'Nuclear recoils' presentation slideshows

AGENDA: 1) Neutrinos 2) Dark matter, Axions, LFV search. 3) Kaons and B-mesons

1.01k views • 87 slides

Poszukiwania Ciemnej Materii

859 views • 70 slides

Direct Detection of CDM: The challenge ahead

619 views • 47 slides

Searches for Dark Matter (the Quest)

Searches for Dark Matter (the Quest). Harry Nelson UCSB 2003 SLAC Summer Insitute Aug. 5-6 2003. Recap - Direct Detection. How to dredge the small (0.01 DRU= ev/(kg d keV)) up out of a bigger background (1 DRU typical) of recoil electrons from comptons?.

524 views • 45 slides

Recent Results from CDMS Experiment

Recent Results from CDMS Experiment. Caltech – 01/06/2004 Vuk Mandic UC Berkeley. Overview. Dark Matter: Evidence and Candidates CDMS Experiment: Setup and Detectors Run Overview Background Discrimination Results: Neutrons vs WIMPs Soudan Status Conclusion. Evidence for Dark Matter.

581 views • 44 slides

COUPP: First Results Dark Matter Limits From a Bubble Chamber

453 views • 32 slides

COUPP: First Results and Current Status Dark Matter Limits From a Bubble Chamber

453 views • 32 slides

The XENON Dark Matter Experiment

The XENON Dark Matter Experiment. Elena Aprile Physics Department and Columbia Astrophysics Laboratory Columbia University http:// www.astro.columbia.edu/~lxe/XENON/. Dark Energy 73%. Energy 2/3. The Case for Non-Baryonic Dark Matter Conclusion from all Evidence.

519 views • 32 slides

Dan Akerib Case Western Reserve University 7 July 2001 Snowmass, Colorado E6.2 Working Group

The CDMS I & II Experiments: Challenges Met, Challenges Faced. Dan Akerib Case Western Reserve University 7 July 2001 Snowmass, Colorado E6.2 Working Group. Case Western Reserve University D.S. Akerib,D. Driscoll, S. Kamat, T.A. Perera, R.W. Schnee, G.Wang

477 views • 32 slides

AN EXPERIMENTAL OVERVIEW OF Direct Dark Matter Searches

414 views • 31 slides

SEARCHING FOR WIMPS UNDERGROUND: THE EXPERIMENTAL QUEST

374 views • 30 slides

The XENON10 dark matter search

The XENON10 dark matter search. T. Shutt Case Western Reserve University. The XENON10 Collaboration. Columbia University Elena Aprile (PI), Karl-Ludwig Giboni , Sharmila Kamat, Maria Elena Monzani , , Guillaume Plante*, and Masaki Yamashita Brown University

405 views • 29 slides

The C ryogenic

The C ryogenic. D ark. M atter. S earch. Michael B. Crisler Fermi National Accelerator Laboratory 03 June 2003. CDMS Collaboration. Case Western Reserve University

366 views • 28 slides

Progress on DEAP

411 views • 26 slides

Outline

Introduction Basic idea of low temperature detectors Sensor comparison (Thermistors, TES, MMC) Low temperature detectors in underground labs Direct Search for WIMPs, Search for ?? 0 ? Low temperature detectors at KRISS X-ray sensors Prospective R & D. Outline. Light detector.

417 views • 25 slides

The XENON10 dark matter search

The XENON10 dark matter search. T. Shutt Case Western Reserve University. The XENON10 Collaboration. Columbia University Elena Aprile (PI), Karl-Ludwig Giboni , Sharmila Kamat, Maria Elena Monzani , , Guillaume Plante*, and Masaki Yamashita Brown University

395 views • 25 slides

The XENON10 dark matter search

The XENON10 dark matter search. T. Shutt Case Western Reserve University. The XENON10 Collaboration. Columbia University Elena Aprile (PI), Karl-Ludwig Giboni , Sharmila Kamat, Maria Elena Monzani , , Guillaume Plante*, and Masaki Yamashita Brown University

395 views • 25 slides

Status of Cold Dark Matter Searches Dan Bauer, Fermilab

399 views • 23 slides

I norganic Scintillators for Rare Event Searches

I norganic Scintillators for Rare Event Searches. Rare Event Searches with Scintillators. Standard Scintillation Detectors vs. Bolometers. Standard scintillation detector Crystal at RT, scintillation light detected by PMT Particle identification by pulseshape possible.

382 views • 22 slides

Data analysis and background investigation in the EDELWEISS direct d ark m atter search

Data analysis and background investigation in the EDELWEISS direct d ark m atter search. Earth moves through DM halo ? DM = 0.3 GeV /cm 3. The corner of the dark we are looking at. ?. ?. Production. t. Annihilation. E R ~ 10 keV. q. q. <v> ? 230 km/s. t. t.

212 views • 13 slides