DMUK Meeting - Oxford

Monday 8 Dec 2014, 09:00 → 17:00 Europe/London

Dennis Sciama Lecture Theatre (Denys Wilkinson Building)

09:15 → 09:45 Calibrating the LUX Detector

Speaker: Dr James Dobson (University of Edinburgh)

Slides JDobson_LUX_DMUK8thDec14.pdf

09:45 → 10:15 The Search for Dark Matter @LHC

Speaker: Dr Steve Worm (RAL)

Slides Worm_141208_DMUK_Oxford.pdf

10:15 → 11:00 Theoretical Uncertainties in Direct Dark Matter Detection and how to deal with them.

Speaker: Dr Felix Kahlhoefer (DESY)

Slides Kahlhoefer.pdf

11:00 → 11:30 Coffee

11:30 → 12:30 Dark Matter from Astrophysics/Cosmology

Speaker: Prof. Jo Dunkley (University of Oxford)

Slides dm_dec08.pdf

12:30 → 13:30 Lunch

13:30 → 13:45 Closing in on the velocity distribution of Dark Matter with direct detection and neutrino telescopes

The next generation of direct detection experiments not only will allow the reconstruction of the Particle Physics properties of Dark Matter (i.e. its mass and scattering cross section), but also the determination of its local velocity distribution. However, this measurement is hinder by the fact that direct detection experiments, being sensitive only above some energy threshold, do not probe down to very low velocities. I am going to show you how this problem can be solved by including the information provided by a (simulated) detection of neutrinos from the Sun. The complementary nature of such a signal will significantly improve the precision in the simultaneous reconstruction of the Dark Mass mass, cross section and velocity distribution.

Speaker: Dr Mattia Fornasa (University of Nottingham)

Slides 01_Fornasa.pdf

13:45 → 14:00 First SD WIMP limits from DRIFT with full z-fiducialisation

First SD WIMP limits from DRIFT with full z-fiducialisation are presented, along with expected improvements in the near future.

Speaker: Mr Andrew Scarff (University of Sheffield)

Slides 02_DRIFT_DMUK_8Dec2014.pdf

14:00 → 14:15 Recent progress with the DEAP-3600 Dark Matter experiment

DEAP-3600 is a single phase liquid argon (LAr) dark matter experiment. It is located 2 km underground at SNOLAB, in Sudbury, Ontario. The detector has 1 tonne fiducial mass target of LAr. Construction of DEAP-3600 is nearly complete and commissioning will start in January 2015. The target sensitivity to spin-independent scattering of 100 GeV WIMPs is 10−46 cm2 which improves the current limits by one order of magnitude. The DEAP- 3600 background target is 0.6 background events in the WIMP region of interest in 3 tonne-years from all sources. This is achieved by selecting ultra low radioactive materials, sanding DEAP-3600 acrylic vessel and developing external calibration sources and deployment systems. The β/γ backgrounds are mitigated by LAr excellent pulse shape discrimination. This talk will present an overview and status of the experiment.

Speaker: Dr Nasim Fatemighomi (Royal Holloway University London)

Slides 03_DMUK_2014_v4_DEAP.pdf

14:15 → 14:30 LZ Project Status

Speaker: Dr Henrique Araújo (Imperial College London)

Slides 04_LZ-DMUK-HA141208.pdf

14:30 → 14:45 LZ background estimation and sensitivity goal

Speaker: Dr Paolo Beltrame (University of Edinburgh)

Slides 05_DM-UK_Meeting_2014_12_08_-_paolo_v0.pdf

14:45 → 15:00 Axion search prospects with the LZ experiment

TBD

Speaker: Ms Maria Francesca Marzioni (University of Edinburgh)

Slides 06_M.F._Marzioni_DM-UK_Oxford_2014_12_08.pdf

15:00 → 15:15 Boulby underground laboratory

TBD

Speaker: Mrs Emma Meehan (STFC)

Slides 07_DMUK_081214_EMeehan.pdf

15:15 → 15:30 UK Screening Facilities

Speaker: Dr Paul Scovell (University of Oxford)

Slides 08_DMUKScreeningPRS.pdf