Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ

Abstract We propose a minimal extension of the standard model by including a U(1) flavor symmetry to establish a correlation between the relic abundance of dark matter, measured by WMAP and PLANCK satellite experiments and non-zero value of sin θ 13 observed at DOUBLE CHOOZ, Daya Bay, RENO and T2K....

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Main Authors: Subhaditya Bhattacharya, Biswajit Karmakar, Narendra Sahu, Arunansu Sil
Format: Article
Language:English
Published: SpringerOpen 2017-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2017)068
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spelling doaj-36890ae930764270bfacdb188720312b2020-11-24T23:02:01ZengSpringerOpenJournal of High Energy Physics1029-84792017-05-012017513510.1007/JHEP05(2017)068Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δSubhaditya Bhattacharya0Biswajit Karmakar1Narendra Sahu2Arunansu Sil3Department of Physics, Indian Institute of Technology GuwahatiDepartment of Physics, Indian Institute of Technology GuwahatiDepartment of Physics, Indian Institute of TechnologyDepartment of Physics, Indian Institute of Technology GuwahatiAbstract We propose a minimal extension of the standard model by including a U(1) flavor symmetry to establish a correlation between the relic abundance of dark matter, measured by WMAP and PLANCK satellite experiments and non-zero value of sin θ 13 observed at DOUBLE CHOOZ, Daya Bay, RENO and T2K. The flavour symmetry is allowed to be broken at a high scale to a remnant Z 2 $$ {\mathcal{Z}}_2 $$ symmetry, which not only ensures the stability to the dark matter, but also gives rise to a modification to the existing A 4-based tri-bimaximal neutrino mixing. This deviation in turn suggests the required non-zero value of sin θ 13. We assume the dark matter to be neutral under the existing A 4 symmetry while charged under the U(1) flavor symmetry. Hence in this set-up, the non-zero value of sin θ 13 predicts the dark matter charge under U(1), which can be tested at various ongoing and future direct and collider dark matter search experiments. We also point out the involvement of nonzero leptonic CP phase δ, which plays an important role in the analysis.http://link.springer.com/article/10.1007/JHEP05(2017)068Beyond Standard ModelNeutrino PhysicsDiscrete Symmetries
collection DOAJ
language English
format Article
sources DOAJ
author Subhaditya Bhattacharya
Biswajit Karmakar
Narendra Sahu
Arunansu Sil
spellingShingle Subhaditya Bhattacharya
Biswajit Karmakar
Narendra Sahu
Arunansu Sil
Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
Journal of High Energy Physics
Beyond Standard Model
Neutrino Physics
Discrete Symmetries
author_facet Subhaditya Bhattacharya
Biswajit Karmakar
Narendra Sahu
Arunansu Sil
author_sort Subhaditya Bhattacharya
title Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
title_short Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
title_full Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
title_fullStr Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
title_full_unstemmed Flavor origin of dark matter and its relation with leptonic nonzero θ 13 and Dirac CP phase δ
title_sort flavor origin of dark matter and its relation with leptonic nonzero θ 13 and dirac cp phase δ
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2017-05-01
description Abstract We propose a minimal extension of the standard model by including a U(1) flavor symmetry to establish a correlation between the relic abundance of dark matter, measured by WMAP and PLANCK satellite experiments and non-zero value of sin θ 13 observed at DOUBLE CHOOZ, Daya Bay, RENO and T2K. The flavour symmetry is allowed to be broken at a high scale to a remnant Z 2 $$ {\mathcal{Z}}_2 $$ symmetry, which not only ensures the stability to the dark matter, but also gives rise to a modification to the existing A 4-based tri-bimaximal neutrino mixing. This deviation in turn suggests the required non-zero value of sin θ 13. We assume the dark matter to be neutral under the existing A 4 symmetry while charged under the U(1) flavor symmetry. Hence in this set-up, the non-zero value of sin θ 13 predicts the dark matter charge under U(1), which can be tested at various ongoing and future direct and collider dark matter search experiments. We also point out the involvement of nonzero leptonic CP phase δ, which plays an important role in the analysis.
topic Beyond Standard Model
Neutrino Physics
Discrete Symmetries
url http://link.springer.com/article/10.1007/JHEP05(2017)068
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AT biswajitkarmakar flavororiginofdarkmatteranditsrelationwithleptonicnonzeroth13anddiraccpphased
AT narendrasahu flavororiginofdarkmatteranditsrelationwithleptonicnonzeroth13anddiraccpphased
AT arunansusil flavororiginofdarkmatteranditsrelationwithleptonicnonzeroth13anddiraccpphased
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