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Interacting Hot Dark Matter [PDF]

open access: greenPhysical Review D, 1997
We discuss the viability of a light particle ($\sim 30$ eV neutrino) with strong self-interactions as a dark matter candidate. The interaction prevents the neutrinos from free-streaming during the radiation dominated regime so galaxy sized density ...
Atrio-Barandela, Fernando   +1 more
core   +7 more sources

Indirect detection of hot dark matter [PDF]

open access: greenJournal of High Energy Physics
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   +4 more sources

Hot new early dark energy: Towards a unified dark sector of neutrinos, dark energy and dark matter

open access: diamondPhysics Letters B, 2022
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   +2 more sources

A model for mixed warm and hot right-handed neutrino dark matter [PDF]

open access: diamondJournal of High Energy Physics, 2021
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

THE HOT DARK MATTER MODEL: FURTHER INVESTIGATION

open access: yesOdessa Astronomical Publications, 2020
e outer region with the dominant hot dark matter (the parabolic orbit of the test particle). It was assumed that the hot dark matter consists of hypothetical Planck neutrinos arising in the decay of the protons at the Planck scale.
D. L. Khokhlov
doaj   +3 more sources

Dark matter as a heavy thermal hot relic

open access: yesPhysics Letters B, 2020
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   +4 more sources

Violation of universal lower bound for the shear viscosity to entropy density ratio in dark energy dominated accretion

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
The universal lower bound of the ratio of shear viscosity to entropy density is suggested by the string theory and gauge duality for any matter. We examined the ratio of shear viscosity to entropy density for viscous accretion flow towards a central ...
Sandip Dutta, Ritabrata Biswas
doaj   +3 more sources

Saxion cosmology for thermalized gravitino dark matter

open access: yesJournal of High Energy Physics, 2017
In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too hot, and is ...
Raymond T. Co   +3 more
doaj   +3 more sources

Polarized equatorial emission and hot spots around black holes with a dark matter halo [PDF]

open access: diamondEuropean Physical Journal C: Particles and Fields
We study linear polarization of the accretion disks around black holes with a dark matter halo. The interaction of the black hole with the dark matter is modeled by considering an exact solution to the Einstein equations which describe a superposition of
Tsanimir Angelov   +4 more
doaj   +2 more sources

Thermal production of cold “hot dark matter” around eV

open access: yesJournal of High Energy Physics, 2023
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   +1 more source

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