Statistics – Computation
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123..103s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 103-115.
Statistics
Computation
3
Abundance, Computational Astrophysics, Cosmology, Light Elements, Mass Distribution, Stellar Evolution, Alpha Particles, Gravitational Collapse, Radiation Distribution, Star Distribution, Stellar Mass Ejection, Universe
Scientific paper
The abundances of light elements (deuterium, helium and lithium) are calculated in unconventional cosmologies in which these elements are produced by interaction of fast α-particles ejected by massive pregalactic stars with a purely hydrogeneous cosmological substrate. The number density and energetics of such stars needed for suitable production of light elements are estimated. It is shown that the models always lead to overproduction of lithium. The intensity of ultraviolet, X-ray, and γ-ray emission caused by explosions of pregalactic massive stars is calculated. The distortions of cosmic background radiation by Compton losses of electrons heated by explosive stars are also calculated.
Shchekinov Iu. A.
Vainer Boris V.
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