Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field

Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet...
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Autor*in:	Akhmedov, Evgeny [verfasserIn] Martínez-Miravé, Pablo

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Schlagwörter:	Neutrino Interactions Neutrino Mixing Non-Standard Neutrino Properties

Anmerkung:	© The Author(s) 2022

Übergeordnetes Werk:	Enthalten in: Journal of high energy physics - Berlin : Springer, 1997, 2022(2022), 10 vom: 20. Okt.
Übergeordnetes Werk:	volume:2022 ; year:2022 ; number:10 ; day:20 ; month:10

Links:	Volltext

DOI / URN:	10.1007/JHEP10(2022)144

Katalog-ID:	SPR049124935

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520			\|a Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters.
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allfields	10.1007/JHEP10(2022)144 doi (DE-627)SPR049124935 (SPR)JHEP10(2022)144-e DE-627 ger DE-627 rakwb eng Akhmedov, Evgeny verfasserin aut Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213 Martínez-Miravé, Pablo (orcid)0000-0001-8649-0546 aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 10 vom: 20. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:10 day:20 month:10 https://dx.doi.org/10.1007/JHEP10(2022)144 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 2022 2022 10 20 10
spelling	10.1007/JHEP10(2022)144 doi (DE-627)SPR049124935 (SPR)JHEP10(2022)144-e DE-627 ger DE-627 rakwb eng Akhmedov, Evgeny verfasserin aut Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213 Martínez-Miravé, Pablo (orcid)0000-0001-8649-0546 aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 10 vom: 20. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:10 day:20 month:10 https://dx.doi.org/10.1007/JHEP10(2022)144 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 2022 2022 10 20 10
allfields_unstemmed	10.1007/JHEP10(2022)144 doi (DE-627)SPR049124935 (SPR)JHEP10(2022)144-e DE-627 ger DE-627 rakwb eng Akhmedov, Evgeny verfasserin aut Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213 Martínez-Miravé, Pablo (orcid)0000-0001-8649-0546 aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 10 vom: 20. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:10 day:20 month:10 https://dx.doi.org/10.1007/JHEP10(2022)144 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 2022 2022 10 20 10
allfieldsGer	10.1007/JHEP10(2022)144 doi (DE-627)SPR049124935 (SPR)JHEP10(2022)144-e DE-627 ger DE-627 rakwb eng Akhmedov, Evgeny verfasserin aut Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213 Martínez-Miravé, Pablo (orcid)0000-0001-8649-0546 aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 10 vom: 20. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:10 day:20 month:10 https://dx.doi.org/10.1007/JHEP10(2022)144 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 2022 2022 10 20 10
allfieldsSound	10.1007/JHEP10(2022)144 doi (DE-627)SPR049124935 (SPR)JHEP10(2022)144-e DE-627 ger DE-627 rakwb eng Akhmedov, Evgeny verfasserin aut Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213 Martínez-Miravé, Pablo (orcid)0000-0001-8649-0546 aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2022(2022), 10 vom: 20. Okt. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2022 year:2022 number:10 day:20 month:10 https://dx.doi.org/10.1007/JHEP10(2022)144 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 2022 2022 10 20 10
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author	Akhmedov, Evgeny
spellingShingle	Akhmedov, Evgeny misc Neutrino Interactions misc Neutrino Mixing misc Non-Standard Neutrino Properties Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
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topic_title	Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field Neutrino Interactions (dpeaa)DE-He213 Neutrino Mixing (dpeaa)DE-He213 Non-Standard Neutrino Properties (dpeaa)DE-He213
topic	misc Neutrino Interactions misc Neutrino Mixing misc Non-Standard Neutrino Properties
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title	Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
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title_full	Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
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title_sort	solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
title_auth	Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
abstract	Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. © The Author(s) 2022
abstractGer	Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. © The Author(s) 2022
abstract_unstemmed	Abstract The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrinos, the combined action of SFP of solar neutrinos and flavour oscillations would manifest itself as a small, yet potentially detectable, flux of electron antineutrinos coming from the Sun. Non-observation of such a flux constrains the product of the neutrino magnetic moment μ and the strength of the solar magnetic field B. We derive a simple analytical expression for the expected %$ {\overline{\nu}}_e %$ appearance probability in the three-flavour framework and we use it to revisit the existing experimental bounds on μB. A full numerical calculation has also been performed to check the validity of the analytical result. We also present our numerical results in energy-binned form, convenient for analyses of the data of the current and future experiments searching for the solar %$ {\overline{\nu}}_e %$ flux. In addition, we give a comprehensive compilation of other existing limits on neutrino magnetic moments and of the expressions for the probed effective magnetic moments in terms of the fundamental neutrino magnetic moments and leptonic mixing parameters. © The Author(s) 2022
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title_short	Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field
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Solar %$ {\overline{\nu}}_e %$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field

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Zugang & Verfügbarkeit

Vorhandene Bände

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