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FYSS (with electrons)

Abstract

In the present equation of state, the relativistic mean field theory with the TM1 parameter set for nucleons has been adopted, the quantum approach for d, t, h and alpha, as well as the liquid drop model for the other nuclei under the assumption of nuclear statistical equilibrium. Temperature dependences of surface and shell energies of heavy nuclei have been taken into account as well as the possibility of pasta phases for heavy nuclei and the Pauli- and self-energy shifts for d, t, h and alpha. Further details can be found in Refs.~[ FYSS_2011, FYSS_2013, FYSS_2017 ]. For the present version of the table contributions from leptons and photons have been added to the original table.

Nparam = 3
Particles = npe N
T min = 1.00e-01
T max = 3.98e+02
T pts = 91
nb min = 9.55e-11
nb max = 6.02e+00
nb pts = 109
Y min = 1.00e-02
Y max = 6.50e-01
Y pts = 65

References

References to the original work:
[FYSS_2017]   Shun Furusawa, Kohsuke Sumiyoshi, Shoichi Yamada, Hideyuki Suzuki., Nucl. Phys. A 957, 188. (2017)
[FYSS_2013]   S. Furusawa, K. Sumiyoshi, S. Yamada, and H. Suzuki, Astrophys. J. 772,95 (2013)
[FYSS_2011]   S. Furusawa, S. Yamada, K. Sumiyoshi, and H. Suzuki, Astrophys. J 738,178 (2011)

Data sheet

Data

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

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