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Published June 7, 2024 | Version v1.1
Software Open

Code for: "One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations". Pearson-Potekhin fitting scheme

  • 1. ROR icon Laboratoire de Physique Corpusculaire de Caen
  • 2. ROR icon Paris Observatory
  • 3. ROR icon University of Alicante

Description

This project contains a series of python scripts that performs an analytical fit to one- or two-argument equations of state (EoS, i.e. pressure as a function of mass-energy density, or pressure as a function of mass-energy density and electronic charge fraction) from the CompOSE database. We use the analytical respresentation described by Haensel & Potekhin 2004, A&A, 428, 191-197 and Pearson et al. 2018, MNRAS, 481, 2994-3026 to perform a fit to the high-density core region, while a polytropic model is added for the crust. We use the Generalised Piecewise Polytrope scheme described in Boyle et al. 2020, Phys. Rev. D, 102, 083027 to ensure continuity in pressure, sound speed and energy-density across the crust-core boundary.

Notes

This code was developed within the framework of the Agence Nationale de la Recherche (ANR) under contract ANR-22-CE31-0001-01 and from the CNRS International Research Project (IRP) “Origine des éléments lourds dans l’univers: Astres Compacts et Nucléosynthèse (ACNu)”.

Technical info

The code makes use of the CompStar Online Supernovae Equations of State (CompOSE) database as well as the corresponding software.

Files

Files (92.1 MB)

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md5:77696ef6dc750c67be70311fbdb22e50
92.1 MB Download

Additional details

Related works

Is documented by
Journal article: 10.1103/PhysRevD.109.103022 (DOI)

Software

Repository URL
https://gitlab.obspm.fr/data_and_software_compose/fit_pearson-potekhin
Programming language
Python
Development Status
Active