DAMA annual modulation effect and asymmetric mirror matter

Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being ma...
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Gespeichert in:

Autor*in:	Addazi, A. [verfasserIn] Berezhiani, Z. [verfasserIn] Bernabei, R. [verfasserIn] Belli, P. [verfasserIn] Cappella, F. [verfasserIn] Cerulli, R. [verfasserIn] Incicchitti, A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	Dark Matter Vacuum Expectation Value Dark Matter Particle Galactic Halo Mirror Matter

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 75(2015), 8 vom: 29. Aug.
Übergeordnetes Werk:	volume:75 ; year:2015 ; number:8 ; day:29 ; month:08

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-015-3634-z

Katalog-ID:	SPR008346585

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allfields	10.1140/epjc/s10052-015-3634-z doi (DE-627)SPR008346585 (SPR)s10052-015-3634-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Addazi, A. verfasserin aut DAMA annual modulation effect and asymmetric mirror matter 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models. Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213 Berezhiani, Z. verfasserin aut Bernabei, R. verfasserin aut Belli, P. verfasserin aut Cappella, F. verfasserin aut Cerulli, R. verfasserin aut Incicchitti, A. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 29. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:29 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3634-z kostenfrei 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 8 29 08
spelling	10.1140/epjc/s10052-015-3634-z doi (DE-627)SPR008346585 (SPR)s10052-015-3634-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Addazi, A. verfasserin aut DAMA annual modulation effect and asymmetric mirror matter 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models. Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213 Berezhiani, Z. verfasserin aut Bernabei, R. verfasserin aut Belli, P. verfasserin aut Cappella, F. verfasserin aut Cerulli, R. verfasserin aut Incicchitti, A. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 29. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:29 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3634-z kostenfrei 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 8 29 08
allfields_unstemmed	10.1140/epjc/s10052-015-3634-z doi (DE-627)SPR008346585 (SPR)s10052-015-3634-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Addazi, A. verfasserin aut DAMA annual modulation effect and asymmetric mirror matter 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models. Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213 Berezhiani, Z. verfasserin aut Bernabei, R. verfasserin aut Belli, P. verfasserin aut Cappella, F. verfasserin aut Cerulli, R. verfasserin aut Incicchitti, A. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 29. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:29 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3634-z kostenfrei 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 8 29 08
allfieldsGer	10.1140/epjc/s10052-015-3634-z doi (DE-627)SPR008346585 (SPR)s10052-015-3634-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Addazi, A. verfasserin aut DAMA annual modulation effect and asymmetric mirror matter 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models. Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213 Berezhiani, Z. verfasserin aut Bernabei, R. verfasserin aut Belli, P. verfasserin aut Cappella, F. verfasserin aut Cerulli, R. verfasserin aut Incicchitti, A. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 29. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:29 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3634-z kostenfrei 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 8 29 08
allfieldsSound	10.1140/epjc/s10052-015-3634-z doi (DE-627)SPR008346585 (SPR)s10052-015-3634-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Addazi, A. verfasserin aut DAMA annual modulation effect and asymmetric mirror matter 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models. Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213 Berezhiani, Z. verfasserin aut Bernabei, R. verfasserin aut Belli, P. verfasserin aut Cappella, F. verfasserin aut Cerulli, R. verfasserin aut Incicchitti, A. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 29. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:29 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3634-z kostenfrei 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_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 8 29 08
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source	Enthalten in The European physical journal 75(2015), 8 vom: 29. Aug. volume:75 year:2015 number:8 day:29 month:08
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author	Addazi, A.
spellingShingle	Addazi, A. ddc 530 bkl 33.50 misc Dark Matter misc Vacuum Expectation Value misc Dark Matter Particle misc Galactic Halo misc Mirror Matter DAMA annual modulation effect and asymmetric mirror matter
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topic_title	530 ASE 33.50 bkl DAMA annual modulation effect and asymmetric mirror matter Dark Matter (dpeaa)DE-He213 Vacuum Expectation Value (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Galactic Halo (dpeaa)DE-He213 Mirror Matter (dpeaa)DE-He213
topic	ddc 530 bkl 33.50 misc Dark Matter misc Vacuum Expectation Value misc Dark Matter Particle misc Galactic Halo misc Mirror Matter
topic_unstemmed	ddc 530 bkl 33.50 misc Dark Matter misc Vacuum Expectation Value misc Dark Matter Particle misc Galactic Halo misc Mirror Matter
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title	DAMA annual modulation effect and asymmetric mirror matter
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title_full	DAMA annual modulation effect and asymmetric mirror matter
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author_browse	Addazi, A. Berezhiani, Z. Bernabei, R. Belli, P. Cappella, F. Cerulli, R. Incicchitti, A.
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title_sort	dama annual modulation effect and asymmetric mirror matter
title_auth	DAMA annual modulation effect and asymmetric mirror matter
abstract	Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models.
abstractGer	Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models.
abstract_unstemmed	Abstract The long-standing model-independent annual modulation effect measured by DAMA Collaboration is examined in the context of asymmetric mirror dark matter, assuming that dark atoms interact with target nuclei in the detector via kinetic mixing between mirror and ordinary photons, both being massless. The relevant ranges for the kinetic mixing parameter are obtained taking into account various existing uncertainties in nuclear and particle physics quantities as well as characteristic density and velocity distributions of dark matter in different halo models.
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title_short	DAMA annual modulation effect and asymmetric mirror matter
url	https://dx.doi.org/10.1140/epjc/s10052-015-3634-z
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author2	Berezhiani, Z. Bernabei, R. Belli, P. Cappella, F. Cerulli, R. Incicchitti, A.
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doi_str	10.1140/epjc/s10052-015-3634-z
up_date	2024-07-03T19:30:33.789Z
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DAMA annual modulation effect and asymmetric mirror matter

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