Neutron stars, strange stars, and the nuclear equation of state
Description:
This article consists of three parts. In part one we review the present status of dense nuclear matter calculations, and introduce a representative collection of realistic nuclear equations of state which are derived for different assumptions about the physical behavior of dense matter (baryon population, pion condensation,.possible transition of baryon matter to quark matter). In part two we review recently performed non-rotating and rotating compact star calculations performed for these equat…
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Date:
November 2, 1992
Creator:
Weber, F. & Glendenning, N.K.
Item Type:
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UNT Libraries Government Documents Department