The maximum and minimum mass of protoneutron stars in the Brueckner theory
classification
🌌 astro-ph.SR
nucl-th
keywords
massprotoneutronequationlow-densitymaximumminimumstarsstate
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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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