Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is...
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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| 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.116.161302 |
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OLC1974562220 |
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| 520 | |a We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. | ||
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10.1103/PhysRevLett.116.161302 doi PQ20160610 (DE-627)OLC1974562220 (DE-599)GBVOLC1974562220 (PRQ)a857-24853fec0544a52fe16f83ac7c9cd1fb6daaa5506b21aadd616226d7db96f2350 (KEY)0009201020160000116001600000resultsonthespindependentscatteringofweaklyinterac DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Phenomenology Experiment High Energy Physics 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.116.161302 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 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.116.161302 doi PQ20160610 (DE-627)OLC1974562220 (DE-599)GBVOLC1974562220 (PRQ)a857-24853fec0544a52fe16f83ac7c9cd1fb6daaa5506b21aadd616226d7db96f2350 (KEY)0009201020160000116001600000resultsonthespindependentscatteringofweaklyinterac DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Phenomenology Experiment High Energy Physics 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.116.161302 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 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 |
| allfields_unstemmed |
10.1103/PhysRevLett.116.161302 doi PQ20160610 (DE-627)OLC1974562220 (DE-599)GBVOLC1974562220 (PRQ)a857-24853fec0544a52fe16f83ac7c9cd1fb6daaa5506b21aadd616226d7db96f2350 (KEY)0009201020160000116001600000resultsonthespindependentscatteringofweaklyinterac DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Phenomenology Experiment High Energy Physics 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.116.161302 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 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.116.161302 doi PQ20160610 (DE-627)OLC1974562220 (DE-599)GBVOLC1974562220 (PRQ)a857-24853fec0544a52fe16f83ac7c9cd1fb6daaa5506b21aadd616226d7db96f2350 (KEY)0009201020160000116001600000resultsonthespindependentscatteringofweaklyinterac DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Phenomenology Experiment High Energy Physics 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.116.161302 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 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.116.161302 doi PQ20160610 (DE-627)OLC1974562220 (DE-599)GBVOLC1974562220 (PRQ)a857-24853fec0544a52fe16f83ac7c9cd1fb6daaa5506b21aadd616226d7db96f2350 (KEY)0009201020160000116001600000resultsonthespindependentscatteringofweaklyinterac DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Akerib, D S verfasserin aut Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. Phenomenology Experiment High Energy Physics 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.116.161302 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 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 Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment Phenomenology Experiment High Energy Physics |
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Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment |
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Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment |
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10.1103/PhysRevLett.116.161302 |
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results on the spin-dependent scattering of weakly interacting massive particles on nucleons from the run 3 data of the lux experiment |
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Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment |
| abstract |
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. |
| abstractGer |
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. |
| abstract_unstemmed |
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date. |
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Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment |
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http://dx.doi.org/10.1103/PhysRevLett.116.161302 http://www.ncbi.nlm.nih.gov/pubmed/27152786 http://arxiv.org/abs/1602.03489 |
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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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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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