Zeplin PowerPoint PPT Presentations

WIMPs in Galaxy. Diffraction off Nucleus. July 26, 2002. ICHEP 31 - Harry Nelson. 6. CDMS II ... hope we have an LSP WIMP and are doing astrophysics with it ...

ZEPLIN: A Dark Matter Direct Search Program Using Liquid Xenon

The ZEPLIN II Liquid Xenon Dark Matter Detector

Implications of Direct Dark Matter Experiments for. MSSM Higgs Searches at the Tevatron ... ANTA. RES. A T L S. ZEPLIN. DZERO. VERITAS. M A G I C. CDF. CMS. H E S ...

Title: G31 beta calibration Author: Laura Baudis Last modified by: marianne sodemann Created Date: 5/8/2003 12:18:32 AM Document presentation format

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Title: Proposed Experiments Author: Nigel J.T. Smith Last modified by: Nigel J.T. Smith Created Date: 6/23/2002 11:15:58 AM Document presentation format

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Title: Development of photodetection system based on multipixel avalanche Geiger photodiodes with WLS for Lxe low-background detectors Author:

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Tentative program 10:00 welcome, coffee 10:30 personal introductions 10:45 The status of GridPix: Harry 11:00 Interest and possibilities in Barcelona: Thorsten, Enric ...

XENON Organization and Management. Elena Aprile. 3. The XENON ... Monte Carlo simulations for detector design and background studies (Columbia /Princeton/Brown) ...

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WIN05 Astroparticle Physics WG4 Summary

Title: Diapositiva 1 Last modified by: Mark Chen Created Date: 11/15/2004 3:03:13 PM Document presentation format: On-screen Show Other titles: Arial Times New Roman ...

SUSY Dark Matter and ATLAS Dan Tovey University of Sheffield

Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...

... - Sisters of Notre Dame Longitudinal study-Alzheimer s All born before 1917 At age 22, each asked to write a one-page autobiography For example ...

Stephen Haywood

SNO Cavern. 110ft H x 75ft OD. Rectangular. Hall. 60ft L x 50ft W x 50ft H (20m x 16.5m x 16.5m) ... Dark Matter, Double Beta Decay, Low-Energy Solar Neutrinos ...

As a result of the thermal freeze-out process, a relic density of WIMPs is left behind: ... LHC Relic Density. Studying SUSY with the LHC and Astrophysics ...

Luminous matter does not account for enough mass to explain rotational velocities of galaxies ... Also groups pursuing Argon (WARP/ArDM), Helium (HERON), Neon (CLEAN) ...

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Title: dark matter Author: High Energy Physics group Description: Schools presentation Last modified by: Susan Cartwright Created Date: 5/19/1998 3:51:11 PM

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Development of High Resolution 3D Track Readout for Directional Dark Matter Detectors

INTRODUCTION AND HISTORY OF PSYCHOLOGY ... Sociocultural View This view emphasizes the importance of social interaction, social learning and a cultural perspective.

VL 13: Dunkle Materie, was ist das? We don t know it, because we don t see it! WdB, C. Sander, V. Zhukov, A. Gladyshev, D. Kazakov, EGRET excess of diffuse ...

Backgrounds result from nuclear processes, thus experimenters require NP ... Low background counting facility (Abstract) Muon induced backgrounds (Abstract) ...

University of Michigan Ann Arbor. Katie Freese (University of Michigan) ... Nma = 0.0200 0.0032 /kg/day/keVee (2-6 keVee) Elegant V, etc. 30 km/s. 232 km/s ...

Bhaskar Dutta

DEVELOPMENT OF PHOTODETECTION SYSTEM BASED ON MULTIPIXEL AVALANCHE GEIGER ... pedestal. RESULTS & PDE CALCULATION. 84 cells. RESULTS & PDE CALCULATION. WLS. Sapphire ...

(Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such objects ... Halo profile (inhomogeneities?) Boundary conditions ...

Institute for Nuclear Research of Russian Academy of Sciences (INR) ... AURIGA. DUAL R&D. ROG. MiniGRAIL. SFERA. Baksan Neutrino Observatory b) Interferometers ...

The way to a final design for the northern hemisphere: From HENAP through APPEC and the EU? ... Or 100 years (Picasso design 1909) Or is it 400 years? ...

Testing CsI photocathodes in Liquid Xenon

PowerPointPrsentation

Isotropy Problem. At time of neutralization, 105 causally disconnected regions ... it 'impossible' to achieve this isotropy. 21 Aug 03. John Huth, Harvard ...

Physics at Canfranc. Underground Laboratory (LSC) Jos Bernab u. IFIC Valencia ... Professor Jose Angel Villar, as Associate Director ...

Dark Matters Mavourneen Wilcox Physics 711 Presentation

Dark Matters Mavourneen Wilcox Physics 711 Presentation

Fast Electronics for a Liquid Xenon Scintillation Detector with Very Low ... Main purpose is to measure quenching factor for nuclear recoils in liquid xenon ...

Bolometer 1. Bolometer 2. Bolometer 3. HEP-Aachen/16-24 July ... Bolometer 1 : Q=f(Er) diagram. Events in red (both inside. and outside the nuclear recoil zone) ...

to galaxies Building electronics for Relativistic Heavy Ion Collider and for Dark Matter Search Wojtek Skulski Department of Physics and Astronomy

Direct dark matter detectors search for elastic nuclear ... Fabricate from low radioactivity. materials. Low Threshold Energy. High Sensitivity/Signal output ...

Dark Matter Detection with Liquid Xenon

Self-gravitating ball of ideal gas at a uniform temperature would have ... Archeological Lead. CDMS II: Overview. Located at the Soudan mine in sunny Minnesota ...

The Quantum Universe

(My feeling) Geant4 is still not considered a fully established and ... Fission, (a,n) and cosmogenic neutrons are not an issue (very different for DM expts) ...

Connecting Quarks with the Cosmos: Notes from the Underground

Astronomy and Astrophysics Advisory Committee Meeting. 12-13 October 2006 ... Andre Rubbia (ETH-Zurich) Kate Scholberg (Duke) Yoichiro Suzuki ( U. of Tokyo) ...