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101“... allow to reproduce the correct DM relic abundance while avoiding the bounds from direct and indirect...”
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102by Plascencia-Contreras, Alexis David“... coannihilation channels are highly relevant for a determination of the correct relic abundance. Firstly, we...”
Published 2018
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103by Luiz, Vivian Ventura Ferreira.“... is one of the open questions of cosmology and particle physics. Several observations, at di erent...”
Published 2017
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104“... and the cosmological evolution of QCD axion including the estimate of the relic abundance as a dark matter candidate....”
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105“... to induce a significant reannihilation process, reducing the dark matter relic abundance. Most...”
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106“... processes τ→μγ and Higgs decay gained at LHC. Within the same parameter spaces, the DM relic abundance...”
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107“... relic abundance and satisfying the current direct search bounds. We extend the Higgs triplet model...”
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108by Debasish Borah, Arnab Dasgupta, Ujjal Kumar Dey, Sudhanwa Patra, Gaurav Tomar“... dark matter are not large enough to generate its relic abundance within the observed limit. We include...”
Published 2017-09-01
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109“... neutralino, as the best-known supersymmetric (SUSY) WIMP, obtains the required relic abundance. Many...”
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110“... sector in the early Universe. We compute the DM relic abundance as a function of the model parameters...”
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111“..., or one of each), finding that it is possible to obtain the observed relic abundance via thermal freeze...”
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112“... mediator. In this model, the DM relic abundance is dominated by the fermionic DM particle which...”
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113“... non-universality, we find that higgsino can be the lightest SUSY particle and its thermal relic...”
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114“..., the observed SM-like Higgs boson mass of around 125 GeV and the relic abundance of the neutralino dark matter...”
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115“... of the observed relic abundance if the dark matter particles solely originate from thermal production....”
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116“... that the impact of these new effects on the thermal relic abundance is significant enough to make it worthwhile...”
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117“... relic abundance from freeze-in are excluded below a few tens of keV, depending on the value of the dark...”
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119“... force between TeV-scale particles, that can impact considerably their annihilation due to the Sommerfeld...”
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120“...) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show...”
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