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

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arxiv 1002.4497 v2 pith:WZKOAUHQ submitted 2010-02-24 astro-ph.SR nucl-th

G.F. Burgio , H.-J. Schulze (INFN Catania , Italy) This is my paper · ORCID
classification astro-ph.SRnucl-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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  1. Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state

    nucl-th 2024-11 conditional novelty 6.0 of 10

    For chirally constrained nuclear equations of state, the minimal proto-neutron star mass is about 0.62 solar masses with trapped neutrinos (YL=0.4, s=1) and about 0.22 solar masses after deleptonization (s=2).

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