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BL_EOS with crust

Abstract

Microscopic equation of state (EoS) of dense beta-stable nuclear matter at zero temperature (T=0) obtained using realistic two-body and three-body nuclear interactions derived in the framework of chiral perturbation theory (ChPT) and including the Delta(1232) isobar intermediate state. This EoS has been derived using the Brueckner-Bethe-Goldstone quantum many-body theory in the Brueckner-Hartree-Fock approximation with the continuous choice for the auxiliary single particle potential. The present table is relative to the nuclear interaction model denoted as N3LODelta+N2LODelta in [BL_2018]. It contains the contributions from electrons and muons in addition to beta-stable nuclear matter. Below a density of n_B = 0.08 fm^(-3), the crust EoS from Douchin and Haensel [DHA_2001] has been added.

Nparam = 1
Particles = npem
T min = 0.0
T max = 0.0
T pts = 1
nb min = 7.93e-15
nb max = 1.29e+00
nb pts = 283
Y min = 0.0
Y max = 0.0
Y pts = 1

References

References to the original work:
[DHA_2001]   F. Douchin, P. Haensel, Astronomy and Astrophysics 380, 151 (2001)
[BL_2018]   I. Bombaci and D. Logoteta, Astron. and Astrophys. 609, A128 (2018)

Data sheet

Data

eos.zip (contains all following files and data sheet)
eos.compo
eos.init
eos.mr
eos.nb
eos.t
eos.thermo
eos.yq
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The EoS "BL_EOS with crust" has not eos.init file associated so computation is not possible.

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