Excluded-volume model for quarkyonic Matter: Three-flavor baryon-quark Mixture

Duarte, Dyana C.; Hernandez-Ortiz, Saul; Jeong, Kie Sang

doi:10.1103/PhysRevC.102.025203

Excluded-volume model for quarkyonic Matter: Three-flavor baryon-quark Mixture

Mar 4, 2020

9 pages

Published in:

Phys.Rev.C 102 (2020) 2, 025203

Published: Aug 13, 2020

e-Print:

2003.02362 [nucl-th]

DOI:

10.1103/PhysRevC.102.025203 (publication)

Report number:

INT-PUB-20-001

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Abstract: (APS)

The single-flavor excluded-volume model based on the effective size of baryons reproduces the hard-soft density evolution of the equation of state (EoS) required by the recent studies of GW170817. This phenomenological model basically realizes the concept of quarkyonic matter which is introduced from large-Nc gauge theory for dense matter. Enhanced nucleon interactions and dynamically generated quark degrees of freedom can reproduce the hard-soft evolution of the EoS. In this paper, we extend the excluded-volume model to a three-flavor system by considering electromagnetic charge and possible weak equilibrium in order to obtain a proper description for the hard-soft behavior of the EoS inferred from the gravitational waves observations.

Note:

11 pages, 6 figures, tex command fixed

Hadronic Physics and QCD
flavor: 3
nucleon: interaction
baryon: size
gravitational radiation
gravitational radiation: emission
gauge field theory
equation of state
electromagnetic field: production
quark

References(63)

Figures(9)

[1]

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

LIGO Scientific and
Virgo

Collaborations

•

B.P. Abbott
(
- LIGO Lab., Caltech
)

et al.

- Phys.Rev.Lett. 119 (2017) 16, 161101
•
e-Print:
- 1710.05832
•
DOI:
- 10.1103/PhysRevLett.119.161101

[2]

GW170817: Measurements of neutron star radii and equation of state

LIGO Scientific and
Virgo

Collaborations

•

B.P. Abbott
(
- LIGO Lab., Caltech
)

et al.

- Phys.Rev.Lett. 121 (2018) 16, 161101
•
e-Print:
- 1805.11581
•
DOI:
- 10.1103/PhysRevLett.121.161101

[3]

Neutron Skins and Neutron Stars in the Multimessenger Era

- Phys.Rev.Lett. 120 (2018) 17, 172702
•
e-Print:
- 1711.06615
•
DOI:
- 10.1103/PhysRevLett.120.172702

[4]

Gravitational-wave constraints on the neutron-star-matter Equation of State

Eemeli Annala
(
- Helsinki U. and
- Helsinki Inst. of Phys.
)
,
Tyler Gorda
(
- Helsinki U. and
- Helsinki Inst. of Phys.
)
,
Aleksi Kurkela
(
- CERN and
- Stavanger U.
)
,
Aleksi Vuorinen
(
- Helsinki U. and
- Helsinki Inst. of Phys.
)

- Phys.Rev.Lett. 120 (2018) 17, 172703
•
e-Print:
- 1711.02644
•
DOI:
- 10.1103/PhysRevLett.120.172703

[5]

Neutron stars and stellar mergers as a laboratory for dense QCD matter

Aleksi Vuorinen
(
- Helsinki Inst. of Phys.
)

- Nucl.Phys.A 982 (2019) 36-42
•
e-Print:
- 1807.04480
•
DOI:
- 10.1016/j.nuclphysa.2018.10.011

[6]

Tidal deformability from GW170817 as a direct probe of the neutron star radius

- Astrophys.J.Lett. 857 (2018) 2, L23
•
e-Print:
- 1803.07687
•
DOI:
- 10.3847/2041-8213/aabcbf

[7]

New constraints on radii and tidal deformabilities of neutron stars from GW170817

Elias R. Most
(
- Frankfurt U.
)
,
Lukas R. Weih
(
- Frankfurt U.
)
,
Luciano Rezzolla
(
- Frankfurt U. and
- Frankfurt U., FIAS
)
,
Jürgen Schaffner-Bielich
(
- Frankfurt U.
)

- Phys.Rev.Lett. 120 (2018) 26, 261103
•
e-Print:
- 1803.00549
•
DOI:
- 10.1103/PhysRevLett.120.261103

[8]

Confronting gravitational-wave observations with modern nuclear physics constraints

I. Tews
(
- Los Alamos
)
,
J. Margueron
(
- Lyon, IPN
)
,
S. Reddy
(
- Washington U., Seattle and
- Michigan State U., JINA
)

- Eur.Phys.J.A 55 (2019) 6, 97
•
e-Print:
- 1901.09874
•
DOI:
- 10.1140/epja/i2019-12774-6

[9]

Xiamen-Custipen Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy, 3–7 January 2019, Xiamen, China

A. Li
,
B.-A. Li
,
F. Xu
,
I. Tews
,
J. Margueron

et al.

[10]

Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory

Collin D. Capano
(
- Hannover, Max Planck Inst. Grav. and
- Leibniz U., Hannover
)
,
Ingo Tews
(
- Los Alamos Natl. Lab., Theor. Div.
)
,
Stephanie M. Brown
(
- Hannover, Max Planck Inst. Grav. and
- Leibniz U., Hannover
)
,
Ben Margalit
(
- UC, Berkeley, Astron. Dept. and
- Santa Barbara, KITP
)
,
Soumi De
(
- Santa Barbara, KITP and
- Syracuse U. (main)
)

et al.

- Nature Astron. 4 (2020) 6, 625-632
•
e-Print:
- 1908.10352
•
DOI:
- 10.1038/s41550-020-1014-6

[11]

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

[12]

A Massive Pulsar in a Compact Relativistic Binary

et al.

- Science 340 (2013) 6131
•
e-Print:
- 1304.6875
•
DOI:
- 10.1126/science.1233232

[13]

Neutron Stars Are Giant Hypernuclei?

N.K. Glendenning
(
- LBL, Berkeley
)

- Astrophys.J. 293 (1985) 470-493,
- Lawrence Berkeley Lab. - LBL-15976 (84,REC.JUL.) 48p
•
DOI:
- 10.1086/163253

[14]

Strangeness in hadronic stellar matter

- Phys.Rev.C 52 (1995) 3470-3482,
- Phys. Rev. C52 (1995) 3470-3482, and State U. New York Stony Brook - NTG-95-15 (95/06,rec.Jul.) 43 p. Minnesota U. Minneapolis - NUC-MINN-95-13-T (95/06,rec.Jul.) 43 p
•
e-Print:
- nucl-th/9506016
•
DOI:
- 10.1103/PhysRevC.52.3470