Physics
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..278..297s&link_type=abstract
Physics Letters B, Volume 278, Issue 3, p. 297-301.
Physics
3
Scientific paper
The discussions on Q-stars are extended to finite temperature. We find
that below the critical temperature Tc the radius, mass and
the frequency of the Q-star will increase with temperature. The critical
temperature at which the Q-star will disappear and the epoch in which
the Q-star can exist are given.
Pan Rong-Shi
Su Cheng-Gang
Su Ru-Keng
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