Analytical representations of unified equations of state of neutron-star matter

By A. Potekhin, A. Fantina, N. Chamel, J. Pearson, S. Goriely. 2004

299 citations recorded by the source corpus.

Analytical representations are derived for two equations of state (EOSs) of neutron-star matter: FPS and SLy. Each of these EOSs is unified, that is, it describes the crust and the core of a neutron star using the same physical model. Two versions of the EOS parametrization are considered. In the first one, pressure and mass density are given as functions of the baryon density. In the second version, pressure, mass density, and baryon density are given as functions of the pseudo-enthalpy, which makes this representation particularly useful for 2-D calculations of stationary rotating configurations of neutron stars.

Subfields: Astronomy and Astrophysics, Geophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/26296c4f54045192c812c05ddd0a4a2d5a0d6de2

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In Astronomy and Astrophysics

  1. Diego Rubiera-García
  2. José A. Pons
  3. D. Page
  4. G. Fiorella Burgio
  5. Aneta Wojnar
  6. A. Potekhin
  7. Marc A. Baldo
  8. M. Centelles

In Geophysics

  1. G. Fiorella Burgio
  2. José A. Pons
  3. D. Page
  4. Marc A. Baldo
  5. Diego Rubiera-García
  6. G. Olmo
  7. Aneta Wojnar
  8. A. Potekhin

In Nuclear and High Energy Physics

  1. G. Fiorella Burgio
  2. Diego Rubiera-García
  3. Aneta Wojnar
  4. José A. Pons
  5. D. Page
  6. Marc A. Baldo
  7. M. Centelles
  8. B. Sharma

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