http://arxiv.org/abs/2110.02616
Neutron stars are unique laboratories to probe matter in extreme conditions, not accessible in terrestrial laboratories. Here, we discuss the modelling of the neutron-star equation of state, particularly in connection with recent constraints coming from both nuclear physics (experiments and ab-initio calculations) and astrophysical observations.
F. Gulminelli and A. Fantina
Thu, 7 Oct 21
13/51
Comments: 8 pages, 3 figures