From the 1 of 5 linked papers with an AI index.
5 papers
Nuclear matter equation of state and astrophysics
Mateus Reinke Pelicer
Neutron-star masses, radii, and inspiral tidal deformabilities now provide quantitative constraints on the cold equation of state (\eos), favoring relatively soft matter around one…
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…
An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars
Mateus Pelicer, Veronica Dexheimer, Joaquin Grefa
For densities beyond nuclear saturation, there is still a large uncertainty in the equations of state (EoS) of dense matter that translate into uncertainties in the internal struct…
Building Neutron Stars with the MUSES Calculation Engine
Mateus Reinke Pelicer, Nikolas Cruz-Camacho, Carlos Conde +25
Exploring the equation of state of dense matter is an essential part of interpreting the observable properties of neutron stars. We present here the first results for dense matter…