000 02466nlm1a2200577 4500
001 637161
005 20231030040200.0
035 _a(RuTPU)RU\TPU\network\1258
035 _aRU\TPU\network\1257
090 _a637161
100 _a20140527a2005 k y0engy50 ba
101 0 _aeng
102 _aUS
135 _adrcn ---uucaa
181 0 _ai
182 0 _ab
200 1 _aCRESST cryogenic dark matter search
_fC. Cozzini [et al.]
203 _aText
_celectronic
300 _aTitle screen
330 _aThe CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorbers for direct WIMP (weakly interactive massive particles) detection. The phonon signal in the CaWO4 crystal is registered in coincidence with the light signal, which is measured with a separate cryogenic light detector. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). As a result an active discrimination of the electron recoils against nuclear recoils is achieved. Results on the properties of the detector modules and on the WIMP sensitivity are presented
333 _aРежим доступа: по договору с организацией-держателем ресурса
461 _tNew Astronomy Reviews
_oScientific Journal
463 _tVol. 49, iss. 2-6
_v[P. 255-258]
_d2005
610 1 _aэлектронный ресурс
610 1 _aтруды учёных ТПУ
701 1 _aCozzini
_bC.
701 1 _aHenry
_bS.
701 1 _aKraus
_bH.
701 1 _aMajorovits
_bB.
701 1 _aRamachers
_bY.
701 1 _aAngloher
_bG.
701 1 _aFrank
_bT.
701 1 _aHauff
_bD.
701 1 _aNinkovic
_bJ.
701 1 _aNinkovic
_bJ.
701 1 _aPetricca
_bF.
701 1 _aProbst
_bF.
701 1 _aSeidel
_bW.
701 1 _aStodolsky
_bL.
701 1 _aUchaykin
_bS. V.
_cspecialist in the field of non-destructive testing
_cEngineer of Tomsk Polytechnic University, Doctor of physical and mathematical sciences
_f1963-
_gSergey Victorovich
_2stltpush
_3(RuTPU)RU\TPU\pers\32279
701 1 _aBucci
_bC.
701 1 _aFeilitzsch
_bF. von
701 1 _aJagemann
_bT.
701 1 _aJochum
_bJ.
701 1 _aRau
_bW.
701 1 _aRazeti
_bM.
701 1 _aStark
_bM.
701 1 _aWulandari
_bH.
801 2 _aRU
_b63413507
_c20140527
_gRCR
856 4 _uhttp://www.sciencedirect.com/science/article/pii/S1387647305000369
942 _cCF