Protoneutron stars with kaon condensate
Nuclear Theory
2009-10-31 v1
Abstract
A new formulation is presented to treat fluctuations around the kaon condensate. Equation of state (EOS) is given for isothermal and isentropic cases in the heavy-baryon-limit (HBL). The coexistent phase appears in the latter case. The mass-radius relation is given for protoneutron stars and the possibility of the delayed collapse is discussed.
Cite
@article{arxiv.nucl-th/9904038,
title = {Protoneutron stars with kaon condensate},
author = {Toshitaka Tatsumi and Masatomi Yasuhira},
journal= {arXiv preprint arXiv:nucl-th/9904038},
year = {2009}
}
Comments
6 pages