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Indirect detection of hot dark matter [PDF]
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
doaj +5 more sources
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
doaj +3 more sources
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
doaj +5 more sources
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
doaj +6 more sources
Improved Hot Dark Matter Bound on the QCD Axion [PDF]
We obtain a reliable cosmological bound on the axion mass m_{a} by (1) deriving the production rate directly from pion-pion scattering data, which overcomes the breakdown of chiral perturbation theory and results in ∼30% differences from previous ...
Alessio Notari +2 more
semanticscholar +6 more sources
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
doaj +2 more sources
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
doaj +2 more sources
Nonthermal hot dark matter from inflaton or moduli decay: Momentum distribution and relaxation of the cosmological mass bound [PDF]
Decay of the inflaton or moduli which dominated the energy density of the universe at early times leads to a matter to radiation transition epoch. We consider non-thermal sterile dark matter particles produced as decay product during such transitions ...
Sukannya Bhattacharya +5 more
openalex +2 more sources
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.
doaj +2 more sources
CosmologicalN-body simulations with generic hot dark matter [PDF]
We have calculated the non-linear effects of generic fermionic and bosonic hot dark matter components in cosmological N-body simulations. For sub-eV masses, the non-linear power spectrum suppression caused by thermal free-streaming resembles the one seen
Jacob Brandbyge, Steen Hannestad
openalex +3 more sources

