The \(\varSigma \) well depth and the proto neutron star matter

DOI10.1007/s10773-012-1349-6zbMath1263.85031OpenAlexW1979132319MaRDI QIDQ1945422

Li Zhang, Xian Feng Zhao

Publication date: 8 April 2013

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-012-1349-6

zbMATH Keywords

baryon octetrelativistic mean field theoryproto neutron star

Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Cites Work

• Unnamed Item
• Magnetorotational instability in proto-neutron stars
• Effects of quark matter nucleation on the evolution of proto-neutron stars

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