Published October 14, 2025 | Version v1

Weighted Equation of State samples for "Nonparametric extensions of nuclear equations of state: Probing the breakdown scale of relativistic mean-field theory"

  • 1. ROR icon University of Illinois Urbana-Champaign
  • 2. EDMO icon California Institute of Technology
  • 3. ROR icon Washington University in St. Louis
  • 4. ROR icon Canadian Institute for Theoretical Astrophysics

Description

Nonparametric equation of state samples for 6 different choices of transition pressure for  "Nonparametric extensions of nuclear equations of state: Probing the breakdown scale of relativistic mean-field theory".  See the README.md for more details.  Each hdf5 file contains 30,000 equation of state samples for each choice of transition pressure, and astrophysical weights which correspond to the astrophysical likelihood of the given equation of state from joint gravitational-wave, x-ray pulse-profile, and radio timing measurements of neutron star masses, radii, and tidal deformabilities.  

For each equation of state, we provide tabulated pressure, energy density, baryon rest-mass density and speed of sound.  We also provide sequences of TOV solutions for different central pressures, including the mass, radius, dimensionless tidal deformability, and moment of inertia.  See the README.md for more details.  

 

Files

WeightedRMFTEoSSamples.zip

Files (4.2 GB)

Name Size
md5:3bcd381da72b87a4bc38d3df95c08a8a
4.2 GB Preview Download