Neutron Star Group

Analytical Representations of Equations of State of Neutron Star Matter These analytical representations are designed for older equations of state FPS, SLy4, and APR. For newer "Brussels-Montreal" equations of state BSk19-22 and BSk24-26, follow this link. For other equations of state, see this collection of links.

	Introduction
	References
	Description of EOS subroutines
	EOS tables and subroutines in Fortran and C/C++

Contact authors:

• Pawel Haensel (CAMK): haensel@camk.edu.pl
• Alexander Potekhin (Department of Theoretical Astrophysics of the Ioffe Institute): palex@astro.ioffe.ru

Please communicate us your opinion and send any suggestions or remarks.

Page created on April 5, 2004, last updated on September 25, 2017 by Alexander Potekhin.