Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground
Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Angloher, G. [verfasserIn] Bauer, P. [verfasserIn] Bento, A. [verfasserIn] Bucci, C. [verfasserIn] Canonica, L. [verfasserIn] Defay, X. [verfasserIn] Erb, A. [verfasserIn] Feilitzsch, F. v. [verfasserIn] Iachellini, N. Ferreiro [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] Langenkämper, A. [verfasserIn] Loebell, J. [verfasserIn] Mancuso, M. [verfasserIn] Mondragon, E. [verfasserIn] Münster, A. [verfasserIn] Oberauer, L. [verfasserIn] Pagliarone, C. [verfasserIn] Petricca, F. [verfasserIn] Potzel, W. [verfasserIn] Pröbst, F. [verfasserIn] Puig, R. [verfasserIn] Reindl, F. [verfasserIn] Rothe, J. [verfasserIn] Schäffner, K. [verfasserIn] Schieck, J. [verfasserIn] Schönert, S. [verfasserIn] Seidel, W. [verfasserIn] Stahlberg, M. [verfasserIn] Stodolsky, L. [verfasserIn] Strandhagen, C. [verfasserIn] Strauss, R. [verfasserIn] Tanzke, A. [verfasserIn] Thi, H. H. Trinh [verfasserIn] Türkoǧlu, 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: |
2017 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 1998, 77(2017), 9 vom: 22. Sept. |
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| Übergeordnetes Werk: |
volume:77 ; year:2017 ; number:9 ; day:22 ; month:09 |
| Links: |
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| DOI / URN: |
10.1140/epjc/s10052-017-5223-9 |
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| Katalog-ID: |
SPR00836382X |
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| 100 | 1 | |a Angloher, G. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
| 264 | 1 | |c 2017 | |
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| 520 | |a Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. | ||
| 700 | 1 | |a Bauer, P. |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 Iachellini, N. Ferreiro |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 Langenkämper, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Loebell, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Mancuso, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Mondragon, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Münster, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Oberauer, L. |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 Puig, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Reindl, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Rothe, J. |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 Stahlberg, M. |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 Strauss, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Tanzke, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Thi, H. H. Trinh |e verfasserin |4 aut | |
| 700 | 1 | |a Türkoǧlu, 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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10.1140/epjc/s10052-017-5223-9 doi (DE-627)SPR00836382X (SPR)s10052-017-5223-9-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Angloher, G. verfasserin aut Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. Bauer, P. 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 Iachellini, N. Ferreiro 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 Langenkämper, A. verfasserin aut Loebell, J. verfasserin aut Mancuso, M. verfasserin aut Mondragon, E. verfasserin aut Münster, A. verfasserin aut Oberauer, L. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Puig, R. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Tanzke, A. verfasserin aut Thi, H. H. Trinh verfasserin aut Türkoǧlu, 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 The European physical journal Berlin : Springer, 1998 77(2017), 9 vom: 22. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:9 day:22 month:09 https://dx.doi.org/10.1140/epjc/s10052-017-5223-9 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 77 2017 9 22 09 |
| spelling |
10.1140/epjc/s10052-017-5223-9 doi (DE-627)SPR00836382X (SPR)s10052-017-5223-9-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Angloher, G. verfasserin aut Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. Bauer, P. 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 Iachellini, N. Ferreiro 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 Langenkämper, A. verfasserin aut Loebell, J. verfasserin aut Mancuso, M. verfasserin aut Mondragon, E. verfasserin aut Münster, A. verfasserin aut Oberauer, L. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Puig, R. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Tanzke, A. verfasserin aut Thi, H. H. Trinh verfasserin aut Türkoǧlu, 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 The European physical journal Berlin : Springer, 1998 77(2017), 9 vom: 22. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:9 day:22 month:09 https://dx.doi.org/10.1140/epjc/s10052-017-5223-9 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 77 2017 9 22 09 |
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10.1140/epjc/s10052-017-5223-9 doi (DE-627)SPR00836382X (SPR)s10052-017-5223-9-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Angloher, G. verfasserin aut Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. Bauer, P. 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 Iachellini, N. Ferreiro 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 Langenkämper, A. verfasserin aut Loebell, J. verfasserin aut Mancuso, M. verfasserin aut Mondragon, E. verfasserin aut Münster, A. verfasserin aut Oberauer, L. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Puig, R. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Tanzke, A. verfasserin aut Thi, H. H. Trinh verfasserin aut Türkoǧlu, 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 The European physical journal Berlin : Springer, 1998 77(2017), 9 vom: 22. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:9 day:22 month:09 https://dx.doi.org/10.1140/epjc/s10052-017-5223-9 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 77 2017 9 22 09 |
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10.1140/epjc/s10052-017-5223-9 doi (DE-627)SPR00836382X (SPR)s10052-017-5223-9-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Angloher, G. verfasserin aut Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. Bauer, P. 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 Iachellini, N. Ferreiro 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 Langenkämper, A. verfasserin aut Loebell, J. verfasserin aut Mancuso, M. verfasserin aut Mondragon, E. verfasserin aut Münster, A. verfasserin aut Oberauer, L. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Puig, R. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Tanzke, A. verfasserin aut Thi, H. H. Trinh verfasserin aut Türkoǧlu, 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 The European physical journal Berlin : Springer, 1998 77(2017), 9 vom: 22. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:9 day:22 month:09 https://dx.doi.org/10.1140/epjc/s10052-017-5223-9 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 77 2017 9 22 09 |
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10.1140/epjc/s10052-017-5223-9 doi (DE-627)SPR00836382X (SPR)s10052-017-5223-9-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Angloher, G. verfasserin aut Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. Bauer, P. 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 Iachellini, N. Ferreiro 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 Langenkämper, A. verfasserin aut Loebell, J. verfasserin aut Mancuso, M. verfasserin aut Mondragon, E. verfasserin aut Münster, A. verfasserin aut Oberauer, L. verfasserin aut Pagliarone, C. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Pröbst, F. verfasserin aut Puig, R. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Seidel, W. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Tanzke, A. verfasserin aut Thi, H. H. Trinh verfasserin aut Türkoǧlu, 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 The European physical journal Berlin : Springer, 1998 77(2017), 9 vom: 22. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:9 day:22 month:09 https://dx.doi.org/10.1140/epjc/s10052-017-5223-9 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 77 2017 9 22 09 |
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Angloher, G. @@aut@@ Bauer, P. @@aut@@ Bento, A. @@aut@@ Bucci, C. @@aut@@ Canonica, L. @@aut@@ Defay, X. @@aut@@ Erb, A. @@aut@@ Feilitzsch, F. v. @@aut@@ Iachellini, N. Ferreiro @@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@@ Langenkämper, A. @@aut@@ Loebell, J. @@aut@@ Mancuso, M. @@aut@@ Mondragon, E. @@aut@@ Münster, A. @@aut@@ Oberauer, L. @@aut@@ Pagliarone, C. @@aut@@ Petricca, F. @@aut@@ Potzel, W. @@aut@@ Pröbst, F. @@aut@@ Puig, R. @@aut@@ Reindl, F. @@aut@@ Rothe, J. @@aut@@ Schäffner, K. @@aut@@ Schieck, J. @@aut@@ Schönert, S. @@aut@@ Seidel, W. @@aut@@ Stahlberg, M. @@aut@@ Stodolsky, L. @@aut@@ Strandhagen, C. @@aut@@ Strauss, R. @@aut@@ Tanzke, A. @@aut@@ Thi, H. H. Trinh @@aut@@ Türkoǧlu, 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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Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. 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Angloher, G. |
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Angloher, G. ddc 530 bkl 33.50 Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
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530 ASE 33.50 bkl Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
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Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
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Angloher, G. Bauer, P. Bento, A. Bucci, C. Canonica, L. Defay, X. Erb, A. Feilitzsch, F. v. Iachellini, N. Ferreiro Gorla, P. Gütlein, A. Hauff, D. Jochum, J. Kiefer, M. Kluck, H. Kraus, H. Lanfranchi, J.-C. Langenkämper, A. Loebell, J. Mancuso, M. Mondragon, E. Münster, A. Oberauer, L. Pagliarone, C. Petricca, F. Potzel, W. Pröbst, F. Puig, R. Reindl, F. Rothe, J. Schäffner, K. Schieck, J. Schönert, S. Seidel, W. Stahlberg, M. Stodolsky, L. Strandhagen, C. Strauss, R. Tanzke, A. Thi, H. H. Trinh Türkoǧlu, C. Uffinger, M. Ulrich, A. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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Angloher, G. |
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results on mev-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
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Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
| abstract |
Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. |
| abstractGer |
Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. |
| abstract_unstemmed |
Abstract Models for light dark matter particles with masses below 1 GeV/c%$^2%$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector performance to detect these particles and extend the direct dark matter search program of CRESST. A prototype 0.5 g sapphire detector developed for the %$\nu %$-cleus experiment has achieved an energy threshold of %$E_{th}=(19.7\pm 0.9)%$ eV. This is one order of magnitude lower than for previous devices and independent of the type of particle interaction. The result presented here is obtained in a setup above ground without significant shielding against ambient and cosmogenic radiation. Although operated in a high-background environment, the detector probes a new range of light-mass dark matter particles previously not accessible by direct searches. We report the first limit on the spin-independent dark matter particle-nucleon cross section for masses between 140 and 500 MeV/c%$^2%$. |
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Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground |
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Bauer, P. Bento, A. Bucci, C. Canonica, L. Defay, X. Erb, A. Feilitzsch, F. v. Iachellini, N. Ferreiro Gorla, P. Gütlein, A. Hauff, D. Jochum, J. Kiefer, M. Kluck, H. Kraus, H. Lanfranchi, J.-C. Langenkämper, A. Loebell, J. Mancuso, M. Mondragon, E. Münster, A. Oberauer, L. Pagliarone, C. Petricca, F. Potzel, W. Pröbst, F. Puig, R. Reindl, F. Rothe, J. Schäffner, K. Schieck, J. Schönert, S. Seidel, W. Stahlberg, M. Stodolsky, L. Strandhagen, C. Strauss, R. Tanzke, A. Thi, H. H. Trinh Türkoǧlu, C. Uffinger, M. Ulrich, A. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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Bauer, P. Bento, A. Bucci, C. Canonica, L. Defay, X. Erb, A. Feilitzsch, F. v. Iachellini, N. Ferreiro Gorla, P. Gütlein, A. Hauff, D. Jochum, J. Kiefer, M. Kluck, H. Kraus, H. Lanfranchi, J.-C. Langenkämper, A. Loebell, J. Mancuso, M. Mondragon, E. Münster, A. Oberauer, L. Pagliarone, C. Petricca, F. Potzel, W. Pröbst, F. Puig, R. Reindl, F. Rothe, J. Schäffner, K. Schieck, J. Schönert, S. Seidel, W. Stahlberg, M. Stodolsky, L. Strandhagen, C. Strauss, R. Tanzke, A. Thi, H. H. Trinh Türkoǧlu, C. Uffinger, M. Ulrich, A. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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| score |
7.4019337 |