2015
DOI: 10.1016/j.astropartphys.2015.02.001
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Sensitivity of alkali halide scintillating calorimeters with particle identification to investigate the DAMA dark matter detection claim

Abstract: Scintillating calorimeters are cryogenic detectors combining a measurement of scintillation with one of phonons to provide particle identification. In view of developing alkali halide devices of this type able to check the DAMA/LIBRA claim for the observation of dark matter, we have simulated detector performances to determine their sensitivity by two methods with little model-dependence. We conclude that if performance of the phonon channel can be brought in line with those of other materials, an exposure of … Show more

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Cited by 11 publications
(6 citation statements)
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“…CsI, pure or doped, is a frequently used scintillator, for instance in neutrino physics [1], or in searches for hypothetical dark matter particles [2] that could account for most of the matter in our Universe [3]. There has been recent interest in the use of CsI as a cryogenic scintillating calorimeter for the detection of direct dark matter interactions with regular matter [4][5][6][7][8]. CsI is an appealing target for such a detector because of its high LY at low temperature and the possibility of probing new WIMP interaction parameter space [6].…”
Section: Introductionmentioning
confidence: 99%
“…CsI, pure or doped, is a frequently used scintillator, for instance in neutrino physics [1], or in searches for hypothetical dark matter particles [2] that could account for most of the matter in our Universe [3]. There has been recent interest in the use of CsI as a cryogenic scintillating calorimeter for the detection of direct dark matter interactions with regular matter [4][5][6][7][8]. CsI is an appealing target for such a detector because of its high LY at low temperature and the possibility of probing new WIMP interaction parameter space [6].…”
Section: Introductionmentioning
confidence: 99%
“…This decade will see the direct direction experiments find dark matter or be blinded by the Sun, even underground. New technologies have thus to be further explored to ensure a smooth transition, such as directional dark matter detectors [224] like Cygnus [225,226], or alkali halide crystals as bolometers [227] such as COSINUS [228]. The search for dark matter has been long but the collective efforts of nuclear, particle and astrophysicists around the world in the new field of astroparticle physics will surely provide answers to one of the biggest questions in science [229].…”
Section: Discussionmentioning
confidence: 99%
“…This material, doped with Tl to enhance light output, is actively used in scintillation detectors for DM searches [594][595][596][597][598][599][600][601][602][603]. Undoped CsI is very attractive for bolometric searches for DM signals [415,604,605], particularly for the detection of the annual modulation of the DM rate [606]. Indeed, a low light yield of CsI at room temperature (a factor ∼20 lower than the light yield of Tl-doped cesium and sodium iodides [607]) can be about an order of magnitude higher at 3.4-10 K [264,608].…”
Section: Strontium Fluoridementioning
confidence: 99%
“…Both pure and Tl-doped NaI exhibit a huge light yield at low temperatures (at ∼2 K), which amounts to about 65% of the light output of NaI(Tl) at room temperature [263]. Therefore, a NaI-based LTD with particle identification is of a great interest for DM search experiments [585,605,606,609], in particular aiming at the investigation of the nature of the galactic DM signature detected in the DAMA/LIBRA and DAMA/NaI experiments with room-temperature NaI(Tl) scintillation detectors (e.g., see [424][425][426][427] and references therein). However, in addition to a low Debye temperature (as in the case of CsI, Section 3.7.1), a high hygroscopicity of NaI is a challenge for bolometric applications of this material.…”
Section: Sodium Iodidementioning
confidence: 99%