Hybrid stars within the framework of the Sigma-Omega-Rho model combined with the MIT and NJL models

Nuclear Physics A - Tập 1037 - Trang 122684 - 2023
Reza Karimi1, H.R. Moshfegh1
1Department of Physics, University of Tehran, Post Office Box 14395-547, Tehran, Iran

Tài liệu tham khảo

Kochankovski Lattimer, 2007, Neutron star observations: prognosis for equation of state constraints, Phys. Rep., 442, 109, 10.1016/j.physrep.2007.02.003 Klähn, 2006, Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions, Phys. Rev. C, 74, 10.1103/PhysRevC.74.035802 Oertel, 2017, Equations of state for supernovae and compact stars, Rev. Mod. Phys., 89, 10.1103/RevModPhys.89.015007 Lattimer, 2013, Constraining the symmetry parameters of the nuclear interaction, Astrophys. J., 771, 51, 10.1088/0004-637X/771/1/51 Romani, 2022, Psr j0952-0607: the fastest and heaviest known galactic neutron star, Astrophys. J. Lett., 934, L18, 10.3847/2041-8213/ac8007 Fonseca, 2021, Refined mass and geometric measurements of the high-mass psr j0740+ 6620, Astrophys. J. Lett., 915, L12, 10.3847/2041-8213/ac03b8 Annala, 2020, Evidence for quark-matter cores in massive neutron stars, Nat. Phys., 16, 907, 10.1038/s41567-020-0914-9 Shuryak, 1980, Quantum chromodynamics and the theory of superdense matter, Phys. Rep., 61, 71, 10.1016/0370-1573(80)90105-2 Tafrihi, 2016, Comparative study of the locv and the fhnc approaches for the nucleonic matter problem, J. Phys. Conf. Ser., 702, 012015, 10.1088/1742-6596/702/1/012015 Owen, 1975, Constrained Jastrow calculations, Phys. Lett. B, 59, 1, 10.1016/0370-2693(75)90139-2 Khanmohamadi, 2020, Hybrid star within the framework of a lowest-order constraint variational method, Phys. Rev. D, 101, 10.1103/PhysRevD.101.023004 Burgio, 2016, Hybrid star structure with the field correlator method, Eur. Phys. J. A, 52, 1, 10.1140/epja/i2016-16060-y Ju, 2021, Hadron-quark mixed phase in the quark-meson coupling model, Phys. Rev. C, 103, 10.1103/PhysRevC.103.025809 Guichon, 1988, A possible quark mechanism for the saturation of nuclear matter, Phys. Lett. B, 200, 235, 10.1016/0370-2693(88)90762-9 Sugahara, 1994, Relativistic mean-field theory for unstable nuclei with non-linear σ and ω terms, Nucl. Phys. A, 579, 557, 10.1016/0375-9474(94)90923-7 Fattoyev, 2010, Relativistic effective interaction for nuclei, giant resonances, and neutron stars, Phys. Rev. C, 82, 10.1103/PhysRevC.82.055803 Karimi, 2022, Baryons’ coupling constants in the sigma–omega–rho model and the mass–radius relation of neutron stars in the presence of hyperons, Ann. Phys., 436, 10.1016/j.aop.2021.168665 Fowler, 1981, Confinement and phase transitions, Z. Phys. C, Part. Fields, 9, 271, 10.1007/BF01410668 Simonov, 2019, Field correlator method for the confinement in qcd, Phys. Rev. D, 99, 10.1103/PhysRevD.99.056012 Chodos, 1974, New extended model of hadrons, Phys. Rev. D, 9, 3471, 10.1103/PhysRevD.9.3471 Farhi, 1984, Strange matter, Phys. Rev. D, 30, 2379, 10.1103/PhysRevD.30.2379 Klähn, 2015, Vector interaction enhanced bag model for astrophysical applications, Astrophys. J., 810, 134, 10.1088/0004-637X/810/2/134 Buballa, 2005, Njl-model analysis of dense quark matter, Phys. Rep., 407, 205, 10.1016/j.physrep.2004.11.004 Hatsuda, 1994, Qcd phenomenology based on a chiral effective Lagrangian, Phys. Rep., 247, 221, 10.1016/0370-1573(94)90022-1 Benić, 2015, A new quark-hadron hybrid equation of state for astrophysics-I. High-mass twin compact stars, Astron. Astrophys., 577, A40, 10.1051/0004-6361/201425318 Christian, 2018, Classifications of twin star solutions for a constant speed of sound parameterized equation of state, Eur. Phys. J. A, 54, 1, 10.1140/epja/i2018-12472-y Han, 2019, Tidal deformability with sharp phase transitions in binary neutron stars, Phys. Rev. D, 99, 10.1103/PhysRevD.99.083014 Paschalidis, 2018, Implications from gw170817 and i-love-q relations for relativistic hybrid stars, Phys. Rev. D, 97, 10.1103/PhysRevD.97.084038 Alvarez-Castillo, 2019, Third family of compact stars within a nonlocal chiral quark model equation of state, Phys. Rev. D, 99, 10.1103/PhysRevD.99.063010 Macher, 2005, Phase transitions in compact stars, Eur. J. Phys., 26, 341, 10.1088/0143-0807/26/3/003 Nandi, 2018, Hybrid stars in the light of gw170817, Astrophys. J., 857, 12, 10.3847/1538-4357/aab78c Glendenning, 1984 Glendenning, 2012 Baym, 1971, The ground state of matter at high densities: equation of state and stellar models, Astrophys. J., 170, 299, 10.1086/151216 Maieron, 2004, Hybrid stars with the color dielectric and the MIT bag models, Phys. Rev. D, 70, 10.1103/PhysRevD.70.043010 Aziz, 2019, Constraining values of bag constant for strange star candidates, Int. J. Mod. Phys. D, 28, 10.1142/S0218271819410062 Rehberg, 1996, Hadronization in the SU(3) Nambu–Jona-Lasinio model, Phys. Rev. C, 53, 410, 10.1103/PhysRevC.53.410 Buballa, 2005, Njl-model analysis of dense quark matter, Phys. Rep., 407, 205, 10.1016/j.physrep.2004.11.004 Hatsuda, 1994, Qcd phenomenology based on a chiral effective Lagrangian, Phys. Rep., 247, 221, 10.1016/0370-1573(94)90022-1 Lutz, 1992, Meson properties at finite temperature and baryon density, Nucl. Phys. A, 542, 521, 10.1016/0375-9474(92)90256-J Hagiwara, 2002, Review of particle physics, Phys. Rev. D, Part. Fields, 66, 10.1103/PhysRevD.66.010001 Sen, 2022, Rotating hybrid stars with color-flavor-locked quark matter, J. Phys. G, Nucl. Part. Phys., 10.1088/1361-6471/ac6f14 Glendenning, 1992, First-order phase transitions with more than one conserved charge: consequences for neutron stars, Phys. Rev. D, 46, 1274, 10.1103/PhysRevD.46.1274 Wu, 2019, Nuclear symmetry energy and hadron-quark mixed phase in neutron stars, Phys. Rev. C, 99, 10.1103/PhysRevC.99.065802 Yasutake, 2011, Hadron-quark phase transitions in hyperon stars, Phys. At. Nucl., 74, 1502, 10.1134/S1063778811100073 Oppenheimer, 1939, On massive neutron cores, Phys. Rev., 55, 374, 10.1103/PhysRev.55.374 Burgio, 2002, Maximum mass of neutron stars with a quark core, Phys. Lett. B, 526, 19, 10.1016/S0370-2693(01)01479-4 Li, 2018, Studies of the structure of massive hybrid stars within a modified njl model, Phys. Rev. D, 97, 10.1103/PhysRevD.97.103013 Bombaci, 1996, The maximum mass of a neutron star, Astron. Astrophys., 305, 871