Simplest neutrino mixing from S4 symmetry

Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this pre...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Krishnan, R. [verfasserIn] Harrison, P. F. Scott, W. G.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2013

Schlagwörter:	Neutrino Physics Beyond Standard Model Standard Model

Anmerkung:	© SISSA, Trieste, Italy 2013

Übergeordnetes Werk:	Enthalten in: Journal of high energy physics - Berlin : Springer, 1997, 2013(2013), 4 vom: 15. Apr.
Übergeordnetes Werk:	volume:2013 ; year:2013 ; number:4 ; day:15 ; month:04

Links:	Volltext

DOI / URN:	10.1007/JHEP04(2013)087

Katalog-ID:	SPR030440386

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allfields	10.1007/JHEP04(2013)087 doi (DE-627)SPR030440386 (SPR)JHEP04(2013)087-e DE-627 ger DE-627 rakwb eng Krishnan, R. verfasserin aut Simplest neutrino mixing from S4 symmetry 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2013 Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. Neutrino Physics (dpeaa)DE-He213 Beyond Standard Model (dpeaa)DE-He213 Standard Model (dpeaa)DE-He213 Harrison, P. F. aut Scott, W. G. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2013(2013), 4 vom: 15. Apr. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2013 year:2013 number:4 day:15 month:04 https://dx.doi.org/10.1007/JHEP04(2013)087 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2013 2013 4 15 04
spelling	10.1007/JHEP04(2013)087 doi (DE-627)SPR030440386 (SPR)JHEP04(2013)087-e DE-627 ger DE-627 rakwb eng Krishnan, R. verfasserin aut Simplest neutrino mixing from S4 symmetry 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2013 Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. Neutrino Physics (dpeaa)DE-He213 Beyond Standard Model (dpeaa)DE-He213 Standard Model (dpeaa)DE-He213 Harrison, P. F. aut Scott, W. G. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2013(2013), 4 vom: 15. Apr. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2013 year:2013 number:4 day:15 month:04 https://dx.doi.org/10.1007/JHEP04(2013)087 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2013 2013 4 15 04
allfields_unstemmed	10.1007/JHEP04(2013)087 doi (DE-627)SPR030440386 (SPR)JHEP04(2013)087-e DE-627 ger DE-627 rakwb eng Krishnan, R. verfasserin aut Simplest neutrino mixing from S4 symmetry 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2013 Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. Neutrino Physics (dpeaa)DE-He213 Beyond Standard Model (dpeaa)DE-He213 Standard Model (dpeaa)DE-He213 Harrison, P. F. aut Scott, W. G. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2013(2013), 4 vom: 15. Apr. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2013 year:2013 number:4 day:15 month:04 https://dx.doi.org/10.1007/JHEP04(2013)087 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2013 2013 4 15 04
allfieldsGer	10.1007/JHEP04(2013)087 doi (DE-627)SPR030440386 (SPR)JHEP04(2013)087-e DE-627 ger DE-627 rakwb eng Krishnan, R. verfasserin aut Simplest neutrino mixing from S4 symmetry 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2013 Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. Neutrino Physics (dpeaa)DE-He213 Beyond Standard Model (dpeaa)DE-He213 Standard Model (dpeaa)DE-He213 Harrison, P. F. aut Scott, W. G. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2013(2013), 4 vom: 15. Apr. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2013 year:2013 number:4 day:15 month:04 https://dx.doi.org/10.1007/JHEP04(2013)087 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2013 2013 4 15 04
allfieldsSound	10.1007/JHEP04(2013)087 doi (DE-627)SPR030440386 (SPR)JHEP04(2013)087-e DE-627 ger DE-627 rakwb eng Krishnan, R. verfasserin aut Simplest neutrino mixing from S4 symmetry 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2013 Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. Neutrino Physics (dpeaa)DE-He213 Beyond Standard Model (dpeaa)DE-He213 Standard Model (dpeaa)DE-He213 Harrison, P. F. aut Scott, W. G. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2013(2013), 4 vom: 15. Apr. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2013 year:2013 number:4 day:15 month:04 https://dx.doi.org/10.1007/JHEP04(2013)087 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2013 2013 4 15 04
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title	Simplest neutrino mixing from S4 symmetry
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title_sort	simplest neutrino mixing from s4 symmetry
title_auth	Simplest neutrino mixing from S4 symmetry
abstract	Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. © SISSA, Trieste, Italy 2013
abstractGer	Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. © SISSA, Trieste, Italy 2013
abstract_unstemmed	Abstract In 2004, two us proposed a texture, the “Simplest” neutrino mass matrix, which predicted $ \sin {\theta_{13 }}=\sqrt{{{{{2\varDelta m_{{^{sol}}}^2}} \left/ {{3\varDelta m_{{^{atm}}}^2}} \right.}}} $ and δCP = 90°. Using today’s measured values for neutrino mass-squared differences, this prediction gives $ {\sin^2}2{\theta_{13 }}\simeq 0.086_{-0.006}^{+0.003 } $, compared with a measured value, found by averaging the results of the Daya Bay and RENO experiments, of $ sin^{2} $2θ13 = 0.093 ± 0.010. Here we present a specific model based on S4 symmetry leading to this successful texture in the context of the type-1 see-saw mechanism, assuming Majorana neutrinos. In this case, slightly different predictions are obtained relating θ13 to the light neutrino masses, which are in accord with current experimental limits and testable at future experiments. Large CP asymmetries remain a generic prediction of the texture. © SISSA, Trieste, Italy 2013
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title_short	Simplest neutrino mixing from S4 symmetry
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Simplest neutrino mixing from S4 symmetry

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