The maximum and minimum mass of protoneutron stars in the Brueckner theory
arXiv:1002.4497 · doi:10.1051/0004-6361/201014308
Abstract
We study the structure of protoneutron stars within the finite-temperature Brueckner-Bethe-Goldstone theoretical approach, paying particular attention to how it is joined to a low-density nuclear equation of state (EOS). We find a slight sensitivity of the minimum value of the protoneutron star mass on the low-density equation of state, whereas the maximum mass is hardly affected.
8 pages, 8 figures
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