We calculate the equation of state for hot dense matter and discuss implications for stellar collapse.
DOI:https://doi.org/10.1103/PhysRevLett.41.1623
©1978 American Physical Society
D. Q. Lamb, J. M. Lattimer, C. J. Pethick*, and D. G. Ravenhall
Vol. 41, Iss. 23 — 4 December 1978
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