A Second Relativistic Mean Field and Virial Equation of State for Astrophysical Simulations - INSPIRE

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A Second Relativistic Mean Field and Virial Equation of State for Astrophysical Simulations

G. Shen
(
- Los Alamos and
- Indiana U., CEEM and
- Indiana U.
)
,
C.J. Horowitz
(
- Indiana U., CEEM and
- Indiana U.
)
,
E. O'Connor
(
- Caltech
)

Mar, 2011

16 pages

Published in:

Phys.Rev.C 83 (2011) 065808

e-Print:

1103.5174 [astro-ph.SR]

DOI:

10.1103/PhysRevC.83.065808

View in:

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Abstract: (arXiv)

We generate a second equation of state (EOS) of nuclear matter for a wide range of temperatures, densities, and proton fractions for use in supernovae, neutron star mergers, and black hole formation simulations. We employ full relativistic mean field (RMF) calculations for matter at intermediate density and high density, and the Virial expansion of a non-ideal gas for matter at low density. For this EOS we use the RMF effective interaction FSUGold, whereas our earlier EOS was based on the RMF effective interaction NL3. The FSUGold interaction has a lower pressure at high densities compared to the NL3 interaction. We calculate the resulting EOS at over 100,000 grid points in the temperature range

T

= 0 to 80 MeV, the density range

n_B

= 10

^{-8}

to 1.6 fm

^{-3}

, and the proton fraction range

Y_p

= 0 to 0.56. We then interpolate these data points using a suitable scheme to generate a thermodynamically consistent equation of state table on a finer grid. We discuss differences between this EOS, our NL3 based EOS, and previous EOSs by Lattimer-Swesty and H. Shen et al for the thermodynamic properties, composition, and neutron star structure. The original FSUGold interaction produces an EOS, that we call FSU1.7, that has a maximum neutron star mass of 1.7 solar masses. A modification in the high density EOS is introduced to increase the maximum neutron star mass to 2.1 solar masses and results in a slightly different EOS that we call FSU2.1. The EOS tables for FSU1.7 and FSU2.1 are available for download.

26.50.+x
21.65.Mn
26.60.Kp
21.60.Jz

References(38)

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[1]

A unified model of the magnetar and radio pulsar bursting phenomenology

Rosalba Perna
(
- JILA, Boulder
)
,
Jose A. Pons
(
- Alicante U.
)

- Astrophys.J.Lett. 727 (2011) L51
•
e-Print:
- 1101.1098
•
DOI:
- 10.1088/2041-8205/727/2/L51

[2]

Theory of Core-Collapse Supernovae

Hans-Thomas Janka
(
- Garching, Max Planck Inst.
)
,
K. Langanke
(
- Darmstadt, GSI and
- Darmstadt, Tech. Hochsch.
)
,
A. Marek
(
- Garching, Max Planck Inst.
)
,
G. Martinez-Pinedo
(
- Darmstadt, GSI
)
,
B. Mueller
(
- Garching, Max Planck Inst.
)

- Phys.Rept. 442 (2007) 38-74
•
e-Print:
- astro-ph/0612072
•
DOI:
- 10.1016/j.physrep.2007.02.002

[3]

Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole

Luca Baiotti
(
- Tokyo U., Komaba and
- Potsdam, Max Planck Inst.
)
,
Bruno Giacomazzo
(
- Potsdam, Max Planck Inst.
)
,
Luciano Rezzolla
(
- Potsdam, Max Planck Inst. and
- Louisiana State U. and
- INFN, Trieste
)

- Phys.Rev.D 78 (2008) 084033
•
e-Print:
- 0804.0594
•
DOI:
- 10.1103/PhysRevD.78.084033

[3]

Gravitational waves from nonspinning black hole-neutron star binaries: dependence on equations of state

Koutarou Kyutoku
(
- Kyoto U.
)
,
Masaru Shibata
(
- Kyoto U.
)
,
Keisuke Taniguchi
(
- New York U., Courant Inst. and
- Tokyo U.
)

- Phys.Rev.D 82 (2010) 044049,
- Phys.Rev.D 84 (2011) 049902 (erratum)
•
e-Print:
- 1008.1460
•
DOI:
- 10.1103/PhysRevD.82.044049

[3]

Equation of state effects in black hole-neutron star mergers

- Class.Quant.Grav. 27 (2010) 114106
•
e-Print:
- 0912.3528
•
DOI:
- 10.1088/0264-9381/27/11/114106

[4]

Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

LIGO Scientific and
VIRGO

Collaborations

•

J. Abadie
(
- LIGO Lab., Caltech
)

et al.

- Class.Quant.Grav. 27 (2010) 173001
•
e-Print:
- 1003.2480
•
DOI:
- 10.1088/0264-9381/27/17/173001

[5]

A Generalized equation of state for hot, dense matter

- Nucl.Phys.A 535 (1991) 331-376
•
DOI:
- 10.1016/0375-9474(91)90452-C

[6]

Relativistic equation of state of nuclear matter for supernova and neutron star

H. Shen
(
- Osaka U., Res. Ctr. Nucl. Phys. and
- Nankai U.
)
,
H. Toki
(
- Osaka U., Res. Ctr. Nucl. Phys. and
- Wako, RIKEN
)
,
K. Oyamatsu
(
- Wako, RIKEN and
- Nagoya U.
)
,
K. Sumiyoshi
(
- Wako, RIKEN
)

- Nucl.Phys.A 637 (1998) 435-450
•
e-Print:
- nucl-th/9805035
•
DOI:
- 10.1016/S0375-9474(98)00236-X

[7]

Relativistic equation of state of nuclear matter for supernova explosion

H. Shen
(
- Osaka U., Res. Ctr. Nucl. Phys. and
- Nankai U.
)
,
H. Toki
(
- Osaka U., Res. Ctr. Nucl. Phys. and
- Wako, RIKEN
)
,
K. Oyamatsu
(
- Wako, RIKEN and
- Nagoya U.
)
,
K. Sumiyoshi
(
- Wako, RIKEN
)

- Prog.Theor.Phys. 100 (1998) 1013
•
e-Print:
- nucl-th/9806095
•
DOI:
- 10.1143/PTP.100.1013

[8]

Statistical Model for a Complete Supernova Equation of State

- Nucl.Phys.A 837 (2010) 210-254
•
e-Print:
- 0911.4073
•
DOI:
- 10.1016/j.nuclphysa.2010.02.010

[9]

Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae

Chikako Ishizuka
(
- Hokkaido U.
)
,
Akira Ohnishi
(
- Hokkaido U.
)
,
Kohsuke Tsubakihara
(
- Hokkaido U.
)
,
Kohsuke Sumiyoshi
(
- Numazu Coll. Tech.
)
,
Shoichi Yamada
(
- Waseda U., RISE
)

- J.Phys.G 35 (2008) 085201
•
e-Print:
- 0802.2318
•
DOI:
- 10.1088/0954-3899/35/8/085201

[10]

EOS of hyperonic matter for core-collapse supernovae

A. Ohnishi
(
- Kyoto U., Yukawa Inst., Kyoto
)
,
K. Tsubakihara
(
- Hokkaido U.
)
,
K. Sumiyoshi
(
- Numazu Coll. Tech.
)
,
C. Ishizuka
(
- Keele U.
)
,
S. Yamada
(
- Waseda U., RISE
)

et al.

- Nucl.Phys.A 835 (2010) 374-377
•
DOI:
- 10.1016/j.nuclphysa.2010.01.222

[11]

Shell States of Neutron Rich Matter

C.J. Horowitz
(
- Indiana U.
)
,
G. Shen
(
- Indiana U.
)

- Phys.Rev.C 78 (2008) 015801
•
e-Print:
- 0805.2774
•
DOI:
- 10.1103/PhysRevC.78.015801

[12]

Equation of State of Dense Matter from a density dependent relativistic mean field model

- Phys.Rev.C 82 (2010) 015806
•
e-Print:
- 1004.0228
•
DOI:
- 10.1103/PhysRevC.82.015806

[13]

Equation of State of nuclear matter in a Virial expansion of nucleons and nuclei

- Phys.Rev.C 82 (2010) 045802
•
e-Print:
- 1006.0489
•
DOI:
- 10.1103/PhysRevC.82.045802

[14]

A New Equation of State for Astrophysical Simulations

- Phys.Rev.C 83 (2011) 035802
•
e-Print:
- 1101.3715
•
DOI:
- 10.1103/PhysRevC.83.035802

[15]

A New parametrization for the Lagrangian density of relativistic mean field theory

G.A. Lalazissis
(
- Munich, Tech. U. and
- Thessaloniki U.
)
,
J. Konig
(
- Munich, Tech. U.
)
,
P. Ring
(
- Munich, Tech. U.
)

- Phys.Rev.C 55 (1997) 540-543
•
e-Print:
- nucl-th/9607039
•
DOI:
- 10.1103/PhysRevC.55.540

[16]

The Virial equation of state of low-density neutron matter

C.J. Horowitz
(
- Indiana U.
)
,
A. Schwenk
(
- Indiana U.
)

- Phys.Lett.B 638 (2006) 153-159
•
e-Print:
- nucl-th/0507064
•
DOI:
- 10.1016/j.physletb.2006.05.055

[17]

Cluster formation and the virial equation of state of low-density nuclear matter

C.J. Horowitz
(
- Indiana U.
)
,
A. Schwenk
(
- Indiana U.
)

- Nucl.Phys.A 776 (2006) 55-79
•
e-Print:
- nucl-th/0507033
•
DOI:
- 10.1016/j.nuclphysa.2006.05.009

[18]

Neutrino Scattering in Heterogeneous Supernova Plasmas

- Phys.Rev.C 74 (2006) 065801
•
e-Print:
- astro-ph/0607564
•
DOI:
- 10.1103/PhysRevC.74.065801

[19]

Neutrino trapping in a supernova and ion screening

C.J. Horowitz
(
- Bonn U. and
- Indiana U.
)

- Phys.Rev.D 55 (1997) 4577-4581
•
e-Print:
- astro-ph/9603138
•
DOI:
- 10.1103/PhysRevD.55.4577

[20]

Neutron-Rich Nuclei and Neutron Stars: A New Accurately Calibrated Interaction for the Study of Neutron-Rich Matter

B.G. Todd-Rutel
(
- Florida State U.
)
,
J. Piekarewicz
(
- Florida State U.
)

- Phys.Rev.Lett. 95 (2005) 122501
•
e-Print:
- nucl-th/0504034
•
DOI:
- 10.1103/PhysRevLett.95.122501

[21]

Validating relativistic models of nuclear structure against theoretical, experimental, and observational constraints

J. Piekarewicz
(
- Florida State U.
)

- Phys.Rev.C 76 (2007) 064310
•
e-Print:
- 0709.2699
•
DOI:
- 10.1103/PhysRevC.76.064310

[22]

Shapiro Delay Measurement of A Two Solar Mass Neutron Star

Paul Demorest
(
- NRAO, Charlottesville
)
,
Tim Pennucci
(
- Virginia U., Astron. Dept.
)
,
Scott Ransom
(
- NRAO, Charlottesville
)
,
Mallory Roberts
(
- Eureka Sci.
)
,
Jason Hessels
(
- ASTRON, Dwingeloo and
- Amsterdam U., Astron. Inst.
)

- Nature 467 (2010) 1081-1083
•
e-Print:
- 1010.5788
•
DOI:
- 10.1038/nature09466

[23]

Relativistic effective interaction for nuclei, giant resonances, and neutron stars

- Phys.Rev.C 82 (2010) 055803
•
e-Print:
- 1008.3030
•
DOI:
- 10.1103/PhysRevC.82.055803

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