Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector
Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abe, K. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2018transfer abstract |
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| Schlagwörter: |
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| Umfang: |
6 |
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| Übergeordnetes Werk: |
Enthalten in: Applying the Go/NoGo processing schema to a visual oddball task in older adults - Steiner, Genevieve Z. ELSEVIER, 2016, Amsterdam |
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| Übergeordnetes Werk: |
volume:787 ; year:2018 ; day:10 ; month:12 ; pages:153-158 ; extent:6 |
| Links: |
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| DOI / URN: |
10.1016/j.physletb.2018.10.050 |
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ELV045147140 |
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| 520 | |a Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. | ||
| 520 | |a Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. | ||
| 650 | 7 | |a Low background |2 Elsevier | |
| 650 | 7 | |a Liquid xenon |2 Elsevier | |
| 650 | 7 | |a Axion-like particle |2 Elsevier | |
| 650 | 7 | |a Hidden photon |2 Elsevier | |
| 650 | 7 | |a Dark matter |2 Elsevier | |
| 700 | 1 | |a Hiraide, K. |4 oth | |
| 700 | 1 | |a Ichimura, K. |4 oth | |
| 700 | 1 | |a Kishimoto, Y. |4 oth | |
| 700 | 1 | |a Kobayashi, K. |4 oth | |
| 700 | 1 | |a Kobayashi, M. |4 oth | |
| 700 | 1 | |a Moriyama, S. |4 oth | |
| 700 | 1 | |a Nakahata, M. |4 oth | |
| 700 | 1 | |a Ogawa, H. |4 oth | |
| 700 | 1 | |a Sato, K. |4 oth | |
| 700 | 1 | |a Sekiya, H. |4 oth | |
| 700 | 1 | |a Suzuki, T. |4 oth | |
| 700 | 1 | |a Takachio, O. |4 oth | |
| 700 | 1 | |a Takeda, A. |4 oth | |
| 700 | 1 | |a Tasaka, S. |4 oth | |
| 700 | 1 | |a Yamashita, M. |4 oth | |
| 700 | 1 | |a Yang, B.S. |4 oth | |
| 700 | 1 | |a Kim, N.Y. |4 oth | |
| 700 | 1 | |a Kim, Y.D. |4 oth | |
| 700 | 1 | |a Itow, Y. |4 oth | |
| 700 | 1 | |a Kanzawa, K. |4 oth | |
| 700 | 1 | |a Masuda, K. |4 oth | |
| 700 | 1 | |a Martens, K. |4 oth | |
| 700 | 1 | |a Suzuki, Y. |4 oth | |
| 700 | 1 | |a Xu, B.D. |4 oth | |
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| 700 | 1 | |a Oka, N. |4 oth | |
| 700 | 1 | |a Takeuchi, Y. |4 oth | |
| 700 | 1 | |a Kim, Y.H. |4 oth | |
| 700 | 1 | |a Lee, K.B. |4 oth | |
| 700 | 1 | |a Lee, M.K. |4 oth | |
| 700 | 1 | |a Fukuda, Y. |4 oth | |
| 700 | 1 | |a Miyasaka, M. |4 oth | |
| 700 | 1 | |a Nishijima, K. |4 oth | |
| 700 | 1 | |a Fushimi, K. |4 oth | |
| 700 | 1 | |a Kanzaki, G. |4 oth | |
| 700 | 1 | |a Nakamura, S. |4 oth | |
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10.1016/j.physletb.2018.10.050 doi GBV00000000000564.pica (DE-627)ELV045147140 (ELSEVIER)S0370-2693(18)30821-9 DE-627 ger DE-627 rakwb eng 610 VZ 77.50 bkl Abe, K. verfasserin aut Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector 2018transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Low background Elsevier Liquid xenon Elsevier Axion-like particle Elsevier Hidden photon Elsevier Dark matter Elsevier Hiraide, K. oth Ichimura, K. oth Kishimoto, Y. oth Kobayashi, K. oth Kobayashi, M. oth Moriyama, S. oth Nakahata, M. oth Ogawa, H. oth Sato, K. oth Sekiya, H. oth Suzuki, T. oth Takachio, O. oth Takeda, A. oth Tasaka, S. oth Yamashita, M. oth Yang, B.S. oth Kim, N.Y. oth Kim, Y.D. oth Itow, Y. oth Kanzawa, K. oth Masuda, K. oth Martens, K. oth Suzuki, Y. oth Xu, B.D. oth Miuchi, K. oth Oka, N. oth Takeuchi, Y. oth Kim, Y.H. oth Lee, K.B. oth Lee, M.K. oth Fukuda, Y. oth Miyasaka, M. oth Nishijima, K. oth Fushimi, K. oth Kanzaki, G. oth Nakamura, S. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 https://doi.org/10.1016/j.physletb.2018.10.050 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 787 2018 10 1210 153-158 6 |
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10.1016/j.physletb.2018.10.050 doi GBV00000000000564.pica (DE-627)ELV045147140 (ELSEVIER)S0370-2693(18)30821-9 DE-627 ger DE-627 rakwb eng 610 VZ 77.50 bkl Abe, K. verfasserin aut Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector 2018transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Low background Elsevier Liquid xenon Elsevier Axion-like particle Elsevier Hidden photon Elsevier Dark matter Elsevier Hiraide, K. oth Ichimura, K. oth Kishimoto, Y. oth Kobayashi, K. oth Kobayashi, M. oth Moriyama, S. oth Nakahata, M. oth Ogawa, H. oth Sato, K. oth Sekiya, H. oth Suzuki, T. oth Takachio, O. oth Takeda, A. oth Tasaka, S. oth Yamashita, M. oth Yang, B.S. oth Kim, N.Y. oth Kim, Y.D. oth Itow, Y. oth Kanzawa, K. oth Masuda, K. oth Martens, K. oth Suzuki, Y. oth Xu, B.D. oth Miuchi, K. oth Oka, N. oth Takeuchi, Y. oth Kim, Y.H. oth Lee, K.B. oth Lee, M.K. oth Fukuda, Y. oth Miyasaka, M. oth Nishijima, K. oth Fushimi, K. oth Kanzaki, G. oth Nakamura, S. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 https://doi.org/10.1016/j.physletb.2018.10.050 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 787 2018 10 1210 153-158 6 |
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10.1016/j.physletb.2018.10.050 doi GBV00000000000564.pica (DE-627)ELV045147140 (ELSEVIER)S0370-2693(18)30821-9 DE-627 ger DE-627 rakwb eng 610 VZ 77.50 bkl Abe, K. verfasserin aut Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector 2018transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Low background Elsevier Liquid xenon Elsevier Axion-like particle Elsevier Hidden photon Elsevier Dark matter Elsevier Hiraide, K. oth Ichimura, K. oth Kishimoto, Y. oth Kobayashi, K. oth Kobayashi, M. oth Moriyama, S. oth Nakahata, M. oth Ogawa, H. oth Sato, K. oth Sekiya, H. oth Suzuki, T. oth Takachio, O. oth Takeda, A. oth Tasaka, S. oth Yamashita, M. oth Yang, B.S. oth Kim, N.Y. oth Kim, Y.D. oth Itow, Y. oth Kanzawa, K. oth Masuda, K. oth Martens, K. oth Suzuki, Y. oth Xu, B.D. oth Miuchi, K. oth Oka, N. oth Takeuchi, Y. oth Kim, Y.H. oth Lee, K.B. oth Lee, M.K. oth Fukuda, Y. oth Miyasaka, M. oth Nishijima, K. oth Fushimi, K. oth Kanzaki, G. oth Nakamura, S. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 https://doi.org/10.1016/j.physletb.2018.10.050 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 787 2018 10 1210 153-158 6 |
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10.1016/j.physletb.2018.10.050 doi GBV00000000000564.pica (DE-627)ELV045147140 (ELSEVIER)S0370-2693(18)30821-9 DE-627 ger DE-627 rakwb eng 610 VZ 77.50 bkl Abe, K. verfasserin aut Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector 2018transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Low background Elsevier Liquid xenon Elsevier Axion-like particle Elsevier Hidden photon Elsevier Dark matter Elsevier Hiraide, K. oth Ichimura, K. oth Kishimoto, Y. oth Kobayashi, K. oth Kobayashi, M. oth Moriyama, S. oth Nakahata, M. oth Ogawa, H. oth Sato, K. oth Sekiya, H. oth Suzuki, T. oth Takachio, O. oth Takeda, A. oth Tasaka, S. oth Yamashita, M. oth Yang, B.S. oth Kim, N.Y. oth Kim, Y.D. oth Itow, Y. oth Kanzawa, K. oth Masuda, K. oth Martens, K. oth Suzuki, Y. oth Xu, B.D. oth Miuchi, K. oth Oka, N. oth Takeuchi, Y. oth Kim, Y.H. oth Lee, K.B. oth Lee, M.K. oth Fukuda, Y. oth Miyasaka, M. oth Nishijima, K. oth Fushimi, K. oth Kanzaki, G. oth Nakamura, S. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 https://doi.org/10.1016/j.physletb.2018.10.050 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 787 2018 10 1210 153-158 6 |
| allfieldsSound |
10.1016/j.physletb.2018.10.050 doi GBV00000000000564.pica (DE-627)ELV045147140 (ELSEVIER)S0370-2693(18)30821-9 DE-627 ger DE-627 rakwb eng 610 VZ 77.50 bkl Abe, K. verfasserin aut Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector 2018transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. Low background Elsevier Liquid xenon Elsevier Axion-like particle Elsevier Hidden photon Elsevier Dark matter Elsevier Hiraide, K. oth Ichimura, K. oth Kishimoto, Y. oth Kobayashi, K. oth Kobayashi, M. oth Moriyama, S. oth Nakahata, M. oth Ogawa, H. oth Sato, K. oth Sekiya, H. oth Suzuki, T. oth Takachio, O. oth Takeda, A. oth Tasaka, S. oth Yamashita, M. oth Yang, B.S. oth Kim, N.Y. oth Kim, Y.D. oth Itow, Y. oth Kanzawa, K. oth Masuda, K. oth Martens, K. oth Suzuki, Y. oth Xu, B.D. oth Miuchi, K. oth Oka, N. oth Takeuchi, Y. oth Kim, Y.H. oth Lee, K.B. oth Lee, M.K. oth Fukuda, Y. oth Miyasaka, M. oth Nishijima, K. oth Fushimi, K. oth Kanzaki, G. oth Nakamura, S. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 https://doi.org/10.1016/j.physletb.2018.10.050 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 787 2018 10 1210 153-158 6 |
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Enthalten in Applying the Go/NoGo processing schema to a visual oddball task in older adults Amsterdam volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 |
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Enthalten in Applying the Go/NoGo processing schema to a visual oddball task in older adults Amsterdam volume:787 year:2018 day:10 month:12 pages:153-158 extent:6 |
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Applying the Go/NoGo processing schema to a visual oddball task in older adults |
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search for dark matter in the form of hidden photons and axion-like particles in the xmass detector |
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Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector |
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Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. |
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Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. |
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Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with 327 kg of liquid xenon in the fiducial volume. No significant signal was observed, and thus we set constraints on the α ′ / α parameter related to kinetic mixing of hidden photons and the coupling constant g A e of axion-like particles in the mass range from 40 to 120 keV/ c 2 , resulting in α ′ / α < 6 × 10 − 26 and g A e < 4 × 10 − 13 . These limits are the most stringent over this mass range derived from both direct and indirect searches to date. |
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Search for dark matter in the form of hidden photons and axion-like particles in the XMASS detector |
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Hiraide, K. Ichimura, K. Kishimoto, Y. Kobayashi, K. Kobayashi, M. Moriyama, S. Nakahata, M. Ogawa, H. Sato, K. Sekiya, H. Suzuki, T. Takachio, O. Takeda, A. Tasaka, S. Yamashita, M. Yang, B.S. Kim, N.Y. Kim, Y.D. Itow, Y. Kanzawa, K. Masuda, K. Martens, K. Suzuki, Y. Xu, B.D. Miuchi, K. Oka, N. Takeuchi, Y. Kim, Y.H. Lee, K.B. Lee, M.K. Fukuda, Y. Miyasaka, M. Nishijima, K. Fushimi, K. Kanzaki, G. Nakamura, S. |
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