Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
Mikhail V. Beznogov, Adriana R. Raduta

TL;DR
This paper develops Bayesian models for the dense matter equation of state using extended Skyrme interactions, incorporating physical constraints to improve the realism of neutron star and nuclear matter predictions.
Contribution
It introduces a Bayesian framework with new physical constraints, notably the neutron Fermi velocity limit, to refine Skyrme-based dense matter models.
Findings
Constraints significantly influence the EOS and neutron star properties.
Imposing the neutron Fermi velocity limit improves model physicality.
Comparison shows differences with previous Skyrme-based results.
Abstract
The non-relativistic model of nuclear matter with Brussels extended Skyrme interactions is employed in order to build, within a Bayesian approach, models for the dense matter equation of state (EOS). In addition to a minimal set of constraints on nuclear empirical parameters; the density behavior of the energy per particle in pure neutron matter (PNM); a lower limit on the maximum neutron star (NS) mass, we require that the Fermi velocity of neutrons () in PNM and symmetric nuclear matter (SNM) with densities up to (arbitrary) does not exceed the speed of light. The latter condition is imposed in order to cure a deficiency present in many Skyrme interactions [Duan and Urban, Phys. Rev. C 108, 025813 (2023)]. We illustrate the importance of this constraint for the posterior distributions. Some of our models are subjected to constraints on the…
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
TopicsCold Atom Physics and Bose-Einstein Condensates · Theoretical and Computational Physics · Advanced Thermodynamics and Statistical Mechanics
