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Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova

We discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as suggested by recent two-dimensional simulations. Analyzing s...

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Detalles Bibliográficos
Autores principales: Ellis, John, Janka, Hans-Thomas, Mavromatos, Nikolaos E., Sakharov, Alexander S., Sarkisyan, Edward K.G.
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.85.105028
http://cds.cern.ch/record/1421183
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author Ellis, John
Janka, Hans-Thomas
Mavromatos, Nikolaos E.
Sakharov, Alexander S.
Sarkisyan, Edward K.G.
author_facet Ellis, John
Janka, Hans-Thomas
Mavromatos, Nikolaos E.
Sakharov, Alexander S.
Sarkisyan, Edward K.G.
author_sort Ellis, John
collection CERN
description We discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as suggested by recent two-dimensional simulations. Analyzing simulations of such neutrino emissions using the wavelet technique adopted in [1], we find that an upper limit m_nu ~ 0.14 eV could be established at the 95% confidence level if the time variations in emissions were to be preserved during neutrino propagation to the Earth.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
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spelling cern-14211832023-03-14T16:38:20Zdoi:10.1103/PhysRevD.85.105028http://cds.cern.ch/record/1421183engEllis, JohnJanka, Hans-ThomasMavromatos, Nikolaos E.Sakharov, Alexander S.Sarkisyan, Edward K.G.Prospective Constraints on Neutrino Masses from a Core-Collapse SupernovaParticle Physics - PhenomenologyWe discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as suggested by recent two-dimensional simulations. Analyzing simulations of such neutrino emissions using the wavelet technique adopted in [1], we find that an upper limit m_nu ~ 0.14 eV could be established at the 95% confidence level if the time variations in emissions were to be preserved during neutrino propagation to the Earth.We discuss the prospects for improved upper limits on neutrino masses that may be provided by a core-collapse supernova explosion in our galaxy, if it exhibits time variations in the neutrino emissions on the scale of a few milliseconds as suggested by recent two-dimensional simulations. Analyzing simulations of such neutrino emissions using the wavelet technique adopted in [1], we find that an upper limit m_nu ~ 0.14 eV could be established at the 95% confidence level if the time variations in emissions were to be preserved during neutrino propagation to the Earth.arXiv:1202.0248KCL-PH-TH-2012-05LCTS-2012-02CERN-PH-TH-2012-010KCL-PH-TH-2012-05LCTS-2012-02CERN-PH-TH-2012-010oai:cds.cern.ch:14211832012-02-02
spellingShingle Particle Physics - Phenomenology
Ellis, John
Janka, Hans-Thomas
Mavromatos, Nikolaos E.
Sakharov, Alexander S.
Sarkisyan, Edward K.G.
Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title_full Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title_fullStr Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title_full_unstemmed Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title_short Prospective Constraints on Neutrino Masses from a Core-Collapse Supernova
title_sort prospective constraints on neutrino masses from a core-collapse supernova
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.85.105028
http://cds.cern.ch/record/1421183
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