Effective Majorana mass and neutrinoless double beta decay

Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Benato, Giovanni [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	Effective Mass Neutrino Mass Light Neutrino Normal Hierarchy Inverted Hierarchy

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 75(2015), 11 vom: 28. Nov.
Übergeordnetes Werk:	volume:75 ; year:2015 ; number:11 ; day:28 ; month:11

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-015-3802-1

Katalog-ID:	SPR008341974

Internformat


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520			\|a Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass.
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allfields	10.1140/epjc/s10052-015-3802-1 doi (DE-627)SPR008341974 (SPR)s10052-015-3802-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Benato, Giovanni verfasserin aut Effective Majorana mass and neutrinoless double beta decay 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass. Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 11 vom: 28. Nov. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:11 day:28 month:11 https://dx.doi.org/10.1140/epjc/s10052-015-3802-1 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 11 28 11
spelling	10.1140/epjc/s10052-015-3802-1 doi (DE-627)SPR008341974 (SPR)s10052-015-3802-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Benato, Giovanni verfasserin aut Effective Majorana mass and neutrinoless double beta decay 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass. Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 11 vom: 28. Nov. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:11 day:28 month:11 https://dx.doi.org/10.1140/epjc/s10052-015-3802-1 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 11 28 11
allfields_unstemmed	10.1140/epjc/s10052-015-3802-1 doi (DE-627)SPR008341974 (SPR)s10052-015-3802-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Benato, Giovanni verfasserin aut Effective Majorana mass and neutrinoless double beta decay 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass. Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 11 vom: 28. Nov. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:11 day:28 month:11 https://dx.doi.org/10.1140/epjc/s10052-015-3802-1 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 11 28 11
allfieldsGer	10.1140/epjc/s10052-015-3802-1 doi (DE-627)SPR008341974 (SPR)s10052-015-3802-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Benato, Giovanni verfasserin aut Effective Majorana mass and neutrinoless double beta decay 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass. Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 11 vom: 28. Nov. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:11 day:28 month:11 https://dx.doi.org/10.1140/epjc/s10052-015-3802-1 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 11 28 11
allfieldsSound	10.1140/epjc/s10052-015-3802-1 doi (DE-627)SPR008341974 (SPR)s10052-015-3802-1-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Benato, Giovanni verfasserin aut Effective Majorana mass and neutrinoless double beta decay 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass. Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213 Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 11 vom: 28. Nov. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:11 day:28 month:11 https://dx.doi.org/10.1140/epjc/s10052-015-3802-1 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 11 28 11
language	English
source	Enthalten in The European physical journal 75(2015), 11 vom: 28. Nov. volume:75 year:2015 number:11 day:28 month:11
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author	Benato, Giovanni
spellingShingle	Benato, Giovanni ddc 530 bkl 33.50 misc Effective Mass misc Neutrino Mass misc Light Neutrino misc Normal Hierarchy misc Inverted Hierarchy Effective Majorana mass and neutrinoless double beta decay
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topic_title	530 ASE 33.50 bkl Effective Majorana mass and neutrinoless double beta decay Effective Mass (dpeaa)DE-He213 Neutrino Mass (dpeaa)DE-He213 Light Neutrino (dpeaa)DE-He213 Normal Hierarchy (dpeaa)DE-He213 Inverted Hierarchy (dpeaa)DE-He213
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title	Effective Majorana mass and neutrinoless double beta decay
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title_full	Effective Majorana mass and neutrinoless double beta decay
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title_sort	effective majorana mass and neutrinoless double beta decay
title_auth	Effective Majorana mass and neutrinoless double beta decay
abstract	Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass.
abstractGer	Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass.
abstract_unstemmed	Abstract The probability distribution for the effective Majorana mass as a function of the lightest neutrino mass in the standard three neutrino scheme is computed via a random sampling from the distributions of the involved mixing angles and squared mass differences. A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. Finally, the prospects for %$0\nu \beta \beta %$ decay search with %$^{76}%$Ge, %$^{130}%$Te and %$^{136}%$Xe are discussed, as well as those for the measurement of the electron neutrino mass.
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title_short	Effective Majorana mass and neutrinoless double beta decay
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up_date	2024-07-03T19:20:01.274Z
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A flat distribution in the %$[0,2\pi ]%$ range for the Majorana phases is assumed, and the dependence of small values of the effective mass on the Majorana phases is highlighted. The study is then extended with the addition of the cosmological bound on the sum of the neutrino masses. 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Effective Majorana mass and neutrinoless double beta decay

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