Microscopic equation of state (EoS) of dense beta-stable nuclear matter at zero temperature (T=0) obtained using realistic two-body and three-body nuclear interactions derived in the framework of chiral perturbation theory (ChPT) and including the Delta(1232) isobar intermediate state. This EoS has been derived using the Brueckner-Bethe-Goldstone quantum many-body theory in the Brueckner-Hartree-Fock approximation with the continuous choice for the auxiliary single particle potential. The present table is relative to the nuclear interaction model denoted as N3LODelta+N2LODelta in [BL_2018]. It contains the contributions from electrons and muons in addition to beta-stable nuclear matter.
Nuclear Matter Properties
Neutron Star Properties
References to the original work:
- [BL_2018] I. Bombaci and D. Logoteta, Astron. and Astrophys. 609, A128 (2018)