Results 1 to 10 of about 164,049 (174)
Thermal production of cold “hot dark matter” around eV [PDF]
A very simple production mechanism of feebly interacting dark matter (DM) that rarely annihilates is thermal production, which predicts the DM mass around eV. This has been widely known as the hot DM scenario.
Wen Yin
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Indirect detection of hot dark matter
Cosmologically stable, light particles that came into thermal contact with the Standard Model in the early universe may persist today as a form of hot dark matter.
Jeff A. Dror +3 more
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A model for mixed warm and hot right-handed neutrino dark matter [PDF]
We discuss a model where a mixed warm and hot keV neutrino dark matter rises naturally. We arrange active and sterile neutrinos in the same SU(3) L multiplet, with the lightest sterile neutrino being dark matter.
Maíra Dutra +3 more
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Hot new early dark energy: Towards a unified dark sector of neutrinos, dark energy and dark matter [PDF]
Hot new early dark energy describes a supercooled, first-order phase transition that takes place at sub-eV temperatures in the dark sector. It lowers the sound horizon, which provides a possible solution to the Hubble tension, and, at the same time, it ...
Florian Niedermann, Martin S. Sloth
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Hot and heavy dark matter from a weak scale phase transition [PDF]
We point out that dark matter which is produced non-adiabatically in a phase transition (PT) with fast bubble walls receives a boost in velocity which leads to long free-streaming lengths.
Iason Baldes, Yann Gouttenoire, Filippo Sala
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Dark matter as a heavy thermal hot relic [PDF]
If, during the early Universe epoch, the dark matter particle thermalizes in a hidden sector which does not thermalize with the Standard Model thermal bath, its relativistic thermal decoupling can easily lead to the observed relic density, even if the ...
Thomas Hambye +2 more
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Improved Hot Dark Matter Bound on the QCD Axion [PDF]
6+8 pages, 7 ...
Alessio Notari +2 more
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Model of the Galaxy with Hot Dark Matter
The model of the galaxy is considered as a structure of the baryonic matter embedded into the hot dark matter. The dark matter is supposed to come into being from the decaying matter after the epoch of structure formation.
Khokhlov Dmitri L.
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Hot leptogenesis from thermal Dark Matter [PDF]
29 pages, 11 figures.
Bernal, Nicolás, Fong, Chee Sheng
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Gravity as a portal to reheating, leptogenesis and dark matter [PDF]
We show that a minimal scenario, utilizing only the graviton as an intermediate messenger between the inflaton, the dark sector and the Standard Model (SM), is able to generate simultaneously the observed relic density of dark matter (DM), the baryon ...
Basabendu Barman +4 more
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