Statistics – Computation
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...354..302c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 354, May 1, 1990, p. 302-309.
Statistics
Computation
8
Computational Astrophysics, Gravitational Collapse, Solitary Waves, Stellar Interiors, Stellar Mass, Astronomical Models, Baryons, Black Holes (Astronomy), Particle Mass, Quarks, Radiative Transfer
Scientific paper
The structure of nontopological solutions of Einstein field equations as proposed by Friedberg, Lee, and Pang (1987) is examined. This analysis incorporates finite temperature effects and pair creation. Quarks are assumed to be the only species that exist in interior of soliton stars. The possibility of primordial creation of soliton stars in the incomplete decay of the degenerate vacuum in early universe is explored. Because of dominance of pair creation inside soliton stars, the luminosity of soliton stars is not determined by its radiative transfer characteristics, and the surface temperature of soliton stars can be the same as its interior temperature. It is possible that soliton stars are intense X-ray radiators at large distances. Soliton stars are nearly 100 percent efficient energy converters, converting the rest energy of baryons entering the interior into radiation. It is possible that a sizable number of baryons may also be trapped inside soliton stars during early epochs of the universe. In addition, if soliton stars exist they could assume the role played by massive black holes in galactic centers.
No associations
LandOfFree
Massive soliton stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Massive soliton stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Massive soliton stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-779544