Current status of Dirac-Brueckner-Hartree-Fock calculations in asymmetric nuclear matter
Francesca Sammarruca, Pei Liu
TL;DR
This paper reviews the latest Dirac-Brueckner-Hartree-Fock calculations for asymmetric nuclear matter, providing updated equations of state and discussing implications for neutron star maximum masses.
Contribution
It offers updated microscopic predictions of the equation of state for asymmetric nuclear matter and analyzes their relevance to neutron star properties.
Findings
Updated equations of state for asymmetric nuclear matter.
Predictions of neutron star maximum masses.
Insights into the features of the nuclear matter EoS.
Abstract
We review the current status of our microscopic calculations in asymmetric nuclear matter. Updated predictions of the equation of state are made available to potential users. We discuss the features of our EoS in relation to the predicted neutron star maximum masses.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsQuantum, superfluid, helium dynamics · Nuclear physics research studies · Atomic and Subatomic Physics Research