The maximum and minimum mass of protoneutron stars in the Brueckner theory
Solar and Stellar Astrophysics
2015-05-18 v2 Nuclear Theory
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.
Keywords
Cite
@article{arxiv.1002.4497,
title = {The maximum and minimum mass of protoneutron stars in the Brueckner theory},
author = {G. F. Burgio and H. -J. Schulze},
journal= {arXiv preprint arXiv:1002.4497},
year = {2015}
}
Comments
8 pages, 8 figures