Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scinti...
Ausführliche Beschreibung
Gespeichert in:
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Akerib, D S [verfasserIn] |
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Artikel |
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Englisch |
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2016 |
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| Schlagwörter: |
Instrumentation and Methods for Astrophysics |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Physical review letters - Ridge, NY : American Physical Society, 1958, 116(2016), 16 |
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| Übergeordnetes Werk: |
volume:116 ; year:2016 ; number:16 |
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| DOI / URN: |
10.1103/PhysRevLett.116.161301 |
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OLC1974562034 |
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| 520 | |a We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. | ||
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10.1103/PhysRevLett.116.161301 doi PQ20160610 (DE-627)OLC1974562034 (DE-599)GBVOLC1974562034 (PRQ)a856-d367ee47417c403d4ad4b38e10660742af5437cab636f9cc9a491dbc90ac5a670 (KEY)0009201020160000116001600000improvedlimitsonscatteringofweaklyinteractingmassi DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment Araújo, H M oth Bai, X oth Bailey, A J oth Balajthy, J oth Beltrame, P oth Bernard, E P oth Bernstein, A oth Biesiadzinski, T P oth Boulton, E M oth Bradley, A oth Bramante, R oth Cahn, S B oth Carmona-Benitez, M C oth Chan, C oth Chapman, J J oth Chiller, A A oth Chiller, C oth Currie, A oth Cutter, J E oth Davison, T J R oth de Viveiros, L oth Dobi, A oth Dobson, J E Y oth Druszkiewicz, E oth Edwards, B N oth Faham, C H oth Fiorucci, S oth Gaitskell, R J oth Gehman, V M oth Ghag, C oth Gibson, K R oth Gilchriese, M G D oth Hall, C R oth Hanhardt, M oth Haselschwardt, S J oth Hertel, S A oth Hogan, D P oth Horn, M oth Huang, D Q oth Ignarra, C M oth Ihm, M oth Jacobsen, R G oth Ji, W oth Kazkaz, K oth Khaitan, D oth Knoche, R oth Larsen, N A oth Lee, C oth Lenardo, B G oth Lesko, K T oth Lindote, A oth Lopes, M I oth Malling, D C oth Manalaysay, A oth Mannino, R L oth Marzioni, M F oth McKinsey, D N oth Mei, D-M oth Mock, J oth Moongweluwan, M oth Morad, J A oth Murphy, A St J oth Nehrkorn, C oth Nelson, H N oth Neves, F oth O'Sullivan, K oth Oliver-Mallory, K C oth Ott, R A oth Palladino, K J oth Pangilinan, M oth Pease, E K oth Phelps, P oth Reichhart, L oth Rhyne, C oth Shaw, S oth Shutt, T A oth Silva, C oth Solovov, V N oth Sorensen, P oth Stephenson, S oth Sumner, T J oth Szydagis, M oth Taylor, D J oth Taylor, W oth Tennyson, B P oth Terman, P A oth Tiedt, D R oth To, W H oth Tripathi, M oth Tvrznikova, L oth Uvarov, S oth Verbus, J R oth Webb, R C oth White, J T oth Whitis, T J oth Witherell, M S oth Wolfs, F L H oth Yazdani, K oth Young, S K oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 16 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:16 http://dx.doi.org/10.1103/PhysRevLett.116.161301 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 16 |
| spelling |
10.1103/PhysRevLett.116.161301 doi PQ20160610 (DE-627)OLC1974562034 (DE-599)GBVOLC1974562034 (PRQ)a856-d367ee47417c403d4ad4b38e10660742af5437cab636f9cc9a491dbc90ac5a670 (KEY)0009201020160000116001600000improvedlimitsonscatteringofweaklyinteractingmassi DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment Araújo, H M oth Bai, X oth Bailey, A J oth Balajthy, J oth Beltrame, P oth Bernard, E P oth Bernstein, A oth Biesiadzinski, T P oth Boulton, E M oth Bradley, A oth Bramante, R oth Cahn, S B oth Carmona-Benitez, M C oth Chan, C oth Chapman, J J oth Chiller, A A oth Chiller, C oth Currie, A oth Cutter, J E oth Davison, T J R oth de Viveiros, L oth Dobi, A oth Dobson, J E Y oth Druszkiewicz, E oth Edwards, B N oth Faham, C H oth Fiorucci, S oth Gaitskell, R J oth Gehman, V M oth Ghag, C oth Gibson, K R oth Gilchriese, M G D oth Hall, C R oth Hanhardt, M oth Haselschwardt, S J oth Hertel, S A oth Hogan, D P oth Horn, M oth Huang, D Q oth Ignarra, C M oth Ihm, M oth Jacobsen, R G oth Ji, W oth Kazkaz, K oth Khaitan, D oth Knoche, R oth Larsen, N A oth Lee, C oth Lenardo, B G oth Lesko, K T oth Lindote, A oth Lopes, M I oth Malling, D C oth Manalaysay, A oth Mannino, R L oth Marzioni, M F oth McKinsey, D N oth Mei, D-M oth Mock, J oth Moongweluwan, M oth Morad, J A oth Murphy, A St J oth Nehrkorn, C oth Nelson, H N oth Neves, F oth O'Sullivan, K oth Oliver-Mallory, K C oth Ott, R A oth Palladino, K J oth Pangilinan, M oth Pease, E K oth Phelps, P oth Reichhart, L oth Rhyne, C oth Shaw, S oth Shutt, T A oth Silva, C oth Solovov, V N oth Sorensen, P oth Stephenson, S oth Sumner, T J oth Szydagis, M oth Taylor, D J oth Taylor, W oth Tennyson, B P oth Terman, P A oth Tiedt, D R oth To, W H oth Tripathi, M oth Tvrznikova, L oth Uvarov, S oth Verbus, J R oth Webb, R C oth White, J T oth Whitis, T J oth Witherell, M S oth Wolfs, F L H oth Yazdani, K oth Young, S K oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 16 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:16 http://dx.doi.org/10.1103/PhysRevLett.116.161301 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 16 |
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10.1103/PhysRevLett.116.161301 doi PQ20160610 (DE-627)OLC1974562034 (DE-599)GBVOLC1974562034 (PRQ)a856-d367ee47417c403d4ad4b38e10660742af5437cab636f9cc9a491dbc90ac5a670 (KEY)0009201020160000116001600000improvedlimitsonscatteringofweaklyinteractingmassi DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment Araújo, H M oth Bai, X oth Bailey, A J oth Balajthy, J oth Beltrame, P oth Bernard, E P oth Bernstein, A oth Biesiadzinski, T P oth Boulton, E M oth Bradley, A oth Bramante, R oth Cahn, S B oth Carmona-Benitez, M C oth Chan, C oth Chapman, J J oth Chiller, A A oth Chiller, C oth Currie, A oth Cutter, J E oth Davison, T J R oth de Viveiros, L oth Dobi, A oth Dobson, J E Y oth Druszkiewicz, E oth Edwards, B N oth Faham, C H oth Fiorucci, S oth Gaitskell, R J oth Gehman, V M oth Ghag, C oth Gibson, K R oth Gilchriese, M G D oth Hall, C R oth Hanhardt, M oth Haselschwardt, S J oth Hertel, S A oth Hogan, D P oth Horn, M oth Huang, D Q oth Ignarra, C M oth Ihm, M oth Jacobsen, R G oth Ji, W oth Kazkaz, K oth Khaitan, D oth Knoche, R oth Larsen, N A oth Lee, C oth Lenardo, B G oth Lesko, K T oth Lindote, A oth Lopes, M I oth Malling, D C oth Manalaysay, A oth Mannino, R L oth Marzioni, M F oth McKinsey, D N oth Mei, D-M oth Mock, J oth Moongweluwan, M oth Morad, J A oth Murphy, A St J oth Nehrkorn, C oth Nelson, H N oth Neves, F oth O'Sullivan, K oth Oliver-Mallory, K C oth Ott, R A oth Palladino, K J oth Pangilinan, M oth Pease, E K oth Phelps, P oth Reichhart, L oth Rhyne, C oth Shaw, S oth Shutt, T A oth Silva, C oth Solovov, V N oth Sorensen, P oth Stephenson, S oth Sumner, T J oth Szydagis, M oth Taylor, D J oth Taylor, W oth Tennyson, B P oth Terman, P A oth Tiedt, D R oth To, W H oth Tripathi, M oth Tvrznikova, L oth Uvarov, S oth Verbus, J R oth Webb, R C oth White, J T oth Whitis, T J oth Witherell, M S oth Wolfs, F L H oth Yazdani, K oth Young, S K oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 16 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:16 http://dx.doi.org/10.1103/PhysRevLett.116.161301 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 16 |
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10.1103/PhysRevLett.116.161301 doi PQ20160610 (DE-627)OLC1974562034 (DE-599)GBVOLC1974562034 (PRQ)a856-d367ee47417c403d4ad4b38e10660742af5437cab636f9cc9a491dbc90ac5a670 (KEY)0009201020160000116001600000improvedlimitsonscatteringofweaklyinteractingmassi DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment Araújo, H M oth Bai, X oth Bailey, A J oth Balajthy, J oth Beltrame, P oth Bernard, E P oth Bernstein, A oth Biesiadzinski, T P oth Boulton, E M oth Bradley, A oth Bramante, R oth Cahn, S B oth Carmona-Benitez, M C oth Chan, C oth Chapman, J J oth Chiller, A A oth Chiller, C oth Currie, A oth Cutter, J E oth Davison, T J R oth de Viveiros, L oth Dobi, A oth Dobson, J E Y oth Druszkiewicz, E oth Edwards, B N oth Faham, C H oth Fiorucci, S oth Gaitskell, R J oth Gehman, V M oth Ghag, C oth Gibson, K R oth Gilchriese, M G D oth Hall, C R oth Hanhardt, M oth Haselschwardt, S J oth Hertel, S A oth Hogan, D P oth Horn, M oth Huang, D Q oth Ignarra, C M oth Ihm, M oth Jacobsen, R G oth Ji, W oth Kazkaz, K oth Khaitan, D oth Knoche, R oth Larsen, N A oth Lee, C oth Lenardo, B G oth Lesko, K T oth Lindote, A oth Lopes, M I oth Malling, D C oth Manalaysay, A oth Mannino, R L oth Marzioni, M F oth McKinsey, D N oth Mei, D-M oth Mock, J oth Moongweluwan, M oth Morad, J A oth Murphy, A St J oth Nehrkorn, C oth Nelson, H N oth Neves, F oth O'Sullivan, K oth Oliver-Mallory, K C oth Ott, R A oth Palladino, K J oth Pangilinan, M oth Pease, E K oth Phelps, P oth Reichhart, L oth Rhyne, C oth Shaw, S oth Shutt, T A oth Silva, C oth Solovov, V N oth Sorensen, P oth Stephenson, S oth Sumner, T J oth Szydagis, M oth Taylor, D J oth Taylor, W oth Tennyson, B P oth Terman, P A oth Tiedt, D R oth To, W H oth Tripathi, M oth Tvrznikova, L oth Uvarov, S oth Verbus, J R oth Webb, R C oth White, J T oth Whitis, T J oth Witherell, M S oth Wolfs, F L H oth Yazdani, K oth Young, S K oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 16 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:16 http://dx.doi.org/10.1103/PhysRevLett.116.161301 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 16 |
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10.1103/PhysRevLett.116.161301 doi PQ20160610 (DE-627)OLC1974562034 (DE-599)GBVOLC1974562034 (PRQ)a856-d367ee47417c403d4ad4b38e10660742af5437cab636f9cc9a491dbc90ac5a670 (KEY)0009201020160000116001600000improvedlimitsonscatteringofweaklyinteractingmassi DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment Araújo, H M oth Bai, X oth Bailey, A J oth Balajthy, J oth Beltrame, P oth Bernard, E P oth Bernstein, A oth Biesiadzinski, T P oth Boulton, E M oth Bradley, A oth Bramante, R oth Cahn, S B oth Carmona-Benitez, M C oth Chan, C oth Chapman, J J oth Chiller, A A oth Chiller, C oth Currie, A oth Cutter, J E oth Davison, T J R oth de Viveiros, L oth Dobi, A oth Dobson, J E Y oth Druszkiewicz, E oth Edwards, B N oth Faham, C H oth Fiorucci, S oth Gaitskell, R J oth Gehman, V M oth Ghag, C oth Gibson, K R oth Gilchriese, M G D oth Hall, C R oth Hanhardt, M oth Haselschwardt, S J oth Hertel, S A oth Hogan, D P oth Horn, M oth Huang, D Q oth Ignarra, C M oth Ihm, M oth Jacobsen, R G oth Ji, W oth Kazkaz, K oth Khaitan, D oth Knoche, R oth Larsen, N A oth Lee, C oth Lenardo, B G oth Lesko, K T oth Lindote, A oth Lopes, M I oth Malling, D C oth Manalaysay, A oth Mannino, R L oth Marzioni, M F oth McKinsey, D N oth Mei, D-M oth Mock, J oth Moongweluwan, M oth Morad, J A oth Murphy, A St J oth Nehrkorn, C oth Nelson, H N oth Neves, F oth O'Sullivan, K oth Oliver-Mallory, K C oth Ott, R A oth Palladino, K J oth Pangilinan, M oth Pease, E K oth Phelps, P oth Reichhart, L oth Rhyne, C oth Shaw, S oth Shutt, T A oth Silva, C oth Solovov, V N oth Sorensen, P oth Stephenson, S oth Sumner, T J oth Szydagis, M oth Taylor, D J oth Taylor, W oth Tennyson, B P oth Terman, P A oth Tiedt, D R oth To, W H oth Tripathi, M oth Tvrznikova, L oth Uvarov, S oth Verbus, J R oth Webb, R C oth White, J T oth Whitis, T J oth Witherell, M S oth Wolfs, F L H oth Yazdani, K oth Young, S K oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 16 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:16 http://dx.doi.org/10.1103/PhysRevLett.116.161301 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 16 |
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Akerib, D S @@aut@@ Araújo, H M @@oth@@ Bai, X @@oth@@ Bailey, A J @@oth@@ Balajthy, J @@oth@@ Beltrame, P @@oth@@ Bernard, E P @@oth@@ Bernstein, A @@oth@@ Biesiadzinski, T P @@oth@@ Boulton, E M @@oth@@ Bradley, A @@oth@@ Bramante, R @@oth@@ Cahn, S B @@oth@@ Carmona-Benitez, M C @@oth@@ Chan, C @@oth@@ Chapman, J J @@oth@@ Chiller, A A @@oth@@ Chiller, C @@oth@@ Currie, A @@oth@@ Cutter, J E @@oth@@ Davison, T J R @@oth@@ de Viveiros, L @@oth@@ Dobi, A @@oth@@ Dobson, J E Y @@oth@@ Druszkiewicz, E @@oth@@ Edwards, B N @@oth@@ Faham, C H @@oth@@ Fiorucci, S @@oth@@ Gaitskell, R J @@oth@@ Gehman, V M @@oth@@ Ghag, C @@oth@@ Gibson, K R @@oth@@ Gilchriese, M G D @@oth@@ Hall, C R @@oth@@ Hanhardt, M @@oth@@ Haselschwardt, S J @@oth@@ Hertel, S A @@oth@@ Hogan, D P @@oth@@ Horn, M @@oth@@ Huang, D Q @@oth@@ Ignarra, C M @@oth@@ Ihm, M @@oth@@ Jacobsen, R G @@oth@@ Ji, W @@oth@@ Kazkaz, K @@oth@@ Khaitan, D @@oth@@ Knoche, R @@oth@@ Larsen, N A @@oth@@ Lee, C @@oth@@ Lenardo, B G @@oth@@ Lesko, K T @@oth@@ Lindote, A @@oth@@ Lopes, M I @@oth@@ Malling, D C @@oth@@ Manalaysay, A @@oth@@ Mannino, R L @@oth@@ Marzioni, M F @@oth@@ McKinsey, D N @@oth@@ Mei, D-M @@oth@@ Mock, J @@oth@@ Moongweluwan, M @@oth@@ Morad, J A @@oth@@ Murphy, A St J @@oth@@ Nehrkorn, C @@oth@@ Nelson, H N @@oth@@ Neves, F @@oth@@ O'Sullivan, K @@oth@@ Oliver-Mallory, K C @@oth@@ Ott, R A @@oth@@ Palladino, K J @@oth@@ Pangilinan, M @@oth@@ Pease, E K @@oth@@ Phelps, P @@oth@@ Reichhart, L @@oth@@ Rhyne, C @@oth@@ Shaw, S @@oth@@ Shutt, T A @@oth@@ Silva, C @@oth@@ Solovov, V N @@oth@@ Sorensen, P @@oth@@ Stephenson, S @@oth@@ Sumner, T J @@oth@@ Szydagis, M @@oth@@ Taylor, D J @@oth@@ Taylor, W @@oth@@ Tennyson, B P @@oth@@ Terman, P A @@oth@@ Tiedt, D R @@oth@@ To, W H @@oth@@ Tripathi, M @@oth@@ Tvrznikova, L @@oth@@ Uvarov, S @@oth@@ Verbus, J R @@oth@@ Webb, R C @@oth@@ White, J T @@oth@@ Whitis, T J @@oth@@ Witherell, M S @@oth@@ Wolfs, F L H @@oth@@ Yazdani, K @@oth@@ Young, S K @@oth@@ ... @@oth@@ |
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550 DNB UA 1000 AVZ rvk Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data Physics High Energy Physics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Cosmology and Nongalactic Astrophysics Astrophysics Experiment |
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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data |
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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data |
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10.1103/PhysRevLett.116.161301 |
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improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 lux data |
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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data |
| abstract |
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. |
| abstractGer |
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. |
| abstract_unstemmed |
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass. |
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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data |
| url |
http://dx.doi.org/10.1103/PhysRevLett.116.161301 http://www.ncbi.nlm.nih.gov/pubmed/27152785 http://arxiv.org/abs/1512.03506 |
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Araújo, H M Bai, X Bailey, A J Balajthy, J Beltrame, P Bernard, E P Bernstein, A Biesiadzinski, T P Boulton, E M Bradley, A Bramante, R Cahn, S B Carmona-Benitez, M C Chan, C Chapman, J J Chiller, A A Chiller, C Currie, A Cutter, J E Davison, T J R de Viveiros, L Dobi, A Dobson, J E Y Druszkiewicz, E Edwards, B N Faham, C H Fiorucci, S Gaitskell, R J Gehman, V M Ghag, C Gibson, K R Gilchriese, M G D Hall, C R Hanhardt, M Haselschwardt, S J Hertel, S A Hogan, D P Horn, M Huang, D Q Ignarra, C M Ihm, M Jacobsen, R G Ji, W Kazkaz, K Khaitan, D Knoche, R Larsen, N A Lee, C Lenardo, B G Lesko, K T Lindote, A Lopes, M I Malling, D C Manalaysay, A Mannino, R L Marzioni, M F McKinsey, D N Mei, D-M Mock, J Moongweluwan, M Morad, J A Murphy, A St J Nehrkorn, C Nelson, H N Neves, F O'Sullivan, K Oliver-Mallory, K C Ott, R A Palladino, K J Pangilinan, M Pease, E K Phelps, P Reichhart, L Rhyne, C Shaw, S Shutt, T A Silva, C Solovov, V N Sorensen, P Stephenson, S Sumner, T J Szydagis, M Taylor, D J Taylor, W Tennyson, B P Terman, P A Tiedt, D R To, W H Tripathi, M Tvrznikova, L Uvarov, S Verbus, J R Webb, R C White, J T Whitis, T J Witherell, M S Wolfs, F L H Yazdani, K Young, S K . |
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