Results 131 to 140 of about 695,053 (252)
Upper bound on hot dark matter density from SO(10) Yukawa unification [PDF]
Andrea Brignole +2 more
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Hydro-Gravitational Dynamics of Planets and Dark Energy
Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the 0.3 Myr ...
Carl H. Gibson, R.E, Schild
doaj
Direct detection of hot dark matter including light sterile neutrinos [PDF]
Yufeng Li, Zhi‐zhong Xing
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Refracted Gravity Solutions from Small to Large Scales
If visible matter alone is present in the Universe, general relativity (GR) and its Newtonian weak field limit (WFL) cannot explain several pieces of evidence, from the largest to the smallest scales.
Valentina Cesare
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COLD + HOT AND COLD DARK MATTER COSMOLOGIES: ANALYSIS OF NUMERICAL SIMULATIONS [PDF]
Anatoly Klypin +2 more
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Galaxy clusters, the most massive, dark-matter-dominated, and most recently assembled structures in the Universe, are key tools for probing cosmology.
Giulia Cerini +6 more
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Electron Neutrino Mass Measurement by Supernova Neutrino Bursts and Implications on Hot Dark Matter
Tomonori Totani
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Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure [PDF]
Nascimento, Caio B. de S. +1 more
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Statistics that capture the directional dependence of the baryon distribution in the cosmic web enable unique tests of cosmology and astrophysical feedback.
M. Lokken +75 more
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Evolution of Clusters in Cold Plus Hot Dark Matter Models [PDF]
Charles Walter, Anatoly Klypin
openalex +1 more source

