CRESST cryogenic dark matter search

Bibliografiset tiedot
Parent link:New Astronomy Reviews: Scientific Journal
Vol. 49, iss. 2-6.— 2005.— [P. 255-258]
Muut tekijät: Cozzini C., Henry S., Kraus H., Majorovits B., Ramachers Y., Angloher G., Frank T., Hauff D., Ninkovic J., Petricca F., Probst F., Seidel W., Stodolsky L., Uchaykin S. V. Sergey Victorovich, Bucci C., Feilitzsch F. von, Jagemann T., Jochum J., Rau W., Razeti M., Stark M., Wulandari H.
Yhteenveto:Title screen
The 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
Режим доступа: по договору с организацией-держателем ресурса
Kieli:englanti
Julkaistu: 2005
Aiheet:
Linkit:http://www.sciencedirect.com/science/article/pii/S1387647305000369
Aineistotyyppi: Elektroninen Kirjan osa
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637161

MARC

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330 |a The 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 |a Режим доступа: по договору с организацией-держателем ресурса 
461 |t New Astronomy Reviews  |o Scientific Journal 
463 |t Vol. 49, iss. 2-6  |v [P. 255-258]  |d 2005 
610 1 |a электронный ресурс 
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701 1 |a Cozzini  |b C. 
701 1 |a Henry  |b S. 
701 1 |a Kraus  |b H. 
701 1 |a Majorovits  |b B. 
701 1 |a Ramachers  |b Y. 
701 1 |a Angloher  |b G. 
701 1 |a Frank  |b T. 
701 1 |a Hauff  |b D. 
701 1 |a Ninkovic  |b J. 
701 1 |a Ninkovic  |b J. 
701 1 |a Petricca  |b F. 
701 1 |a Probst  |b F. 
701 1 |a Seidel  |b W. 
701 1 |a Stodolsky  |b L. 
701 1 |a Uchaykin  |b S. V.  |c specialist in the field of non-destructive testing  |c Engineer of Tomsk Polytechnic University, Doctor of physical and mathematical sciences  |f 1963-  |g Sergey Victorovich  |3 (RuTPU)RU\TPU\pers\32279 
701 1 |a Bucci  |b C. 
701 1 |a Feilitzsch  |b F. von 
701 1 |a Jagemann  |b T. 
701 1 |a Jochum  |b J. 
701 1 |a Rau  |b W. 
701 1 |a Razeti  |b M. 
701 1 |a Stark  |b M. 
701 1 |a Wulandari  |b H. 
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