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Neutron star properties from semiclassical methods in nuclear physics

Authors: Constança Providência

Ref.: Conference on Quantum-Many-Body Correlations in memory of Peter Schuck (QMBC 2023). IJCLab, Orsay, France (2023)

Abstract: What does a minimal set of nuclear matter constraints together with a 2M condition tell us about the neutron star EOS based on a microscopic model? Can we get the neutron star composition? Which are possible signatures of the presence of hyperons inside neutron stars? How can we describe the warm non-homogeneous stellar matter self-consistently?

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