The maximum and minimum mass of protoneutron stars in the Brueckner theory

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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8 pages, 8 figures

Scientific paper

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.

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