From the 1 of 18 linked papers with an AI index.
18 papers
The equation of state for neutron stars
Veronica Dexheimer
This chapter is intended as an introduction to dense matter and the equation of state of neutron stars and their mergers. It begins with a brief description of neutron star interio…
Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties
Isaac Legred, Mateus Reinke Pelicer, Veronica Dexheimer +2
The paper presents a neural‑accelerated Bayesian framework that uses a surrogate neural network to efficiently calibrate chiral mean‑field nuclear interaction models against nuclea…
Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine
Johannes Jahan, Kevin P. Pala, Yumu Yang +42
The equation of state of hot and dense matter is essential for describing heavy-ion collisions at all collision energies. Here, we explore the capabilities of the latest version of…
S-wave kaon condensation in neutron-star matter within a chiral model framework with dynamical meson masses
Yuhan Wang, Rajesh Kumar, Joaquin Grefa +4
We investigate s-wave kaon condensation in dense matter and neutron stars within the updated Chiral Mean Field model with an improved meson description (mCMF), which incorporates d…
Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state
Nikolas Cruz-Camacho, Carlos Conde-Ocazionez, Veronica Dexheimer +2
The equation of state of matter at supranuclear densities governs the astrophysical observables of neutron stars. A realistic, though complex, description is provided by the Chiral…
Many-body effects on dense matter with hyperons at finite temperature
Rafael Bán Jacobsen, Ricardo Luciano Sonego Farias, Veronica Dexheimer
In this work, we present the first extension of the Many-Body Forces (MBF) Model to finite temperature. The MBF Model describes nuclear matter in a relativistic quantum hadrodynami…