Results 1 to 10 of about 32,390 (153)
Model of the Galaxy with Hot Dark Matter [PDF]
Abstract 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. The galaxy is divided into two regions. In the inner region, the baryonic matter predominates over the hot dark matter
Khokhlov Dmitri L.
exaly +3 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 dark matter particle mass is many orders of magnitude heavier than the usual $\sim$ eV hot relic mass ...
Laurent Vanderheyden +2 more
exaly +5 more sources
Hot new early dark energy: Towards a unified dark sector of neutrinos, dark energy and dark matter
10 pages, 1 figure, v3: matches published version; added detailed discussion of model's signatures and figure with constraints on heaviest neutrino ...
Florian Niedermann, Martin S Sloth
exaly +5 more sources
Improved Hot Dark Matter Bound on the QCD Axion
6+8 pages, 7 ...
Fabrizio Rompineve +2 more
exaly +4 more sources
Biodiversity and emerging infectious threats: the microbial dark matter of Southwest China. [PDF]
Southwest China is a global biodiversity hotspot, and its complex and diverse ecosystems harbor vast amounts of “microbial dark matter.” This paper systematically examines the distribution characteristics of microbial dark matter in hosts such as ...
Guo N, Liu Z, Li Z, Xu J.
europepmc +2 more sources
Indirect detection of hot dark matter
A bstract 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. For relics with masses in the eV range, their role in structure formation depends
Jeff A. Dror +3 more
openaire +3 more sources
Thermal production of cold “hot dark matter” around eV
Abstract 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. Despite there are several observational hints from background lights suggesting a DM in this mass range, the hot ...
Wen Yin
openaire +4 more sources
THE HOT DARK MATTER MODEL: FURTHER INVESTIGATION
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. Galaxies formed from the baryonic matter, and the hot dark matter appears in the galaxies later.
D. L. Khokhlov
openaire +5 more sources
THE CASE OF 1.5 eV NEUTRINO HOT DARK MATTER [PDF]
3 pages, Proceedings Marcel Grossmann XII, Paris ...
exaly +3 more sources
Interference with gravitational instability: Hot and fuzzy dark matter
Wave or fuzzy dark matter produced with high momenta behaves in many ways like hot particle dark matter while also possessing seemingly different phenomenology due to wave interference. We develop wave perturbation theory to show that white noise density fluctuations generated by the interference of high-momenta waves are gravitationally unstable in ...
Huangyu Xiao, Rayne Liu, Wayne Hu
exaly +3 more sources

