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141“... roles in determining the relic abundance and also responsible for the monochromatic neutrino lines...”
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142“... Interacting Massive Particles (FIMP) interacting just gravitationally with the standard model particles...”
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143“... parameters satisfying the recent measurement of relic abundance. With the obtained parameter sets, we predict...”
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144by Michael Duerr, Alexander Grohsjean, Felix Kahlhoefer, Bjoern Penning, Kai Schmidt-Hoberg, Christian Schwanenberger“... and the possibility to relax constraints from the dark matter relic abundance by opening up a new annihilation channel...”
Published 2017-04-01
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145“... clusters tended to be parallel epitaxially coalesced into unity leaving abundant relic of the subgrains...”
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146“... in which the observed DM relic abundance can be reproduced with scalar DM mass in the MeV range, with a...”
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147by Greene, Brian Randolph“... (the "nino") is shown to be the lightest supersymmetric particle with a relic abundance near the critical...”
Published 1986
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148“... at high temperature, DM is then found to have mass around TeV≲mX≲1011 GeV to get the right relic abundance...”
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149“... particles may annihilate into charged fermions that produce gamma-ray to be observed. In this paper, we...”
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150by Mark D. Goodsell, Sabine Kraml, Humberto Reyes-González, Sophie L. Williamson“... for at least part of the observed relic abundance while evading constraints from DM direct detection, LEP...”
Published 2020-10-01
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151“... abundance for this composition of the DM is analyzed as well as the DM particles scattering off nucleons. A...”
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152“... is rapid enough. We investigate the relic abundance in the freeze-in and dark freeze-out regimes, calculate...”
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153by Freya Blekman, Nishita Desai, Anastasiia Filimonova, Abanti Ranadhir Sahasransu, Susanne Westhoff“...-annihilation sets the relic abundance upon freeze-out. At the LHC, searches for soft displaced leptons...”
Published 2020-11-01
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154“... this process, we find that it is possible to obtain the correct relic abundance for dark matter masses...”
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156“... in predicting relic abundances of matter. Examples of renormalizable models realizing this scenario...”
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157“... an important role in producing the current dark matter relic abundance of the universe, showing a strong...”
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158“... of DM on the thermal bath particles is sup-pressed. This leads to the early kinetic decoupling of DM...”
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159“... 4 or E 8. We compute their relic abundance generated by gravitational freeze-in and by inflationary...”
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160“... below 1025 GeV. The scenario where the thermal relic abundance of a Higgsino accounts for the whole dark...”
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