Light dark matter search using a diamond cryogenic detector
Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the result...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Angloher, G. [verfasserIn] Banik, S. [verfasserIn] Benato, G. [verfasserIn] Bento, A. [verfasserIn] Bertolini, A. [verfasserIn] Breier, R. [verfasserIn] Bucci, C. [verfasserIn] Burkhart, J. [verfasserIn] Canonica, L. [verfasserIn] D’Addabbo, A. [verfasserIn] Lorenzo, S. Di [verfasserIn] Einfalt, L. [verfasserIn] Erb, A. [verfasserIn] Feilitzsch, F. v. [verfasserIn] Fichtinger, S. [verfasserIn] Fuchs, D. [verfasserIn] Garai, A. [verfasserIn] Ghete, V. M. [verfasserIn] Gorla, P. [verfasserIn] Guillaumon, P. V. [verfasserIn] Gupta, S. [verfasserIn] Hauff, D. [verfasserIn] Jes̆kovský, M. [verfasserIn] Jochum, J. [verfasserIn] Kaznacheeva, M. [verfasserIn] Kinast, A. [verfasserIn] Kluck, H. [verfasserIn] Kraus, H. [verfasserIn] Kuckuk, S. [verfasserIn] Langenkämper, A. [verfasserIn] Mancuso, M. [verfasserIn] Marini, L. [verfasserIn] Mauri, B. [verfasserIn] Meyer, L. [verfasserIn] Mokina, V. [verfasserIn] Olmi, M. [verfasserIn] Ortmann, T. [verfasserIn] Pagliarone, C. [verfasserIn] Pattavina, L. [verfasserIn] Petricca, F. [verfasserIn] Potzel, W. [verfasserIn] Povinec, P. [verfasserIn] Pröbst, F. [verfasserIn] Pucci, F. [verfasserIn] Reindl, F. [verfasserIn] Rothe, J. [verfasserIn] Schäffner, K. [verfasserIn] Schieck, J. [verfasserIn] Schönert, S. [verfasserIn] Schwertner, C. [verfasserIn] Stahlberg, M. [verfasserIn] Stodolsky, L. [verfasserIn] Strandhagen, C. [verfasserIn] Strauss, R. [verfasserIn] Usherov, I. [verfasserIn] Wagner, F. [verfasserIn] Willers, M. [verfasserIn] Zema, V. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2024 |
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| Anmerkung: |
© The Author(s) 2024 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Springer Berlin Heidelberg, 1998, 84(2024), 3 vom: 27. März |
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| Übergeordnetes Werk: |
volume:84 ; year:2024 ; number:3 ; day:27 ; month:03 |
| Links: |
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| DOI / URN: |
10.1140/epjc/s10052-024-12647-3 |
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| Katalog-ID: |
SPR055317626 |
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| 100 | 1 | |a Angloher, G. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Light dark matter search using a diamond cryogenic detector |
| 264 | 1 | |c 2024 | |
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| 500 | |a © The Author(s) 2024 | ||
| 520 | |a Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. | ||
| 700 | 1 | |a Banik, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Benato, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bento, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bertolini, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Breier, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Bucci, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Burkhart, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Canonica, L. |e verfasserin |4 aut | |
| 700 | 1 | |a D’Addabbo, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Lorenzo, S. Di |e verfasserin |4 aut | |
| 700 | 1 | |a Einfalt, L. |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 Fichtinger, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Fuchs, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Garai, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Ghete, V. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Gorla, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Guillaumon, P. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Gupta, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Hauff, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Jes̆kovský, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Jochum, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Kaznacheeva, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Kinast, A. |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 Kuckuk, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Langenkämper, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Mancuso, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Marini, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Mauri, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Meyer, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Mokina, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Olmi, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Ortmann, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Pagliarone, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Pattavina, L. |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 Povinec, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Pröbst, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Pucci, F. |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 Schwertner, C. |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 Usherov, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Wagner, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Willers, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Zema, V. |e verfasserin |4 aut | |
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10.1140/epjc/s10052-024-12647-3 doi (DE-627)SPR055317626 (SPR)s10052-024-12647-3-e DE-627 ger DE-627 rakwb eng 530 VZ 33.50 bkl Angloher, G. verfasserin aut Light dark matter search using a diamond cryogenic detector 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. Banik, S. verfasserin aut Benato, G. verfasserin aut Bento, A. verfasserin aut Bertolini, A. verfasserin aut Breier, R. verfasserin aut Bucci, C. verfasserin aut Burkhart, J. verfasserin aut Canonica, L. verfasserin aut D’Addabbo, A. verfasserin aut Lorenzo, S. Di verfasserin aut Einfalt, L. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Fichtinger, S. verfasserin aut Fuchs, D. verfasserin aut Garai, A. verfasserin aut Ghete, V. M. verfasserin aut Gorla, P. verfasserin aut Guillaumon, P. V. verfasserin aut Gupta, S. verfasserin aut Hauff, D. verfasserin aut Jes̆kovský, M. verfasserin aut Jochum, J. verfasserin aut Kaznacheeva, M. verfasserin aut Kinast, A. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Kuckuk, S. verfasserin aut Langenkämper, A. verfasserin aut Mancuso, M. verfasserin aut Marini, L. verfasserin aut Mauri, B. verfasserin aut Meyer, L. verfasserin aut Mokina, V. verfasserin aut Olmi, M. verfasserin aut Ortmann, T. verfasserin aut Pagliarone, C. verfasserin aut Pattavina, L. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Povinec, P. verfasserin aut Pröbst, F. verfasserin aut Pucci, F. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Schwertner, C. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Usherov, I. verfasserin aut Wagner, F. verfasserin aut Willers, M. verfasserin aut Zema, V. verfasserin aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 84(2024), 3 vom: 27. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:84 year:2024 number:3 day:27 month:03 https://dx.doi.org/10.1140/epjc/s10052-024-12647-3 X:SPRINGER Resolving-System kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER 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 VZ AR 84 2024 3 27 03 |
| spelling |
10.1140/epjc/s10052-024-12647-3 doi (DE-627)SPR055317626 (SPR)s10052-024-12647-3-e DE-627 ger DE-627 rakwb eng 530 VZ 33.50 bkl Angloher, G. verfasserin aut Light dark matter search using a diamond cryogenic detector 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. Banik, S. verfasserin aut Benato, G. verfasserin aut Bento, A. verfasserin aut Bertolini, A. verfasserin aut Breier, R. verfasserin aut Bucci, C. verfasserin aut Burkhart, J. verfasserin aut Canonica, L. verfasserin aut D’Addabbo, A. verfasserin aut Lorenzo, S. Di verfasserin aut Einfalt, L. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Fichtinger, S. verfasserin aut Fuchs, D. verfasserin aut Garai, A. verfasserin aut Ghete, V. M. verfasserin aut Gorla, P. verfasserin aut Guillaumon, P. V. verfasserin aut Gupta, S. verfasserin aut Hauff, D. verfasserin aut Jes̆kovský, M. verfasserin aut Jochum, J. verfasserin aut Kaznacheeva, M. verfasserin aut Kinast, A. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Kuckuk, S. verfasserin aut Langenkämper, A. verfasserin aut Mancuso, M. verfasserin aut Marini, L. verfasserin aut Mauri, B. verfasserin aut Meyer, L. verfasserin aut Mokina, V. verfasserin aut Olmi, M. verfasserin aut Ortmann, T. verfasserin aut Pagliarone, C. verfasserin aut Pattavina, L. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Povinec, P. verfasserin aut Pröbst, F. verfasserin aut Pucci, F. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Schwertner, C. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Usherov, I. verfasserin aut Wagner, F. verfasserin aut Willers, M. verfasserin aut Zema, V. verfasserin aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 84(2024), 3 vom: 27. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:84 year:2024 number:3 day:27 month:03 https://dx.doi.org/10.1140/epjc/s10052-024-12647-3 X:SPRINGER Resolving-System kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER 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 VZ AR 84 2024 3 27 03 |
| allfields_unstemmed |
10.1140/epjc/s10052-024-12647-3 doi (DE-627)SPR055317626 (SPR)s10052-024-12647-3-e DE-627 ger DE-627 rakwb eng 530 VZ 33.50 bkl Angloher, G. verfasserin aut Light dark matter search using a diamond cryogenic detector 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. Banik, S. verfasserin aut Benato, G. verfasserin aut Bento, A. verfasserin aut Bertolini, A. verfasserin aut Breier, R. verfasserin aut Bucci, C. verfasserin aut Burkhart, J. verfasserin aut Canonica, L. verfasserin aut D’Addabbo, A. verfasserin aut Lorenzo, S. Di verfasserin aut Einfalt, L. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Fichtinger, S. verfasserin aut Fuchs, D. verfasserin aut Garai, A. verfasserin aut Ghete, V. M. verfasserin aut Gorla, P. verfasserin aut Guillaumon, P. V. verfasserin aut Gupta, S. verfasserin aut Hauff, D. verfasserin aut Jes̆kovský, M. verfasserin aut Jochum, J. verfasserin aut Kaznacheeva, M. verfasserin aut Kinast, A. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Kuckuk, S. verfasserin aut Langenkämper, A. verfasserin aut Mancuso, M. verfasserin aut Marini, L. verfasserin aut Mauri, B. verfasserin aut Meyer, L. verfasserin aut Mokina, V. verfasserin aut Olmi, M. verfasserin aut Ortmann, T. verfasserin aut Pagliarone, C. verfasserin aut Pattavina, L. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Povinec, P. verfasserin aut Pröbst, F. verfasserin aut Pucci, F. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Schwertner, C. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Usherov, I. verfasserin aut Wagner, F. verfasserin aut Willers, M. verfasserin aut Zema, V. verfasserin aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 84(2024), 3 vom: 27. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:84 year:2024 number:3 day:27 month:03 https://dx.doi.org/10.1140/epjc/s10052-024-12647-3 X:SPRINGER Resolving-System kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER 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 VZ AR 84 2024 3 27 03 |
| allfieldsGer |
10.1140/epjc/s10052-024-12647-3 doi (DE-627)SPR055317626 (SPR)s10052-024-12647-3-e DE-627 ger DE-627 rakwb eng 530 VZ 33.50 bkl Angloher, G. verfasserin aut Light dark matter search using a diamond cryogenic detector 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. Banik, S. verfasserin aut Benato, G. verfasserin aut Bento, A. verfasserin aut Bertolini, A. verfasserin aut Breier, R. verfasserin aut Bucci, C. verfasserin aut Burkhart, J. verfasserin aut Canonica, L. verfasserin aut D’Addabbo, A. verfasserin aut Lorenzo, S. Di verfasserin aut Einfalt, L. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Fichtinger, S. verfasserin aut Fuchs, D. verfasserin aut Garai, A. verfasserin aut Ghete, V. M. verfasserin aut Gorla, P. verfasserin aut Guillaumon, P. V. verfasserin aut Gupta, S. verfasserin aut Hauff, D. verfasserin aut Jes̆kovský, M. verfasserin aut Jochum, J. verfasserin aut Kaznacheeva, M. verfasserin aut Kinast, A. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Kuckuk, S. verfasserin aut Langenkämper, A. verfasserin aut Mancuso, M. verfasserin aut Marini, L. verfasserin aut Mauri, B. verfasserin aut Meyer, L. verfasserin aut Mokina, V. verfasserin aut Olmi, M. verfasserin aut Ortmann, T. verfasserin aut Pagliarone, C. verfasserin aut Pattavina, L. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Povinec, P. verfasserin aut Pröbst, F. verfasserin aut Pucci, F. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Schwertner, C. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Usherov, I. verfasserin aut Wagner, F. verfasserin aut Willers, M. verfasserin aut Zema, V. verfasserin aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 84(2024), 3 vom: 27. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:84 year:2024 number:3 day:27 month:03 https://dx.doi.org/10.1140/epjc/s10052-024-12647-3 X:SPRINGER Resolving-System kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER 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 VZ AR 84 2024 3 27 03 |
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10.1140/epjc/s10052-024-12647-3 doi (DE-627)SPR055317626 (SPR)s10052-024-12647-3-e DE-627 ger DE-627 rakwb eng 530 VZ 33.50 bkl Angloher, G. verfasserin aut Light dark matter search using a diamond cryogenic detector 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. Banik, S. verfasserin aut Benato, G. verfasserin aut Bento, A. verfasserin aut Bertolini, A. verfasserin aut Breier, R. verfasserin aut Bucci, C. verfasserin aut Burkhart, J. verfasserin aut Canonica, L. verfasserin aut D’Addabbo, A. verfasserin aut Lorenzo, S. Di verfasserin aut Einfalt, L. verfasserin aut Erb, A. verfasserin aut Feilitzsch, F. v. verfasserin aut Fichtinger, S. verfasserin aut Fuchs, D. verfasserin aut Garai, A. verfasserin aut Ghete, V. M. verfasserin aut Gorla, P. verfasserin aut Guillaumon, P. V. verfasserin aut Gupta, S. verfasserin aut Hauff, D. verfasserin aut Jes̆kovský, M. verfasserin aut Jochum, J. verfasserin aut Kaznacheeva, M. verfasserin aut Kinast, A. verfasserin aut Kluck, H. verfasserin aut Kraus, H. verfasserin aut Kuckuk, S. verfasserin aut Langenkämper, A. verfasserin aut Mancuso, M. verfasserin aut Marini, L. verfasserin aut Mauri, B. verfasserin aut Meyer, L. verfasserin aut Mokina, V. verfasserin aut Olmi, M. verfasserin aut Ortmann, T. verfasserin aut Pagliarone, C. verfasserin aut Pattavina, L. verfasserin aut Petricca, F. verfasserin aut Potzel, W. verfasserin aut Povinec, P. verfasserin aut Pröbst, F. verfasserin aut Pucci, F. verfasserin aut Reindl, F. verfasserin aut Rothe, J. verfasserin aut Schäffner, K. verfasserin aut Schieck, J. verfasserin aut Schönert, S. verfasserin aut Schwertner, C. verfasserin aut Stahlberg, M. verfasserin aut Stodolsky, L. verfasserin aut Strandhagen, C. verfasserin aut Strauss, R. verfasserin aut Usherov, I. verfasserin aut Wagner, F. verfasserin aut Willers, M. verfasserin aut Zema, V. verfasserin aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 84(2024), 3 vom: 27. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:84 year:2024 number:3 day:27 month:03 https://dx.doi.org/10.1140/epjc/s10052-024-12647-3 X:SPRINGER Resolving-System kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER 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 VZ AR 84 2024 3 27 03 |
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Angloher, G. @@aut@@ Banik, S. @@aut@@ Benato, G. @@aut@@ Bento, A. @@aut@@ Bertolini, A. @@aut@@ Breier, R. @@aut@@ Bucci, C. @@aut@@ Burkhart, J. @@aut@@ Canonica, L. @@aut@@ D’Addabbo, A. @@aut@@ Lorenzo, S. Di @@aut@@ Einfalt, L. @@aut@@ Erb, A. @@aut@@ Feilitzsch, F. v. @@aut@@ Fichtinger, S. @@aut@@ Fuchs, D. @@aut@@ Garai, A. @@aut@@ Ghete, V. M. @@aut@@ Gorla, P. @@aut@@ Guillaumon, P. V. @@aut@@ Gupta, S. @@aut@@ Hauff, D. @@aut@@ Jes̆kovský, M. @@aut@@ Jochum, J. @@aut@@ Kaznacheeva, M. @@aut@@ Kinast, A. @@aut@@ Kluck, H. @@aut@@ Kraus, H. @@aut@@ Kuckuk, S. @@aut@@ Langenkämper, A. @@aut@@ Mancuso, M. @@aut@@ Marini, L. @@aut@@ Mauri, B. @@aut@@ Meyer, L. @@aut@@ Mokina, V. @@aut@@ Olmi, M. @@aut@@ Ortmann, T. @@aut@@ Pagliarone, C. @@aut@@ Pattavina, L. @@aut@@ Petricca, F. @@aut@@ Potzel, W. @@aut@@ Povinec, P. @@aut@@ Pröbst, F. @@aut@@ Pucci, F. @@aut@@ Reindl, F. @@aut@@ Rothe, J. @@aut@@ Schäffner, K. @@aut@@ Schieck, J. @@aut@@ Schönert, S. @@aut@@ Schwertner, C. @@aut@@ Stahlberg, M. @@aut@@ Stodolsky, L. @@aut@@ Strandhagen, C. @@aut@@ Strauss, R. @@aut@@ Usherov, I. @@aut@@ Wagner, F. @@aut@@ Willers, M. @@aut@@ Zema, V. @@aut@@ |
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Angloher, G. ddc 530 bkl 33.50 Light dark matter search using a diamond cryogenic detector |
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Angloher, G. Banik, S. Benato, G. Bento, A. Bertolini, A. Breier, R. Bucci, C. Burkhart, J. Canonica, L. D’Addabbo, A. Lorenzo, S. Di Einfalt, L. Erb, A. Feilitzsch, F. v. Fichtinger, S. Fuchs, D. Garai, A. Ghete, V. M. Gorla, P. Guillaumon, P. V. Gupta, S. Hauff, D. Jes̆kovský, M. Jochum, J. Kaznacheeva, M. Kinast, A. Kluck, H. Kraus, H. Kuckuk, S. Langenkämper, A. Mancuso, M. Marini, L. Mauri, B. Meyer, L. Mokina, V. Olmi, M. Ortmann, T. Pagliarone, C. Pattavina, L. Petricca, F. Potzel, W. Povinec, P. Pröbst, F. Pucci, F. Reindl, F. Rothe, J. Schäffner, K. Schieck, J. Schönert, S. Schwertner, C. Stahlberg, M. Stodolsky, L. Strandhagen, C. Strauss, R. Usherov, I. Wagner, F. Willers, M. Zema, V. |
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Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. © The Author(s) 2024 |
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Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. © The Author(s) 2024 |
| abstract_unstemmed |
Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments. © The Author(s) 2024 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR055317626</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240508064652.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240328s2024 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1140/epjc/s10052-024-12647-3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR055317626</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s10052-024-12647-3-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">33.50</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Angloher, G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Light dark matter search using a diamond cryogenic detector</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2024</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Author(s) 2024</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$. 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