Sensitivities to neutrino electromagnetic properties at the TEXONO experiment
The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency no...
Ausführliche Beschreibung
Autor*in: |
T.S. Kosmas [verfasserIn] O.G. Miranda [verfasserIn] D.K. Papoulias [verfasserIn] M. Tórtola [verfasserIn] J.W.F. Valle [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
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2015 |
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Übergeordnetes Werk: |
In: Physics Letters B - Elsevier, 2015, 750(2015), C, Seite 459-465 |
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Übergeordnetes Werk: |
volume:750 ; year:2015 ; number:C ; pages:459-465 |
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Link aufrufen |
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DOI / URN: |
10.1016/j.physletb.2015.09.054 |
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Katalog-ID: |
DOAJ035209046 |
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10.1016/j.physletb.2015.09.054 doi (DE-627)DOAJ035209046 (DE-599)DOAJee67fbae249d4beb87883e085adb783b DE-627 ger DE-627 rakwb eng QC1-999 T.S. Kosmas verfasserin aut Sensitivities to neutrino electromagnetic properties at the TEXONO experiment 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. Reactor neutrinos Coherent elastic neutrino–nucleus scattering (CENNS) Weak mixing angle Neutrino magnetic moment Neutrino charge radius Quenching factor Physics O.G. Miranda verfasserin aut D.K. Papoulias verfasserin aut M. Tórtola verfasserin aut J.W.F. Valle verfasserin aut In Physics Letters B Elsevier, 2015 750(2015), C, Seite 459-465 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:750 year:2015 number:C pages:459-465 https://doi.org/10.1016/j.physletb.2015.09.054 kostenfrei https://doaj.org/article/ee67fbae249d4beb87883e085adb783b kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269315007297 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei https://doaj.org/toc/1873-2445 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 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 750 2015 C 459-465 |
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10.1016/j.physletb.2015.09.054 doi (DE-627)DOAJ035209046 (DE-599)DOAJee67fbae249d4beb87883e085adb783b DE-627 ger DE-627 rakwb eng QC1-999 T.S. Kosmas verfasserin aut Sensitivities to neutrino electromagnetic properties at the TEXONO experiment 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. Reactor neutrinos Coherent elastic neutrino–nucleus scattering (CENNS) Weak mixing angle Neutrino magnetic moment Neutrino charge radius Quenching factor Physics O.G. Miranda verfasserin aut D.K. Papoulias verfasserin aut M. Tórtola verfasserin aut J.W.F. Valle verfasserin aut In Physics Letters B Elsevier, 2015 750(2015), C, Seite 459-465 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:750 year:2015 number:C pages:459-465 https://doi.org/10.1016/j.physletb.2015.09.054 kostenfrei https://doaj.org/article/ee67fbae249d4beb87883e085adb783b kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269315007297 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei https://doaj.org/toc/1873-2445 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 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 750 2015 C 459-465 |
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10.1016/j.physletb.2015.09.054 doi (DE-627)DOAJ035209046 (DE-599)DOAJee67fbae249d4beb87883e085adb783b DE-627 ger DE-627 rakwb eng QC1-999 T.S. Kosmas verfasserin aut Sensitivities to neutrino electromagnetic properties at the TEXONO experiment 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. Reactor neutrinos Coherent elastic neutrino–nucleus scattering (CENNS) Weak mixing angle Neutrino magnetic moment Neutrino charge radius Quenching factor Physics O.G. Miranda verfasserin aut D.K. Papoulias verfasserin aut M. Tórtola verfasserin aut J.W.F. Valle verfasserin aut In Physics Letters B Elsevier, 2015 750(2015), C, Seite 459-465 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:750 year:2015 number:C pages:459-465 https://doi.org/10.1016/j.physletb.2015.09.054 kostenfrei https://doaj.org/article/ee67fbae249d4beb87883e085adb783b kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269315007297 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei https://doaj.org/toc/1873-2445 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 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 750 2015 C 459-465 |
allfieldsGer |
10.1016/j.physletb.2015.09.054 doi (DE-627)DOAJ035209046 (DE-599)DOAJee67fbae249d4beb87883e085adb783b DE-627 ger DE-627 rakwb eng QC1-999 T.S. Kosmas verfasserin aut Sensitivities to neutrino electromagnetic properties at the TEXONO experiment 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. Reactor neutrinos Coherent elastic neutrino–nucleus scattering (CENNS) Weak mixing angle Neutrino magnetic moment Neutrino charge radius Quenching factor Physics O.G. Miranda verfasserin aut D.K. Papoulias verfasserin aut M. Tórtola verfasserin aut J.W.F. Valle verfasserin aut In Physics Letters B Elsevier, 2015 750(2015), C, Seite 459-465 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:750 year:2015 number:C pages:459-465 https://doi.org/10.1016/j.physletb.2015.09.054 kostenfrei https://doaj.org/article/ee67fbae249d4beb87883e085adb783b kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269315007297 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei https://doaj.org/toc/1873-2445 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 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 750 2015 C 459-465 |
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10.1016/j.physletb.2015.09.054 doi (DE-627)DOAJ035209046 (DE-599)DOAJee67fbae249d4beb87883e085adb783b DE-627 ger DE-627 rakwb eng QC1-999 T.S. Kosmas verfasserin aut Sensitivities to neutrino electromagnetic properties at the TEXONO experiment 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. Reactor neutrinos Coherent elastic neutrino–nucleus scattering (CENNS) Weak mixing angle Neutrino magnetic moment Neutrino charge radius Quenching factor Physics O.G. Miranda verfasserin aut D.K. Papoulias verfasserin aut M. Tórtola verfasserin aut J.W.F. Valle verfasserin aut In Physics Letters B Elsevier, 2015 750(2015), C, Seite 459-465 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:750 year:2015 number:C pages:459-465 https://doi.org/10.1016/j.physletb.2015.09.054 kostenfrei https://doaj.org/article/ee67fbae249d4beb87883e085adb783b kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269315007297 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei https://doaj.org/toc/1873-2445 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 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 750 2015 C 459-465 |
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The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. |
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The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. |
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The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. Focusing on low threshold Germanium-based targets with kg-scale mass, we find a remarkable efficiency not only for detecting CENNS events due to the weak interaction, but also for probing novel electromagnetic neutrino interactions. Specifically, we demonstrate that such experiments are complementary in performing precision Standard Model tests as well as in shedding light on sub-leading effects due to neutrino magnetic moment and neutrino charge radius. This work employs realistic nuclear structure calculations based on the quasi-particle random phase approximation (QRPA) and takes into consideration the crucial quenching effect corrections. Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies. |
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Kosmas</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Sensitivities to neutrino electromagnetic properties at the TEXONO experiment</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The possibility of measuring neutral-current coherent elastic neutrino–nucleus scattering (CENNS) at the TEXONO experiment has opened high expectations towards probing exotic neutrino properties. 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Such a treatment, in conjunction with a simple statistical analysis, shows that the attainable sensitivities are improved by one order of magnitude as compared to previous studies.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Reactor neutrinos</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Coherent elastic neutrino–nucleus scattering (CENNS)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Weak mixing angle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Neutrino magnetic moment</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Neutrino charge radius</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Quenching factor</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Physics</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">O.G. Miranda</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D.K. Papoulias</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Tórtola</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J.W.F. Valle</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">In</subfield><subfield code="t">Physics Letters B</subfield><subfield code="d">Elsevier, 2015</subfield><subfield code="g">750(2015), C, Seite 459-465</subfield><subfield code="w">(DE-627)266015360</subfield><subfield code="w">(DE-600)1466612-1</subfield><subfield code="x">18732445</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:750</subfield><subfield code="g">year:2015</subfield><subfield code="g">number:C</subfield><subfield code="g">pages:459-465</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1016/j.physletb.2015.09.054</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doaj.org/article/ee67fbae249d4beb87883e085adb783b</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://www.sciencedirect.com/science/article/pii/S0370269315007297</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/0370-2693</subfield><subfield code="y">Journal toc</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">https://doaj.org/toc/1873-2445</subfield><subfield code="y">Journal toc</subfield><subfield code="z">kostenfrei</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_DOAJ</subfield></datafield><datafield tag="912" ind1=" 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