos.
So the type for the
organization so these are the
connections of each country with
different experiments and also in
cosmology and Astro particles so as
you can see it's a very rich and
complex landscape.
And I think some
coordination can be useful.
So we are
finishing up the writing of this
physics briefing book.
It's based on
40 submitted white papers and these
are the members of the preparatory
group, as you can see here.
And when
this is final we will put this in the
archives and.
Just an idea.
Astro
Ass trophies idea.
astrophysics.
So
those are the main chapters in this
briefing and just a few highlights of
what I learned at least.
So those are
my personal picks.
It has nothing to do with the preparatory
groups my personal picks so we have of course in
the region the Auger Observatory.
The success story in the region.
We have
developed new technology for the
liquid Aragon scintilation Ariapuca
adopted in DUNE and full development
for new front-enread-out.
And a lot
of things in the region Neutrino/DM
detectors and there is a southern
wide-field view gamma-ray answer
sorry.
So this is built on the hot
experience in Mexico for MRAs and also
the possibility -- this is very
exciting of an underground facility in
the region called ANDES in the slides
with give but this is not approved
yet.
So it's a very exciting
possibility.
Finally, we are
developing a strategy document.
In
this document we have ten
recommendations that are going to be
submitted -- were submitted to the
high level strategy group.
Here you can see the members of the high level
strategy group.
This group is chaired
by Luciano Miani and Fernando Quevedo.
And representatives from around the
worm.
And a representative of the
advisory group.
Next steps October
20th a meeting of the high level
strategy group.
And they are going to
go through the document -- strategy
document that was submitted to them.
And October 27th there is going to be
this meeting of the Ibero-American
ministers of science, technology and
innovation.
This meeting here and
again we have a mandate interest them.
So we have to report our progress to
this meeting.
So this is all I have
to say.
Thank you very much.
>> Thank you very much, that was very
interesting and keeping us on time.
So we will save questions to the end
and move right awatt to last talk
which is professor Shavanka.
The
Center for Fundamental Physics Zewaii
City of Science Ask Technology in
Europe.
A member of the African
strategy and I can say he is both a
theorist and fundamentalist at IRF.
Thanks for being with us.
>> Thank you very much and thank you
very much for the opportunity.
I will discuss -- in fact Africa and the
middle east we do not really have a
strategy yet.
We started in this --
as I will mention but at least I will
show you the activity that we have in
our region and all through the country
involved and I will give you overview
about this.
So essentially Africa and
the middle east they have several high
energy physics activities.
In
particular with LHC.
There is
involvement in CMS collaboration and
ATLAS collaborations and ALICE and
other experiments and collaborator
experiments and of course theory for
particle physicallics and cosmology
and astrophysics as you will
-- as you will see.
As we said we don't have the strategy
for the countriesing to and in fact it
is initiated by a group of citizens to
set some strategy for Africa.
For
physics and high energy physics in
particular.
And it started to do so
under the umbrella of African fiscal
society.
And I hope that by June or
October 2021 we will have some
documents for this strategy.
Machine learning,
which is quite a hot
topic
nowadays,
Secondly country involved
is turkey.
Turkey has been involved in this
business
since
1961 as an observer country
and then in 2015, became one of the member
states.
They have large numbers of
members involved in certain
-- concern
C
ER
N
.
Again, they are also involved
with
Argonaut physics analysis
and also
B physics and so on.
And also in addition to this, they are involved
in the technical physics
at
Hg Cal and the prototypes systems.
This is also
a big country involved in CMS.
Another big country involved in CMS is
around.
They joined since 2002
-- Iran.
They joined since 2002
and they are also involved
in an
RBC group
like
Egypt
.
Like other groups, they are doing
organ metaphysics
-- (unknown term) metaphysics
analysis
.
We have another country, Cyprus in CMS.
It is not Africa, it is Middle East.
They
are a member
in CMS
and they are
involved
in collaborating
in different aspects
and also different subjects of physics.
Physics analysis
and (inaudible) physics
LS GC.
Small countries recently joined like
Lebanon for example.
They just joined
a couple of years ago
and they are starting with
a few numbers of
students and supporting engineering and so on
and I think we are encouraging
all the big and small countries
to be involved
in this collaboration
and this has created a kind of match work in
fact collaboration
between the regions.
Now we move
to the ATLAS collaboration
which is one of the big
experiments
at
(inaudible).
At ATLAS
, we have
turkey.
Turkey is also involved in the ATLAS experiments
and
during the data taking of the detectors
and
Turkey was involved with even 100 institutes
so they are really doing
a good job
.
From the Arabic region,
Egypt
and
CMS and
ATLAS.
(unknown term) has about 22 physicists
,
22 PhD students and 10 Masters.
It includes physics as usual, detector or
operation, commuting, detector performance
, machine learning and so on
and also updates for the machines.
This is the typical involvement
of all reasonable big institutes
.
Israel is also in ATLAS
and in fact
,
they are the first non-European
CERN
member states and they have four ATLAS groups
and they provided me with this information
.
About 15 staff members
as well as postdocs, engineers and
technicians are involved.
They are also involved
in different aspects
of physics
analysis
and machine learning
.
So this is
South Africa.
They are a big country involved in
ATLAS
and ALICE.
Again, this is quite big and strong groups
involved in this collaboration.
Other activities like
ALICE
and
AMS
02
, Turkey is involved in this experiment.
And also more important now, Turkey is involved
within FCC
, which is the
future circular collider
which we hope
will give us a large scale for detecting
(inaudible).
Israel is also involved
with other experiments like
Bell to
and
(inaudible) for neutrinos and so on.
We also have (inaudible) involved in
(inaudible) physics.
Then Egypt has a large group
of involvements
in different aspects of particle physics
and also quantum gravities
and astrophysics.
The same for (unknown term).
I think Turkey is also the same
.
-- The same for Morocco and I think
Turkey is also the same.
Big countries like Egypt, Morocco, Turkey
and South Africa.
And that's it
for this virtual time.
And as I said,
I will bind your will really have
a well-defined strategy
for building collaborations
.
Thank you very much.
>> Thank you very much.
That was wonderful.
I'm happy to know about all that activity
which I hadn't really appreciated before.
There's only a couple of minutes and I was
looking at the questions that came in on the Q&A.
There were several about the ILC.
One of them got answered
by Joanne on Slack
but
I wanted to ask
if Taylor would like to come in
on that
summer couple of them.
Another question
, while he's getting organized
, that came up
was for South America
.
What is the end days
and tell us more about Andy's
and what is the prospects for the
funding.
>> This is Geoff
and I can't see the question though.
>>
They were just generally, what's the
status?
There a couple of variance on it, but why
don't you just give us a run-down.
>> Sure.
So one slide which I went to rather quickly
which shows some progress
is that
(unknown term) has established what's called
the ILC international development team.
And like team
is charged
with preparing for the ILC pre-lap
which is a four-year period
before construction starts
where final questions
are being sorted out
on R&D
and some of the technical work.
And also governance structures are set up
and there's time to get international funding
and so forth.
So IDT, this international
development team that has
taken about a year and 1/2 or so to work,
there is no guarantee
that the work of the IDT
will result in funding for the prenup.
But we are somewhat encouraged right now
that we will continue to make progress.
>>
OK, thank you very much.
We are able to end on time.
There is now 15 minute break and we will resume
at 1:25 central time
with
Fiona Harris
in talking about the (unknown term) 2020.
Thanks to all the people in the session.
>>
I can answer the question about Andy's
if you want.
>> Sorry?
>> I can answer the question
about Andy's later
if you want.
>>
Right, right.
Sorry about that.
>> The broadcast is still going.
>> Do I do anything?
I guess I should stop my video.