000 | 02924nlm1a2200481 4500 | ||
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001 | 637159 | ||
005 | 20231030040200.0 | ||
035 | _a(RuTPU)RU\TPU\network\1256 | ||
035 | _aRU\TPU\network\1252 | ||
090 | _a637159 | ||
100 | _a20140526a2005 k y0engy50 ba | ||
101 | 0 | _aeng | |
102 | _aUS | ||
135 | _adrcn ---uucaa | ||
181 | 0 | _ai | |
182 | 0 | _ab | |
200 | 1 |
_aCaWO4 crystals as scintillators for cryogenic dark matter search _fJ. Ninkovic [et al.] |
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203 |
_aText _celectronic |
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300 | _aTitle screen | ||
330 | _aAlthough it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a slow light response. However, a high Z and a good light output make this crystal a candidate for use in direct dark matter search experiments. The Cryogenic Rare Event Search using Superconducting Thermometers (CRESST II) experiment looks for hypothetical massive elementary particles called Weakly Interacting Massive Particles (WIMPs). In an elastic collision of WIMPs with ordinary matter a WIMP transfers part of its energy to a nucleus. Such nuclear recoils are the signals dark matter searches look for. CRESST is using CaWO4 crystals with coincident detection of phonons and scintillation light to suppress radioactive background. Light output and energy resolution of different CaWO4 samples were systematically measured. Best samples have an energy resolution at the 137Cs line (661 keV)<8%. As CRESST is a rare event search experiment it has to prevent the background caused by natural radioactivity; therefore, a study of the radiopurity of CaWO4 crystals has been performed. X-ray luminescence properties of crystal samples, in the temperature range 77–500 K, will be presented | ||
333 | _aРежим доступа: по договору с организацией-держателем ресурса | ||
461 |
_tNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment _oScientific Journal |
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463 |
_tVol. 537, iss. 1-2 _v[P. 339-343] _d2005 |
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610 | 1 | _aтруды учёных ТПУ | |
610 | 1 | _aэлектронный ресурс | |
701 | 1 |
_aNinkovic _bJ. |
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701 | 1 |
_aAngloher _bG. |
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701 | 1 |
_aBucci _bC. |
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701 | 1 |
_aCozzini _bC. |
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701 | 1 |
_aFrank _bT. |
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701 | 1 |
_aHauff _bD. |
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701 | 1 |
_aKraus _bH. |
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701 | 1 |
_aMajorovits _bB. |
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701 | 1 |
_aMikhailik _bV. |
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701 | 1 |
_aPetricca _bF. |
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701 | 1 |
_aProbst _bF. |
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701 | 1 |
_aRamachers _bY. |
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701 | 1 |
_aRau _bW. |
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701 | 1 |
_aSeidel _bW. |
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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 |
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801 | 2 |
_aRU _b63413507 _c20160512 _gRCR |
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856 | 4 | _uhttp://www.sciencedirect.com/science/article/pii/S0168900204018480 | |
942 | _cCF |