The CRESST Experiment: Recent Results and Prospects; Arxiv.org

The CRESST Experiment: Recent Results and Prospects; Arxiv.org

Bibliografiske detaljer
Parent link:Arxiv.org.— 2001.— High Energy Physics - Experiment
Andre forfattere: Stefano P. Di, Bruckmayer M., Bucci C., Cooper S., Cozzini C., Feilitzsch F. von, Frank T., Hauff D., Jagemann T., Jochum J., Keeling R., Kraus H., Marchese J., Pergolesi D., Probst F., Ramachers Y., Schnagl J., Seidel W., Sergeyev I., Stark M., Stodolsky L., Uchaykin S. V. Sergey Victorovich, Wulandari H.
Summary:Title screen
The CRESST experiment seeks hypothetical WIMP particles that could account for the bulk of dark matter in the Universe. The detectors are cryogenic calorimeters in which WIMPs would scatter elastically on nuclei, releasing phonons. The first phase of the experiment has successfully deployed several 262 g sapphire devices in the Gran Sasso underground laboratories. A main source of background has been identified as microscopic mechanical fracturing of the crystals, and has been eliminated, improving the background rate by up to three orders of magnitude at low energies, leaving a rate close to one count per day per kg and per keV above 10 keV recoil energy. This background now appears to be dominated by radioactivity, and future CRESST scintillating calorimeters which simultaneously measure light and phonons will allow rejection of a great part of it
Sprog:engelsk
Udgivet: 2001
Fag:
электронный ресурс
труды учёных ТПУ
Online adgang:http://arxiv.org/abs/hep-ex/0011064
Format: Electronisk Book Chapter
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637197

MARC

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200 1 |a The CRESST Experiment: Recent Results and Prospects  |f P. Di Stefano [et al.] 
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330 |a The CRESST experiment seeks hypothetical WIMP particles that could account for the bulk of dark matter in the Universe. The detectors are cryogenic calorimeters in which WIMPs would scatter elastically on nuclei, releasing phonons. The first phase of the experiment has successfully deployed several 262 g sapphire devices in the Gran Sasso underground laboratories. A main source of background has been identified as microscopic mechanical fracturing of the crystals, and has been eliminated, improving the background rate by up to three orders of magnitude at low energies, leaving a rate close to one count per day per kg and per keV above 10 keV recoil energy. This background now appears to be dominated by radioactivity, and future CRESST scintillating calorimeters which simultaneously measure light and phonons will allow rejection of a great part of it 
463 |t Arxiv.org  |v High Energy Physics - Experiment  |d 2001 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
701 1 |a Stefano  |b P. Di 
701 1 |a Bruckmayer  |b M. 
701 1 |a Bucci  |b C. 
701 1 |a Cooper  |b S. 
701 1 |a Cozzini  |b C. 
701 1 |a Feilitzsch  |b F. von 
701 1 |a Frank  |b T. 
701 1 |a Hauff  |b D. 
701 1 |a Jagemann  |b T. 
701 1 |a Jochum  |b J. 
701 1 |a Keeling  |b R. 
701 1 |a Kraus  |b H. 
701 1 |a Marchese  |b J. 
701 1 |a Pergolesi  |b D. 
701 1 |a Probst  |b F. 
701 1 |a Ramachers  |b Y. 
701 1 |a Schnagl  |b J. 
701 1 |a Seidel  |b W. 
701 1 |a Sergeyev  |b I. 
701 1 |a Stark  |b M. 
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 Wulandari  |b H. 
801 2 |a RU  |b 63413507  |c 20141021  |g RCR 
850 |a 63413507 
856 4 |u http://arxiv.org/abs/hep-ex/0011064 
942 |c CF 

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