Physics
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pthph..66.1504h&link_type=abstract
Progress of Theoretical Physics, Vol. 66, No. 4, pp. 1504-1507
Physics
Scientific paper
We study the evolution of a Super-Massive Star (SMS) in a dense stellar
and primordial black holes' system. The dissipation of kinetic energy of
the holes via gravitational interaction in the SMS becomes greater than
the critical luminosity. This quasi pile stage continues for about 1
× 104 years.
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