Exploring Low-Mass Dark Matter with CRESST
Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoi...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Strauss, R. [verfasserIn] Angloher, G. [verfasserIn] Bento, A. [verfasserIn] Bucci, C. [verfasserIn] Canonica, L. [verfasserIn] Defay, X. [verfasserIn] Erb, A. [verfasserIn] Feilitzsch, F. v. [verfasserIn] Ferreiro Iachellini, N. [verfasserIn] Gorla, P. [verfasserIn] Gütlein, A. [verfasserIn] Hauff, D. [verfasserIn] Jochum, J. [verfasserIn] Kiefer, M. [verfasserIn] Kluck, H. [verfasserIn] Kraus, H. [verfasserIn] Lanfranchi, J. C. [verfasserIn] Loebell, J. [verfasserIn] Münster, A. [verfasserIn] Pagliarone, C. [verfasserIn] Petricca, F. [verfasserIn] Potzel, W. [verfasserIn] Pröbst, F. [verfasserIn] Reindl, F. [verfasserIn] Schäffner, K. [verfasserIn] Schieck, J. [verfasserIn] Schönert, S. [verfasserIn] Seidel, W. [verfasserIn] Stodolsky, L. [verfasserIn] Strandhagen, C. [verfasserIn] Tanzke, A. [verfasserIn] Trinh Thi, H. H. [verfasserIn] Türkoglu, C. [verfasserIn] Uffinger, M. [verfasserIn] Ulrich, A. [verfasserIn] Usherov, I. [verfasserIn] Wawoczny, S. [verfasserIn] Willers, M. [verfasserIn] Wüstrich, M. [verfasserIn] Zöller, A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Dordrecht : Springer Science + Business Media B.V., 1969, 184(2016), 3-4 vom: 28. Jan., Seite 866-872 |
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| Übergeordnetes Werk: |
volume:184 ; year:2016 ; number:3-4 ; day:28 ; month:01 ; pages:866-872 |
| Links: |
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| DOI / URN: |
10.1007/s10909-016-1492-1 |
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| Katalog-ID: |
SPR014527677 |
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| 245 | 1 | 0 | |a Exploring Low-Mass Dark Matter with CRESST |
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| 520 | |a Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. | ||
| 650 | 4 | |a Dark matter |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Cryogenic detector |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Low-mass dark matter particles |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Angloher, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bento, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bucci, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Canonica, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Defay, X. |e verfasserin |4 aut | |
| 700 | 1 | |a Erb, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Feilitzsch, F. v. |e verfasserin |4 aut | |
| 700 | 1 | |a Ferreiro Iachellini, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Gorla, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Gütlein, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Hauff, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Jochum, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Kiefer, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Kluck, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Kraus, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Lanfranchi, J. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Loebell, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Münster, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Pagliarone, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Petricca, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Potzel, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Pröbst, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Reindl, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Schäffner, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Schieck, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Schönert, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Seidel, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Stodolsky, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Strandhagen, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Tanzke, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Trinh Thi, H. H. |e verfasserin |4 aut | |
| 700 | 1 | |a Türkoglu, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Uffinger, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Ulrich, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Usherov, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Wawoczny, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Willers, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Wüstrich, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Zöller, A. |e verfasserin |4 aut | |
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10.1007/s10909-016-1492-1 doi (DE-627)SPR014527677 (SPR)s10909-016-1492-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Exploring Low-Mass Dark Matter with CRESST 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 Angloher, G. verfasserin aut Bento, A. verfasserin aut Bucci, C. verfasserin aut Canonica, L. verfasserin aut Defay, X. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Ferreiro Iachellini, N. verfasserin aut Gorla, P. verfasserin aut Gütlein, A. verfasserin aut Hauff, D. verfasserin aut Jochum, J. verfasserin aut Kiefer, M. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Lanfranchi, J. C. verfasserin aut Loebell, J. verfasserin aut Münster, A. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Reindl, F. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Tanzke, A. verfasserin aut Trinh Thi, H. H. verfasserin aut Türkoglu, C. verfasserin aut Uffinger, M. verfasserin aut Ulrich, A. verfasserin aut Usherov, I. verfasserin aut Wawoczny, S. verfasserin aut Willers, M. verfasserin aut Wüstrich, M. verfasserin aut Zöller, A. verfasserin aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 184(2016), 3-4 vom: 28. Jan., Seite 866-872 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 https://dx.doi.org/10.1007/s10909-016-1492-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.09 ASE 33.30 ASE 33.60 ASE AR 184 2016 3-4 28 01 866-872 |
| spelling |
10.1007/s10909-016-1492-1 doi (DE-627)SPR014527677 (SPR)s10909-016-1492-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Exploring Low-Mass Dark Matter with CRESST 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 Angloher, G. verfasserin aut Bento, A. verfasserin aut Bucci, C. verfasserin aut Canonica, L. verfasserin aut Defay, X. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Ferreiro Iachellini, N. verfasserin aut Gorla, P. verfasserin aut Gütlein, A. verfasserin aut Hauff, D. verfasserin aut Jochum, J. verfasserin aut Kiefer, M. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Lanfranchi, J. C. verfasserin aut Loebell, J. verfasserin aut Münster, A. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Reindl, F. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Tanzke, A. verfasserin aut Trinh Thi, H. H. verfasserin aut Türkoglu, C. verfasserin aut Uffinger, M. verfasserin aut Ulrich, A. verfasserin aut Usherov, I. verfasserin aut Wawoczny, S. verfasserin aut Willers, M. verfasserin aut Wüstrich, M. verfasserin aut Zöller, A. verfasserin aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 184(2016), 3-4 vom: 28. Jan., Seite 866-872 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 https://dx.doi.org/10.1007/s10909-016-1492-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.09 ASE 33.30 ASE 33.60 ASE AR 184 2016 3-4 28 01 866-872 |
| allfields_unstemmed |
10.1007/s10909-016-1492-1 doi (DE-627)SPR014527677 (SPR)s10909-016-1492-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Exploring Low-Mass Dark Matter with CRESST 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 Angloher, G. verfasserin aut Bento, A. verfasserin aut Bucci, C. verfasserin aut Canonica, L. verfasserin aut Defay, X. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Ferreiro Iachellini, N. verfasserin aut Gorla, P. verfasserin aut Gütlein, A. verfasserin aut Hauff, D. verfasserin aut Jochum, J. verfasserin aut Kiefer, M. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Lanfranchi, J. C. verfasserin aut Loebell, J. verfasserin aut Münster, A. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Reindl, F. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Tanzke, A. verfasserin aut Trinh Thi, H. H. verfasserin aut Türkoglu, C. verfasserin aut Uffinger, M. verfasserin aut Ulrich, A. verfasserin aut Usherov, I. verfasserin aut Wawoczny, S. verfasserin aut Willers, M. verfasserin aut Wüstrich, M. verfasserin aut Zöller, A. verfasserin aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 184(2016), 3-4 vom: 28. Jan., Seite 866-872 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 https://dx.doi.org/10.1007/s10909-016-1492-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.09 ASE 33.30 ASE 33.60 ASE AR 184 2016 3-4 28 01 866-872 |
| allfieldsGer |
10.1007/s10909-016-1492-1 doi (DE-627)SPR014527677 (SPR)s10909-016-1492-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Exploring Low-Mass Dark Matter with CRESST 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 Angloher, G. verfasserin aut Bento, A. verfasserin aut Bucci, C. verfasserin aut Canonica, L. verfasserin aut Defay, X. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Ferreiro Iachellini, N. verfasserin aut Gorla, P. verfasserin aut Gütlein, A. verfasserin aut Hauff, D. verfasserin aut Jochum, J. verfasserin aut Kiefer, M. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Lanfranchi, J. C. verfasserin aut Loebell, J. verfasserin aut Münster, A. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Reindl, F. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Tanzke, A. verfasserin aut Trinh Thi, H. H. verfasserin aut Türkoglu, C. verfasserin aut Uffinger, M. verfasserin aut Ulrich, A. verfasserin aut Usherov, I. verfasserin aut Wawoczny, S. verfasserin aut Willers, M. verfasserin aut Wüstrich, M. verfasserin aut Zöller, A. verfasserin aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 184(2016), 3-4 vom: 28. Jan., Seite 866-872 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 https://dx.doi.org/10.1007/s10909-016-1492-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.09 ASE 33.30 ASE 33.60 ASE AR 184 2016 3-4 28 01 866-872 |
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10.1007/s10909-016-1492-1 doi (DE-627)SPR014527677 (SPR)s10909-016-1492-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Exploring Low-Mass Dark Matter with CRESST 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 Angloher, G. verfasserin aut Bento, A. verfasserin aut Bucci, C. verfasserin aut Canonica, L. verfasserin aut Defay, X. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Ferreiro Iachellini, N. verfasserin aut Gorla, P. verfasserin aut Gütlein, A. verfasserin aut Hauff, D. verfasserin aut Jochum, J. verfasserin aut Kiefer, M. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Lanfranchi, J. C. verfasserin aut Loebell, J. verfasserin aut Münster, A. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Reindl, F. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Tanzke, A. verfasserin aut Trinh Thi, H. H. verfasserin aut Türkoglu, C. verfasserin aut Uffinger, M. verfasserin aut Ulrich, A. verfasserin aut Usherov, I. verfasserin aut Wawoczny, S. verfasserin aut Willers, M. verfasserin aut Wüstrich, M. verfasserin aut Zöller, A. verfasserin aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 184(2016), 3-4 vom: 28. Jan., Seite 866-872 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 https://dx.doi.org/10.1007/s10909-016-1492-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.09 ASE 33.30 ASE 33.60 ASE AR 184 2016 3-4 28 01 866-872 |
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Enthalten in Journal of low temperature physics 184(2016), 3-4 vom: 28. Jan., Seite 866-872 volume:184 year:2016 number:3-4 day:28 month:01 pages:866-872 |
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Dark matter Cryogenic detector Low-mass dark matter particles |
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Strauss, R. @@aut@@ Angloher, G. @@aut@@ Bento, A. @@aut@@ Bucci, C. @@aut@@ Canonica, L. @@aut@@ Defay, X. @@aut@@ Erb, A. @@aut@@ Feilitzsch, F. v. @@aut@@ Ferreiro Iachellini, N. @@aut@@ Gorla, P. @@aut@@ Gütlein, A. @@aut@@ Hauff, D. @@aut@@ Jochum, J. @@aut@@ Kiefer, M. @@aut@@ Kluck, H. @@aut@@ Kraus, H. @@aut@@ Lanfranchi, J. C. @@aut@@ Loebell, J. @@aut@@ Münster, A. @@aut@@ Pagliarone, C. @@aut@@ Petricca, F. @@aut@@ Potzel, W. @@aut@@ Pröbst, F. @@aut@@ Reindl, F. @@aut@@ Schäffner, K. @@aut@@ Schieck, J. @@aut@@ Schönert, S. @@aut@@ Seidel, W. @@aut@@ Stodolsky, L. @@aut@@ Strandhagen, C. @@aut@@ Tanzke, A. @@aut@@ Trinh Thi, H. H. @@aut@@ Türkoglu, C. @@aut@@ Uffinger, M. @@aut@@ Ulrich, A. @@aut@@ Usherov, I. @@aut@@ Wawoczny, S. @@aut@@ Willers, M. @@aut@@ Wüstrich, M. @@aut@@ Zöller, A. @@aut@@ |
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|
| author |
Strauss, R. |
| spellingShingle |
Strauss, R. ddc 530 bkl 33.09 bkl 33.30 bkl 33.60 misc Dark matter misc Cryogenic detector misc Low-mass dark matter particles Exploring Low-Mass Dark Matter with CRESST |
| authorStr |
Strauss, R. |
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530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Exploring Low-Mass Dark Matter with CRESST Dark matter (dpeaa)DE-He213 Cryogenic detector (dpeaa)DE-He213 Low-mass dark matter particles (dpeaa)DE-He213 |
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Exploring Low-Mass Dark Matter with CRESST |
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Exploring Low-Mass Dark Matter with CRESST |
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Strauss, R. |
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Strauss, R. Angloher, G. Bento, A. Bucci, C. Canonica, L. Defay, X. Erb, A. Feilitzsch, F. v. Ferreiro Iachellini, N. Gorla, P. Gütlein, A. Hauff, D. Jochum, J. Kiefer, M. Kluck, H. Kraus, H. Lanfranchi, J. C. Loebell, J. Münster, A. Pagliarone, C. Petricca, F. Potzel, W. Pröbst, F. Reindl, F. Schäffner, K. Schieck, J. Schönert, S. Seidel, W. Stodolsky, L. Strandhagen, C. Tanzke, A. Trinh Thi, H. H. Türkoglu, C. Uffinger, M. Ulrich, A. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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exploring low-mass dark matter with cresst |
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Exploring Low-Mass Dark Matter with CRESST |
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Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. |
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Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. |
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Abstract The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, whose second phase has been successfully finished in summer 2015, aims at the direct detection of dark matter particles. The intrinsic radiopurity of CaWO%$_4%$ crystals, the capability to reject recoil events from alpha-surface contamination, and the energy threshold were significantly improved compared to previous runs of the experiment. A moderate exposure of 29 kg-days acquired by one %$\sim %$250 g CaWO%$_4%$ detector provides competitive limits on the spin-independent dark matter particle-nucleon cross section and probes a new region of parameter space for dark matter particle masses below 3 GeV/c%$^2%$. The potential for low-mass dark matter particle search can be further exploited by a new detector design planned for CRESST-III. We describe the experimental strategy for the near future and give projections for the sensitivity. |
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Exploring Low-Mass Dark Matter with CRESST |
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Angloher, G. Bento, A. Bucci, C. Canonica, L. Defay, X. Erb, A. Feilitzsch, F. v. Ferreiro Iachellini, N. Gorla, P. Gütlein, A. Hauff, D. Jochum, J. Kiefer, M. Kluck, H. Kraus, H. Lanfranchi, J. C. Loebell, J. Münster, A. Pagliarone, C. Petricca, F. Potzel, W. Pröbst, F. Reindl, F. Schäffner, K. Schieck, J. Schönert, S. Seidel, W. Stodolsky, L. Strandhagen, C. Tanzke, A. Trinh Thi, H. H. Türkoglu, C. Uffinger, M. Ulrich, A. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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