Ramage,GGR. KK state. For some compactifications LKP stable ... Cryptons,... Indirect detection. Direct detection possible. CMSSM. Ramage, GGR. SO(10) ...
Men define each other as as having control over women and children ... 'You're going do every damn thing I tell you to do and you have no choice.' 'I got control. ...
Smell. Taste. Touch. Hearing. Sight. Hearing and Seeing. We proclaim to you the one who existed from the beginning, whom we have heard and seen. ... Smell ...
Dialogue impos par le syst me : s quencement strict des actions. Difficult ... de regrouper dans une m me fen tre des affichages r partis sur plusieurs pages ...
one ton class projects: Liquid Xenon: XENON, ZEPLIN. cryogenic: EURECA (EDELWEISS, CRESST, ... LHC observes new particles. fits to SuSy. parameters predict ...
Ease in learning the system originally and in assimilating ... video surveillance and burglar alarms. Multiple-zone environmental controls. Maintenance records ...
Bubble Chamber tweaking. For rate. For background. Data. Conclusions. Outline. WIMPs. Bubble Chambers. Bubble Chamber tweaking. For rate. For background. Data ...
CMB constraints on WIMP annihilation: energy absorption during recombination ... Photoionization. ELECTRONS. PHOTONS. All fast relative to Hubble time. ...
Possible problems: perturbation of asteroids and validity of Gould approximations. ... Guess: No, the asteroid orbits are very special and in general WIMP orbits are ...
Weakly Interacting Massive Particles (WIMPs) may be gravitationally ... There, they annihilate with each other, producing n's. IceCube will search for these n's ...
KIMS collaboration. 2007. 11. 23. S. Ryu, Rotation curve of Spiral Galaxies ... from the rotation curve of Milky Way Galaxy. 8 x 8 x 30 cm3, ~8 kg. 30 km/s. 220 km/s ...
Mani Tripathi, INPAC Meeting. New Collaboration. Groups formerly in XENON10: ... Neutrons ( ,n) & fission subdominant. External: large water shield with muon veto. ...
This material has been developed by Georgia Tech HCI faculty, and ... sheets of paper on our desks, so is a familiar concept. ... the cluttered desk : ...
When Wimps Rule the Earth: ... When a so-so company s stock is in the tank and shareholders are restless and unimpressed with short-term earnings boosts and when ...
Betas mostly triplet (slow long pulse) Recoils mostly singlet ... Betas ... Beta/gamma backgrounds are under control with pulse shape and ionization ...
'The evidence for cold, non-baryonic dark matter is one of the ... Invisibly Higgs decay. 16. Th. and Exp. of t. ch hep-ph/0605003. FCNC in SM. 17. 2HDM. 18 ...
Introduction of our low mass wimp experiment. Structure of CsI ... Cryogenic bolometer. 262g Sapphire detector. The lowest threshold. gotten until now: 500keV ...
... of the light can be detected. But: Highly non-gaussian fluctuations! ... This could offer an auto-matic method to tag the 'birth' of barium in the decay, ...
Measured by HR(High Resolution) ICP-MASS in Old Dominion U. (USA) ... 237 kg days data. Background spectra of current crystal. Summary and prospects ...
TP: When a so-so company's stock is in the tank and shareholders are restless ... share price it can buy back a big hunk of its stock which not only lifts the ...
... Direct Manipulation WIMP (Windows ... then give command Hollan argues this user feel more important to DM than Shneiderman's methods Direct Manipulation, ...
if high QF applies for WIMP recoils: results comparable to EDELWEISS (10-6 pb) Light yield ... Different targets (WIMP signature) Collect European competence ...
The Heidelberg Dark Matter Search Experiment Laura Baudis Stanford University The HDMS detectors 2 HPGe detectors in one cryostat system inner: WIMP target outer ...
stau pairs. Q-balls. WIMPS. monopole. Extra-Dimensions ... Physics beyond the standard model. WIMPS. David Hardtke -- University of California, Berkeley ...
Extraordinary Dark Matter (WIMPS) Weakly Interacting Massive Particles: ... WIMPs can't contract to center because they don't radiate away their orbital energy ...
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 ...
CDMS increasing sensitivity to WIMP interactions by increasing detector mass ... World's best limits on WIMP dark matter properties above 44 GeV/c2 ...
(Semi) UHE Neutrinos in Super-Kamiokande Looking for point sources and WIMPs Alec Habig, Univ. of Minnesota Duluth For the Super-Kamiokande Collaboration
IHM de demain ? Interfaces Post-Wimp . Delozanne, M1-IHM, Paris 5 Elisabeth.Delozanne@math-info.univ-paris5.fr http://www.math-info.univ-paris5.fr/~delozanne