Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST
Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Strauss, R. [verfasserIn] Ciemniak, C. [verfasserIn] Deuter, G. [verfasserIn] Feilitzsch, F. V. [verfasserIn] Gütlein, A. [verfasserIn] Hagn, H. [verfasserIn] Hellgartner, D. [verfasserIn] Jochum, J. [verfasserIn] Lanfranchi, J.-C. [verfasserIn] Münster, A. [verfasserIn] Potzel, W. [verfasserIn] Roth, S. [verfasserIn] Rottler, K. [verfasserIn] Sailer, C. [verfasserIn] Scholl, S. [verfasserIn] Sivers, M. V. [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: |
2014 |
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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, 176(2014), 5-6 vom: 23. Jan., Seite 905-910 |
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| Übergeordnetes Werk: |
volume:176 ; year:2014 ; number:5-6 ; day:23 ; month:01 ; pages:905-910 |
| Links: |
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| DOI / URN: |
10.1007/s10909-013-1075-3 |
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| Katalog-ID: |
SPR014523485 |
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| 100 | 1 | |a Strauss, R. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
| 264 | 1 | |c 2014 | |
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| 520 | |a Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). | ||
| 650 | 4 | |a Dark matter |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a CRESST |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Quenching factor |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a CaWO |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Ciemniak, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Deuter, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Feilitzsch, F. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Gütlein, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Hagn, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Hellgartner, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Jochum, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Lanfranchi, J.-C. |e verfasserin |4 aut | |
| 700 | 1 | |a Münster, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Potzel, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Roth, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Rottler, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Sailer, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Scholl, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Sivers, M. V. |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/s10909-013-1075-3 doi (DE-627)SPR014523485 (SPR)s10909-013-1075-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 Ciemniak, C. verfasserin aut Deuter, G. verfasserin aut Feilitzsch, F. V. verfasserin aut Gütlein, A. verfasserin aut Hagn, H. verfasserin aut Hellgartner, D. verfasserin aut Jochum, J. verfasserin aut Lanfranchi, J.-C. verfasserin aut Münster, A. verfasserin aut Potzel, W. verfasserin aut Roth, S. verfasserin aut Rottler, K. verfasserin aut Sailer, C. verfasserin aut Scholl, S. verfasserin aut Sivers, M. V. 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 176(2014), 5-6 vom: 23. Jan., Seite 905-910 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 https://dx.doi.org/10.1007/s10909-013-1075-3 lizenzpflichtig 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 176 2014 5-6 23 01 905-910 |
| spelling |
10.1007/s10909-013-1075-3 doi (DE-627)SPR014523485 (SPR)s10909-013-1075-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 Ciemniak, C. verfasserin aut Deuter, G. verfasserin aut Feilitzsch, F. V. verfasserin aut Gütlein, A. verfasserin aut Hagn, H. verfasserin aut Hellgartner, D. verfasserin aut Jochum, J. verfasserin aut Lanfranchi, J.-C. verfasserin aut Münster, A. verfasserin aut Potzel, W. verfasserin aut Roth, S. verfasserin aut Rottler, K. verfasserin aut Sailer, C. verfasserin aut Scholl, S. verfasserin aut Sivers, M. V. 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 176(2014), 5-6 vom: 23. Jan., Seite 905-910 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 https://dx.doi.org/10.1007/s10909-013-1075-3 lizenzpflichtig 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 176 2014 5-6 23 01 905-910 |
| allfields_unstemmed |
10.1007/s10909-013-1075-3 doi (DE-627)SPR014523485 (SPR)s10909-013-1075-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 Ciemniak, C. verfasserin aut Deuter, G. verfasserin aut Feilitzsch, F. V. verfasserin aut Gütlein, A. verfasserin aut Hagn, H. verfasserin aut Hellgartner, D. verfasserin aut Jochum, J. verfasserin aut Lanfranchi, J.-C. verfasserin aut Münster, A. verfasserin aut Potzel, W. verfasserin aut Roth, S. verfasserin aut Rottler, K. verfasserin aut Sailer, C. verfasserin aut Scholl, S. verfasserin aut Sivers, M. V. 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 176(2014), 5-6 vom: 23. Jan., Seite 905-910 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 https://dx.doi.org/10.1007/s10909-013-1075-3 lizenzpflichtig 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 176 2014 5-6 23 01 905-910 |
| allfieldsGer |
10.1007/s10909-013-1075-3 doi (DE-627)SPR014523485 (SPR)s10909-013-1075-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 Ciemniak, C. verfasserin aut Deuter, G. verfasserin aut Feilitzsch, F. V. verfasserin aut Gütlein, A. verfasserin aut Hagn, H. verfasserin aut Hellgartner, D. verfasserin aut Jochum, J. verfasserin aut Lanfranchi, J.-C. verfasserin aut Münster, A. verfasserin aut Potzel, W. verfasserin aut Roth, S. verfasserin aut Rottler, K. verfasserin aut Sailer, C. verfasserin aut Scholl, S. verfasserin aut Sivers, M. V. 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 176(2014), 5-6 vom: 23. Jan., Seite 905-910 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 https://dx.doi.org/10.1007/s10909-013-1075-3 lizenzpflichtig 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 176 2014 5-6 23 01 905-910 |
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10.1007/s10909-013-1075-3 doi (DE-627)SPR014523485 (SPR)s10909-013-1075-3-e DE-627 ger DE-627 rakwb eng 530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Strauss, R. verfasserin aut Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 Ciemniak, C. verfasserin aut Deuter, G. verfasserin aut Feilitzsch, F. V. verfasserin aut Gütlein, A. verfasserin aut Hagn, H. verfasserin aut Hellgartner, D. verfasserin aut Jochum, J. verfasserin aut Lanfranchi, J.-C. verfasserin aut Münster, A. verfasserin aut Potzel, W. verfasserin aut Roth, S. verfasserin aut Rottler, K. verfasserin aut Sailer, C. verfasserin aut Scholl, S. verfasserin aut Sivers, M. V. 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 176(2014), 5-6 vom: 23. Jan., Seite 905-910 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 https://dx.doi.org/10.1007/s10909-013-1075-3 lizenzpflichtig 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 176 2014 5-6 23 01 905-910 |
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Enthalten in Journal of low temperature physics 176(2014), 5-6 vom: 23. Jan., Seite 905-910 volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 |
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Enthalten in Journal of low temperature physics 176(2014), 5-6 vom: 23. Jan., Seite 905-910 volume:176 year:2014 number:5-6 day:23 month:01 pages:905-910 |
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Dark matter CRESST Quenching factor CaWO |
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Strauss, R. @@aut@@ Ciemniak, C. @@aut@@ Deuter, G. @@aut@@ Feilitzsch, F. V. @@aut@@ Gütlein, A. @@aut@@ Hagn, H. @@aut@@ Hellgartner, D. @@aut@@ Jochum, J. @@aut@@ Lanfranchi, J.-C. @@aut@@ Münster, A. @@aut@@ Potzel, W. @@aut@@ Roth, S. @@aut@@ Rottler, K. @@aut@@ Sailer, C. @@aut@@ Scholl, S. @@aut@@ Sivers, M. V. @@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 CRESST misc Quenching factor misc CaWO Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
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1573-7357 |
| topic_title |
530 ASE 33.09 bkl 33.30 bkl 33.60 bkl Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST Dark matter (dpeaa)DE-He213 CRESST (dpeaa)DE-He213 Quenching factor (dpeaa)DE-He213 CaWO (dpeaa)DE-He213 |
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ddc 530 bkl 33.09 bkl 33.30 bkl 33.60 misc Dark matter misc CRESST misc Quenching factor misc CaWO |
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ddc 530 bkl 33.09 bkl 33.30 bkl 33.60 misc Dark matter misc CRESST misc Quenching factor misc CaWO |
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ddc 530 bkl 33.09 bkl 33.30 bkl 33.60 misc Dark matter misc CRESST misc Quenching factor misc CaWO |
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Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
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(DE-627)SPR014523485 (SPR)s10909-013-1075-3-e |
| title_full |
Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
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Strauss, R. |
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Journal of low temperature physics |
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Journal of low temperature physics |
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Strauss, R. Ciemniak, C. Deuter, G. Feilitzsch, F. V. Gütlein, A. Hagn, H. Hellgartner, D. Jochum, J. Lanfranchi, J.-C. Münster, A. Potzel, W. Roth, S. Rottler, K. Sailer, C. Scholl, S. Sivers, M. V. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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176 |
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530 ASE 33.09 bkl 33.30 bkl 33.60 bkl |
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Elektronische Aufsätze |
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Strauss, R. |
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10.1007/s10909-013-1075-3 |
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530 |
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verfasserin |
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results of quenching factor measurements of cawo%$_4%$ at mk temperatures for the direct dark matter search experiment cresst |
| title_auth |
Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
| abstract |
Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). |
| abstractGer |
Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). |
| abstract_unstemmed |
Abstract The CRESST experiment aims at a direct detection of WIMP dark matter (DM) using scintillating CaWO%$_4%$ crystals operated as phonon detectors at mK temperatures. An important feature of the experiment is the active background discrimination technique exploiting the different light outputs depending on the kind of particle interaction. The reduced light yield of nuclear recoils compared to electron recoils is quantified by quenching factors (QFs). The precise measurement of the QFs and thus the identification of the individual recoiling nucleus in the multi-target material CaWO%$_4%$ is crucial for neutron background discrimination and assuming a positive DM signal would allow to a certain extent WIMP-mass spectroscopy. At the Munich tandem accelerator a dedicated neutron scattering facility has been set up to measure the QFs of CaWO%$_4%$, in particular that of tungsten, at mK temperatures. Monoenergetic neutrons (11 MeV) produced by the accelerator are scattered off a CRESST-like detector module that is operated in a dilution refrigerator. In this setup, the recoiling nucleus (O, Ca and W) is identified by time-of-flight measurement in liquid-scintillator detectors placed at fixed scattering angles. The QF of W could be determined with unprecedented accuracy at mK temperatures and under realistic measurement conditions: %$QF_W=0.0196\pm 0.0022%$ (preliminary value). |
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| container_issue |
5-6 |
| title_short |
Results of Quenching Factor Measurements of CaWO%$_4%$ at mK Temperatures for the Direct Dark Matter Search Experiment CRESST |
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https://dx.doi.org/10.1007/s10909-013-1075-3 |
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| author2 |
Ciemniak, C. Deuter, G. Feilitzsch, F. V. Gütlein, A. Hagn, H. Hellgartner, D. Jochum, J. Lanfranchi, J.-C. Münster, A. Potzel, W. Roth, S. Rottler, K. Sailer, C. Scholl, S. Sivers, M. V. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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Ciemniak, C. Deuter, G. Feilitzsch, F. V. Gütlein, A. Hagn, H. Hellgartner, D. Jochum, J. Lanfranchi, J.-C. Münster, A. Potzel, W. Roth, S. Rottler, K. Sailer, C. Scholl, S. Sivers, M. V. Usherov, I. Wawoczny, S. Willers, M. Wüstrich, M. Zöller, A. |
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| doi_str |
10.1007/s10909-013-1075-3 |
| up_date |
2024-07-04T02:06:30.530Z |
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1803612366341931008 |
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| score |
7.398796 |