Captures of Hot and Warm Sterile Antineutrino Dark Matter on EC-decaying Ho-163 Nuclei [PDF]
, 2011 Capturing low-energy electron antineutrinos on radioactive Ho-163 nuclei, which decay into Dy-163 via electron capture (EC), is a noteworthy opportunity to detect relic sterile antineutrinos.
Li, Y. F., Xing, Zhi-zhong
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Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter [PDF]
Monthly Notices of the Royal Astronomical Society, 2012 We describe a methodology to accurately compute halo mass functions, progenitor mass functions, merger rates and merger trees in non-cold dark matter universes using a self-consistent treatment of the generalized extended Press-Schechter formalism.
Benson, Andrew J. +8 more
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Warm Dark Matter versus Bumpy Power Spectra [PDF]
Monthly Notices of the Royal Astronomical Society, 2002 In this paper we are exploring the differences between a Warm Dark Matter model and a CDM model where the power on a certain scale is reduced by introducing a narrow negative feature ("dip").
Alexander Knebe +20 more
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Warm dark matter chills out: constraints on the halo mass function and the free-streaming length of dark matter with eight quadruple-image strong gravitational lenses [PDF]
Monthly notices of the Royal Astronomical Society, 2019 The free-streaming length of dark matter depends on fundamental dark matter physics, and determines the abundance and concentration of dark matter haloes on sub-galactic scales.
Daniel Gilman +5 more
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Indistinguishability of Warm Dark Matter, Modified Gravity, and Coupled Cold Dark Matter [PDF]
Physical Review D, 2013 The current accelerated expansion of our universe could be due to an unknown energy component with negative pressure (dark energy) or a modification to general relativity (modified gravity).
Chen, Zu-Cheng +3 more
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Warm Dark Matter Sterile Neutrinos in Electron Capture and Beta Decay Spectra [PDF]
Advances in High Energy Physics, 2016 We briefly review the motivation to search for sterile neutrinos in the keV mass scale, as dark matter candidates, and the prospects to find them in beta decay or electron capture spectra, with a global perspective.
O. Moreno +2 more
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Free streaming in warm wave dark matter [PDF]
Journal of Cosmology and Astroparticle PhysicsWe provide a framework for numerically computing the effects of free-streaming in scalar fields produced after inflation. First, we provide a detailed prescription for setting up initial conditions in the field. This prescription allows us to specify the
Siyang Ling, Mustafa A. Amin
semanticscholar +4 more sources
REIONIZATION IN THE WARM DARK MATTER MODEL [PDF]
The Astrophysical Journal, 2012 Compared with the cold dark matter (CDM) model, in the warm dark matter (WDM) model formation of small scale structure is suppressed. It is often thought that this would delay the reionization of the intergalactic medium (IGM), as the star formation rate during the epoch of reionization (EOR) would be lowered. However, during the later stage of the EOR,
Bin Yue, Xuelei Chen
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Early galaxy formation in warm dark matter cosmologies [PDF]
The Astrophysical Journal, 2015 We present a framework for high-redshift ($z \geq 7$) galaxy formation that traces their dark matter (DM) and baryonic assembly in four cosmologies: Cold Dark Matter (CDM) and Warm Dark Matter (WDM) with particle masses of $m_x =$ 1.5, 3 and 5 ${\rm keV}$
Dayal, Pratika +2 more
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Linear Cosmological Structure Limits on Warm Dark Matter [PDF]
Physical Review D, 2005 I consider constraints from observations on a cutoff scale in clustering due to free streaming of the dark matter in a warm dark matter cosmological model with a cosmological constant.
G. Kauffmann +3 more
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