Neutron Star Group

Analytical Representations of Equations of State of Neutron Star Matter These analytical representations are designed for older equations of state FPS and SLy4. For newer equations of state BSk19-20-21, see this http URL.

	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

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Page created on April 5, 2004, last updated on May 20, 2007 by Alexander Potekhin.