Results 1 to 10 of about 579,498 (204)
Indirect detection of hot dark matter [PDF]
Journal of High Energy PhysicsCosmologically 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
Axion hot dark matter bounds [PDF]
, 2008 We derive cosmological limits on two-component hot dark matter consisting of neutrinos and axions. We restrict the large-scale structure data to the safely linear regime, excluding the Lyman-alpha forest.
Hannestad, S. +3 more
core +4 more sources
Hot new early dark energy: Towards a unified dark sector of neutrinos, dark energy and dark matter
Physics 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
Hot leptogenesis from thermal Dark Matter [PDF]
Journal of Cosmology and Astroparticle Physics, 2017 29 pages, 11 figures.
Nicolás Bernal, Chee Sheng Fong
openalex +4 more sources
Improved Hot Dark Matter Bound on the QCD Axion [PDF]
Physical Review Letters, 2023 6+8 pages, 7 ...
Alessio Notari +2 more
openalex +4 more sources
Hot and heavy dark matter from a weak scale phase transition [PDF]
SciPost Physics, 2023 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 +4 more sources
Hidden Hot Dark Matter as Cold Dark Matter [PDF]
, 2009 We show that hidden hot dark matter, hidden-sector dark matter with interactions that decouple when it is relativistic, is a viable dark matter candidate provided it has never been in thermal equilibrium with the particles of the standard model.
Sigurdson, Kris
core +4 more sources
Interacting Hot Dark Matter [PDF]
Physical 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 +5 more sources
Hot QCD and warm dark matter [PDF]
Proceedings of XXIVth International Symposium on Lattice Field Theory — PoS(LAT2006), 2006 One of the possible explanations for the dark matter needed in the standard cosmological model is so-called warm dark matter, in the form of right-handed ("sterile") neutrinos with a mass in the keV range.
Laine, M.
core +5 more sources