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Common origin of warm dark matter and dark radiation [PDF]
Journal of Cosmology and Astroparticle Physics, 2020 We consider a cosmological scenario where a relativistic particle and a stable massive particle are simultaneously produced from the decay of a late-decaying particle after Big-Bang Nucleosynthesis but before matter-radiation equality. The relativistic and massive particles behave as dark radiation and warm dark matter, respectively.
Buen-Abad, Manuel A. +2 more
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Cosmological constraints on variable warm dark matter [PDF]
Physics Letters B, 2013 11 pages, 6 figures, 1 table, revtex4; v2: discussions added, Phys. Lett.
Hao Wei, Zu-Cheng Chen, Jing Liu
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New constraints on warm dark matter from the Lyman-
Physical Review D, 2022 The forest of Lyman-$\alpha$ absorption lines detected in the spectra of distant quasars encodes information on the nature and properties of dark matter and the thermodynamics of diffuse baryonic material.
B. Villasenor +3 more
semanticscholar +1 more source
Interacting warm dark matter [PDF]
Journal of Cosmology and Astroparticle Physics, 2013 22 pages, 7 figures, 2 tables.
Cruz, Norman +3 more
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A model for mixed warm and hot right-handed neutrino dark matter
Journal 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
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The energy cascade from warm dark matter decays [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2008 Abstract We use a set of Monte Carlo simulations to follow the cascade produced by a primary electron of energy Ein in the intergalactic medium. We choose Ein= 3–10 keV as expected from the decay of one of the most popular warm dark matter (WDM) candidates, sterile neutrinos.
M. Valdés, Andrea Ferrara
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Warm-plus-hot neutrino dark matter [PDF]
Physical Review D, 1995 We investigate a new hybrid-model universe containing two types of dark matter, one ``warm'' and the other ``hot.'' The hot component is an ordinary light neutrino with mass \ensuremath{\sim}25${\mathit{h}}^{2}$ eV while the warm component is a sterile neutrino with mass \ensuremath{\sim}700${\mathit{h}}^{2}$ eV.
, Malaney, , Starkman, , Widrow
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Dark matter in astrophysics/cosmology
SciPost Physics Lecture Notes, 2022 These lecture notes aim to provide an introduction to dark matter from the perspective of astrophysics/cosmology. We start with a rapid overview of cosmology, including the evolution of the Universe, its thermal history and structure formation.
Anne M. Green
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Warm Little Inflaton Becomes Cold Dark Matter [PDF]
Physical Review Letters, 2019 6 pages, 2 figures; Matches version published in Physical Review ...
Rosa, João G., Ventura, Luís B.
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Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation [PDF]
, 2022 Precision analysis of galaxy-galaxy strong gravitational lensing images provides a unique way of characterizing small-scale dark matter halos, and could allow us to uncover the fundamental properties of dark matter's constituents. Recently, gravitational
Noemi Anau Montel +4 more
semanticscholar +1 more source