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KRT(FSU2H*)

DOI

Abstract

This is the EOS table of homogenous hadronic and leptonic matter which is based on the RMF interaction FSU2H as defined in Ref. [TCR_2017,PFPR_2019] with updated hyperonic coupling constants and extended to finite temperatures as in Ref. [KRT_2022]

Nparam = 3
Particles = npeBs
T min = 1.00e-01
T max = 9.99e+01
T pts = 11
nb min = 5.00e-02
nb max = 9.99e-01
nb pts = 50
Y min = 1.00e-02
Y max = 4.99e-01
Y pts = 50

Nuclear Matter Properties

ns = 0.1505 fm-3
E0 = 16.28 Mev
K = 238.0 Mev
K' = 24.6 Mev
J = 30.5 Mev
L = 44.5 Mev
Ksym = 87.0 MeV

Neutron Star Properties

Mmax = 2.02 Msun
MDU,e = N/A Msun
RMmax = 12.0 km
R1.4 = 13.3 km

References

References to the original work:
[PFPR_2019]   C. Providência, M. Fortin, H. Pais, and A. Rabhi, Astron. Space Sci. 6, 13 (2019)
[KRT_2022]   Hristijan Kochankovski, Angels Ramos, Laura Tolos, MNRAS 517, 507 (2022)
[TCR_2017]   Laura Tolos, Mario Centelles, Angels Ramos, Astrophys. J 834,1 (2017)

Data sheet

eos.pdf

Data

eos.zip (8.55 MB)
eos.zip_checksum.txt
Single files
eos.compo
eos.init
eos.nb
eos.t
eos.yq
eos.thermo
eos.micro
eos.thermo.ns
eos.nb.ns
eos.mr
12.012.513.013.514.014.515.015.516.00.20.40.60.81.01.21.41.61.82.02.2radius (km)radiusmass (M_sun)massMass radius relation of a cold spherically symmetric neutron starPSR J1614-2230PSR J0348+0432
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The EoS "KRT(FSU2H*)" has not eos.init file associated so computation is not possible.

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