A two-component scalar dark matter scenario comprising an additional scalar doublet and a Y = 0 scalar triplet is proposed. Key features of the ensuing dark matter phenomenology are highlighted with emphasis on interconversion between the two dark matter components. For suitable choices of the model parameters, we show that such interconversion can explain the observed relic abundance when the doublet dark matter component has mass in the desert region while the triplet component has sub-TeV mass. This finding is important in the context of such mass regions known to predict underabundant relic density for the standalone cases of the scalar doublet and triplet. In addition, we also show that the present scenario can stabilize the electroweak vacuum up to the Planck scale in the parameter space responsible for the requisite dark matter observables.
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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.
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.
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