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JJ(VQCD(APR)), intermediate

Abstract

These EoSs (soft, intermediate, and stiff variants) are mostly based on gauge/gravity duality and include both nuclear and quark matter phases. They were selected as representative examples from a larger family of EoSs constructed in [JJNR_2021]. EoSs of this type were first considered in [ EJNS_2020]. They use the APR EoS [APRP_1989] for nuclear matter at low densities, and the holographic V-QCD model for dense nuclear matter [ IJN_2019] as well as for quark matter [JJR_2019]. To be precise, the EoSs are those considered in [JJNR_2021] with APR low density EoS, matching density of 1.6 times the saturation density, and V-QCD with potentials 5b, 7a, and 8b for the the soft, intermediate, and stiff variants, respectively.

Nparam = 1
Particles = npeNq
T min = 0.0
T max = 0.0
T pts = 1
nb min = 1.00e-12
nb max = 9.99e+00
nb pts = 651
Y min = 0.0
Y max = 0.0
Y pts = 1

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:
[APRP_1998]   A. Akmal, V. R. Pandharipande and D. G. Ravenhall, Phys. Rev. C 58, 1804 (1998)
[JJR_2019]   N. Jokela, M. Jarvinen and J. Remes, JHEP 03, 041 (2019)
[IJN_2019]   T. Ishii, M. Jarvinen and G. Nijs, JHEP 07, 003 (2019)
[EJNS_2020]   C. Ecker, M. Jarvinen, G. Nijs and W. van der Schee, Phys. Rev. D 101, 103006 (2020)
[JJNR_2021]   N. Jokela, M. Jarvinen, G. Nijs and J. Remes, Phys. Rev. D 103, 086004 (2021)

Data sheet

eos.pdf

Data

eos.zip (0.14 MB)
eos.zip_checksum.txt
Single files
eos.init
eos.nb
eos.t
eos.yq
eos.thermo
eos.mr
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