Results 31 to 40 of about 556,485 (362)

Gravitino Warm Dark Matter with Entropy Production [PDF]

open access: greenJournal of High Energy Physics, 2001
Gravitinos with a mass in the keV range are an interesting candidate for warm dark matter. Recent measurements of the matter density of the universe and of cosmic structures at the dwarf galaxy scale rule out the simplest gravitino models with thermal freeze-out.
Edward A. Baltz, Murayama, Hitoshi
openalex   +3 more sources

Strongly coupled dark energy with warm dark matter vs. LCDM [PDF]

open access: greenJournal of Cosmology and Astroparticle Physics, 2017
Cosmologies including strongly Coupled (SC) Dark Energy (DE) and Warm dark matter (SCDEW) are based on a conformally invariant (CI) attractor solution modifying the early radiative expansion. Then, aside of radiation, a kinetic field $ $ and a DM component account for a stationary fraction, $\sim 1\, \%$, of the total energy.
S. A. Bonometto   +2 more
openalex   +4 more sources

Implications of the Stellar Mass Density of High-z Massive Galaxies from JWST on Warm Dark Matter [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2023
A significant excess of the stellar mass density at high redshift has been discovered from the early data release of James Webb Space Telescope (JWST), and it may require a high star formation efficiency.
Hengjie Lin   +3 more
semanticscholar   +1 more source

thesan-hr: Galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter and interacting dark matter [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
Using high-resolution cosmological radiation-hydrodynamic (RHD) simulations (thesan-hr), we explore the impact of alternative dark matter (altDM) models on galaxies during the Epoch of Reionization.
Xuejian Shen   +10 more
semanticscholar   +1 more source

Massive prompt cusps: A new signature of warm dark matter [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2023
Every dark matter halo and subhalo is expected to have a prompt ρ∝r−1.5 central density cusp, which is a relic of its condensation out of the smooth mass distribution of the early universe.
M. Sten Delos
semanticscholar   +1 more source

Understanding the Formation of Galaxies with Warm Dark Matter [PDF]

open access: yesJournal of Modern Physics, 2023
The formation of galaxies with warm dark matter is approximately adiabatic. The cold dark matter limit is singular and requires relaxation. In these lecture notes we develop, step-by-step, the physics of galaxies with warm dark matter, and their ...
B. Hoeneisen
semanticscholar   +1 more source

Extending the unified subhalo model to warm dark matter [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
Using a set of high-resolution N-body simulations, we extend the unified distribution model of cold dark matter (CDM) subhaloes to the warm dark matter(WDM) case.
Feihong He   +3 more
semanticscholar   +1 more source

Warm Dark Matter from Higher-Dimensional Gauge Theories

open access: yesUniverse, 2021
Warm dark matter particles with masses in the keV range have been linked with the large group representations in gauge theories through a high number of species at decoupling.
Sinziana Paduroiu   +3 more
doaj   +1 more source

Warm dark Matter constraints from the joint analysis of CMB, Lyman-α, and global 21 cm data [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
With the help of our previously built MCMC-based parameter estimation package CosmoReionMC, we investigate in detail the potential of 21 cm global signal, when combined with CMB and observations related to the QSO absorption spectra, to constraint the ...
Atrideb Chatterjee, T. R. Choudhury
semanticscholar   +1 more source

Primordial black-hole dark matter via warm natural inflation

open access: yesPhysics Letters B, 2022
We report on a study of the natural warm inflationary paradigm (WNI). We show two important new results arise in this model. One is that the observational constraints on the primordial power spectrum from the cosmic microwave background (CMB) can be ...
Miguel Correa   +3 more
doaj   +1 more source

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