Results 121 to 130 of about 695,053 (252)
Decay-Produced Neutrino Hot Dark Matter
Physical Review Letters, 1998 We investigate different types of neutrino hot dark matter with respect to structure formation and anisotropies in the cosmic microwave background radiation (CMBR). The possibility of neutrino hot dark matter produced through the decay of a heavier neutrino by the process nu_H -> nu_L + phi, where phi is a scalar particle, is discussed in detail ...
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Early Objects in the Cosmic String Theory with Hot Dark Matter [PDF]
, 1997 Richhild Moessner, Robert Brandenberger
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Merger Effects on the Spin and Shape Alignments of Galaxy Stellar, Cold and Hot Gas, and Dark Matter Components [PDF]
, 2022 Jounghun Lee, Jun Sung Moon
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The evolution of X-ray clusters in a cold plus hot dark matter universe [PDF]
, 1994 Greg L. Bryan +4 more
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Future cosmological sensitivity for hot dark matter axions [PDF]
, 2015 Maria Archidiacono +11 more
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Structure Formation with Cold + Hot Dark Matter
, 1993 33pp., 16+ figures not included (available by mail), SCIPP-92 ...
Klypin, Anatoly +3 more
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C-19 and Hot, Wide Star Streams
The Astrophysical JournalThe C-19 star stream has the abundance characteristics of an unusually metal-poor globular cluster but kinematically is uncharacteristically hot and wide for a cluster stream, having a line-of-sight velocity dispersion of 7 ± 2 km s ^−1 and a 1 σ width
Raymond G. Carlberg +7 more
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Cosmology: What One Needs to Know
Zygon, 2000 Cosmology, the study of the universe, has a past, which is reviewed here. The standard model—the Big Bang, or the hot, dense early universe that is still expanding—is based on observations that are basically consistent but which require additional input
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Dark Matter and Metal Abundances in Elliptical Galaxies from X-ray\n Observations of the Hot ISM [PDF]
, 1998 Michael Loewenstein
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A Warm-Plus-Hot Dark Matter Universe
, 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 $\sim 25h^2$~eV while the warm component is a sterile neutrino with mass $\sim 700h^2$~eV. The two types of dark matter arise entirely within the neutrino sector and do not require
Malaney, R. A. +2 more
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