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BHB(DD2L) (with electrons)

Abstract

This is the hadronic EOS table of Ref. [BHB_2014], which is based on the statistical model of Hempel and Schaffner-Bielich [HSNP_2010] with RMF interactions DD2 [TRKBP_2010] and which has been extended by Lambda hyperons [BHB_2014]. Contributions of neutrons, anti-neutrons, protons, anti-protons, lambdas, anti-lambdas, and nuclei are included. For the masses of nuclei, FRDM [MNKA_1997] was used. The manual from Matthias Hempel's web page gives further information about the EOS table. On this web page, also routines are available which allow to determine the abundances of all nuclei for all conditions.

Nparam = 3
Particles = npe Bs N
T min = 1.00e-01
T max = 1.58e+02
T pts = 81
nb min = 1.00e-12
nb max = 9.99e-01
nb pts = 301
Y min = 1.00e-02
Y max = 6.00e-01
Y pts = 60

Nuclear Matter Properties

ns = 0.0 fm-3
E0 = 0.0 Mev
K = 0.0 Mev
K' = 0.0 Mev
J = 0.0 Mev
L = 0.0 Mev
Ksym = 0.0 MeV

Neutron Star Properties

Mmax = 0.0 Msun
MDU,e = 0.0 Msun
RMmax = 0.0 km
R1.4 = 0.0 km

References

References to the original work:
[HSNP_2010]   M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
[TRKBP_2010]   S. Typel, G. Röpke, T. Klähn, D. Blaschke, and H.H. Wolter, Phys. Rev. C 81, 015803 (2010)
[BHB_2014]   S. Banik, M. Hempel, and D. Bandyopadhyay, Astrophys.J.Suppl. 214, 22 (2014)
[MNKA_1997]   P. Möller, J.R. Nix, and K.-L. Kratz, Atomic Data and Nuclear Data Tables 66, 131 (1997)

Data sheet

eos.pdf

Data

eos.zip (118.53 MB)
eos.zip_checksum.txt
Single files
eos.compo
eos.init
eos.micro
eos.nb
eos.t
eos.thermo
eos.yq
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