Two dark matter candidates in a doublet-triplet Higgs model
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作者:
Melara-Duron, S.
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Univ Nacl Autonoma Mexico, Inst Fis, AP 20-364, Mexico City 01000, Mexico
Univ Nacl Autonoma Honduras, Fac Ciencias Espaciales, Dept Astron & Astrofis, Blvd Suyapa, Tegucigalpa, HondurasUniv Nacl Autonoma Mexico, Inst Fis, AP 20-364, Mexico City 01000, Mexico
Melara-Duron, S.
[1
,2
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Gaitan, R.
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Univ Nacl Autonoma Mexico, Fac Estudios Super Cuautitlan, Dept Fis, Teoloyucan 54770, Estado De Mexic, MexicoUniv Nacl Autonoma Mexico, Inst Fis, AP 20-364, Mexico City 01000, Mexico
Gaitan, R.
[3
]
Lamprea, J. M.
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Univ Nacl Autonoma Mexico, Fac Estudios Super Cuautitlan, Dept Fis, Teoloyucan 54770, Estado De Mexic, Mexico
Ctr Invest & Estudios Avanzados IPN, Dept Fis, Apdo Postal 14-740, Mexico City 07000, MexicoUniv Nacl Autonoma Mexico, Inst Fis, AP 20-364, Mexico City 01000, Mexico
Lamprea, J. M.
[3
,4
]
机构:
[1] Univ Nacl Autonoma Mexico, Inst Fis, AP 20-364, Mexico City 01000, Mexico
[2] Univ Nacl Autonoma Honduras, Fac Ciencias Espaciales, Dept Astron & Astrofis, Blvd Suyapa, Tegucigalpa, Honduras
[3] Univ Nacl Autonoma Mexico, Fac Estudios Super Cuautitlan, Dept Fis, Teoloyucan 54770, Estado De Mexic, Mexico
[4] Ctr Invest & Estudios Avanzados IPN, Dept Fis, Apdo Postal 14-740, Mexico City 07000, Mexico
We study a Standard Model extension that provides a bi-component dark matter scenario as well as a mechanism for the generation of left-handed neutrino masses. We extend the Standard Model scalar sector by adding an inert SU(2)L\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$SU(2)_L$$\end{document} complex doublet with hypercharge Y=1/2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$Y= 1/2$$\end{document} and a real inert SU(2)L\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$SU(2)_L$$\end{document} triplet with hypercharge Y=0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$Y=0$$\end{document}. These scalars provide suitable dark matter candidates belonging to two different dark sectors that are stabilised by the discrete symmetries Z2xZ2 '\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$Z_2 \times Z_2'$$\end{document}. We consider the contribution of both candidates to the total relic abundance in order to reduce the desert regions in the inert doublet and inert triplet models. In addition, we have added an active real scalar SU(2)L\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$SU(2)_L$$\end{document} triplet with hypercharge Y=1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$Y=1$$\end{document} in order to generate light neutrino Majorana masses through the type-II seesaw mechanism. We have analysed the dark matter phenomenology for the model and alongside with the neutrino mass generation.
机构:
Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
Ctr Theory, Jefferson Lab, Newport News, VA 23606 USAColl William & Mary, Dept Phys, Williamsburg, VA 23187 USA
Lee, Hye-Sung
Sher, Marc
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Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USAColl William & Mary, Dept Phys, Williamsburg, VA 23187 USA
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School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, SeoulSchool of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, Seoul
Baek S.
Nomura T.
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School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, SeoulSchool of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, Seoul
机构:
CERN, Div Theory, CH-1211 Geneva 23, SwitzerlandCERN, Div Theory, CH-1211 Geneva 23, Switzerland
Gong, Jinn-Ouk
Lee, Hyun Min
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CERN, Div Theory, CH-1211 Geneva 23, SwitzerlandCERN, Div Theory, CH-1211 Geneva 23, Switzerland
Lee, Hyun Min
Kang, Sin Kyu
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Seoul Natl Univ Sci & Technol, Inst Convergence Fundamental Studies, Seoul 139931, South Korea
Seoul Natl Univ Sci & Technol, Sch Liberal Arts, Seoul 139931, South KoreaCERN, Div Theory, CH-1211 Geneva 23, Switzerland
机构:
Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USAUniv Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
Babu, K. S.
Chakdar, Shreyashi
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机构:
Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USAUniv Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
Chakdar, Shreyashi
Mohapatra, Rabindra N.
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Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
Univ Maryland, Dept Phys, College Pk, MD 20742 USAUniv Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA