Index of equations of state files

file name	description

eosA		PANDHARIPANDE NEUTRON: A&B EOS A
eosAU		WFF1 (denoted AV14+UVII in WFF) matched to Negele-Vautherin
eosB		PANDHARIPANDE HYPERON: A&B EOS B
eosC		BETHE-JOHNSON MODEL 1: A&B EOS C
eosF		PANDHARIPANDE (HYPERON) AND ARPONEN: A&B EOS F
eosFP		FRIEDMAN&PANDHARIPANDE EOS.(NEGELE-VAUTHERIN FOR 
			N<.1FM**-3,THEN * BPS FOR N<.001FM**-3)
eosFPS	        Lorenz, Ravenhall and Pethick, 1993, PRL 70,379
eosG		CANUTO-CHITRE (SOLID): A&B EOS G 
eosL		PANDHARIPANDE AND SMITH (MEAN FIELD): A&B EOS L
eosN		WALECKA-SEROT: A&B EOS N
eosNV		Negele & Vautherin, 1973, Nucl. Phys. A207, 298
eosO		BOWERS, GLEESON, AND PEDIGO. A&B EOS O
eosUU		WFF2 (denoted UV14+UVII in WFF) matched to Negele-Vautherin
eosWNV		WFF3 (denoted UV14+TNI in WFF) matched to Negele-Vautherin
eosWS		WFF3 (UV14+TNI) mathed to EOS FPS

A&B = Arnett and Bowers (1977) APJS 33, 415
WFF = Wiringa, Fiks and Fabrocini (1988), Phys. Rev. C 38, 1010


The equation of state files are in the format required for 
Nikolaos Stergioulas' rotating star codes:     
rns.c	(rapidly rotating neutron stars in equilibrium) 

The format required is as follows:
line 1) number of tabulated points in file
remaining lines) four columns:

column 1) energy density/c^2 	(g/cm^3)
column 2) pressure		(dynes/cm^2)
column 3) enthalpy 		(cm^2/s^2)
column 4) baryon number density (cm^{-3})

The program HnG.c can be used to convert an equation of state in the form
energy density vs pressure to Nick's format. Look at a listing of the 
c code to learn how to use  the program.