B-L neutralino dark matter
We focus on the supersymetric extension of the gauge group SU(3) c × SU(2)L × U(1)y × U(1)B-L in which we have included the right handed neutrino superfield gauged only under B - L. In this context, it is possible to address the problem of neutrino masses and the DM problem can be tackled via the B-...
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2014
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v485_n1_p_HernandezPinto http://hdl.handle.net/20.500.12110/paper_17426588_v485_n1_p_HernandezPinto |
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paper:paper_17426588_v485_n1_p_HernandezPinto2023-06-08T16:27:27Z B-L neutralino dark matter Physics Gauge group Neutralino dark matter Neutrino mass Right-handed neutrinos Elementary particles We focus on the supersymetric extension of the gauge group SU(3) c × SU(2)L × U(1)y × U(1)B-L in which we have included the right handed neutrino superfield gauged only under B - L. In this context, it is possible to address the problem of neutrino masses and the DM problem can be tackled via the B-L fermion sector instead of the MSSM one. © Published under licence by IOP Publishing Ltd. 2014 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v485_n1_p_HernandezPinto http://hdl.handle.net/20.500.12110/paper_17426588_v485_n1_p_HernandezPinto |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Physics Gauge group Neutralino dark matter Neutrino mass Right-handed neutrinos Elementary particles |
spellingShingle |
Physics Gauge group Neutralino dark matter Neutrino mass Right-handed neutrinos Elementary particles B-L neutralino dark matter |
topic_facet |
Physics Gauge group Neutralino dark matter Neutrino mass Right-handed neutrinos Elementary particles |
description |
We focus on the supersymetric extension of the gauge group SU(3) c × SU(2)L × U(1)y × U(1)B-L in which we have included the right handed neutrino superfield gauged only under B - L. In this context, it is possible to address the problem of neutrino masses and the DM problem can be tackled via the B-L fermion sector instead of the MSSM one. © Published under licence by IOP Publishing Ltd. |
title |
B-L neutralino dark matter |
title_short |
B-L neutralino dark matter |
title_full |
B-L neutralino dark matter |
title_fullStr |
B-L neutralino dark matter |
title_full_unstemmed |
B-L neutralino dark matter |
title_sort |
b-l neutralino dark matter |
publishDate |
2014 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17426588_v485_n1_p_HernandezPinto http://hdl.handle.net/20.500.12110/paper_17426588_v485_n1_p_HernandezPinto |
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1768546321826840576 |