From the 1 of 21 linked papers with an AI index.
21 papers
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…
Donutization Inside Neutron Stars: Shell-Localized Scalar Fields
Hao-Jui Kuan, Alan Tsz-Lok Lam, Jacquelyn Noronha-Hostler +1
Heavy scalar fields ( eV) in scalar-tensor gravity are expected to be hidden from neutron-star observations because their Compton wavelength is sub-stellar. We…
Symmetry Energy Expansion with Strange Dense Matter
Yumu Yang, Nikolas Cruz Camacho, Mauricio Hippert +1
The quantum chromodynamics (QCD) phase diagram at large densities and low temperatures can be probed using both neutron stars and low-energy heavy-ion collisions. Heavy-ion collisi…
Dynamical tidal response of neutron stars as a probe of dense-matter properties
Abhishek Hegade K. R., Yumu Yang, Mauricio Hippert +4
Dynamical tidal deformations play a crucial role in the gravitational waves emitted by binary neutron star systems during their late inspiral. In this work, we systematically explo…
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…