Abstract.
Microscopically, the equation of state (EOS) and other properties of asymmetric nuclear matter at zero temperature have been investigated extensively by adopting the non-relativistic Brueckner-Hartree-Fock (BHF) and the extended BHF approaches by using the self-consistent Green’s function approach or by including a phenomenological three-body force. Once three-body forces are introduced, the phenomenological saturation point is reproduced and the theory is applied to the study of neutron star properties. We can calculate the total mass and radius for neutron stars using various equations of state at high densities in \( \beta\)-equilibrium without hyperons. A comparison with other microscopic predictions based on non-relativistic and density-dependent relativistic mean-field calculations has been done. It is found that relativistic EOS yields however larger mass and radius for neutron star than predictions based on non-relativistic approaches. Also the three-body force plays a crucial role to deduce the theoretical value of the maximum mass of neutron stars in agreement with recent measurements of the neutron star mass.
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References
F. Weber, N.K. Glendenning, M.K. Weigel, Astrophys. J. 373, 579 (1991)
C.P. Lorenz, D.G. Ravenhall, C.J. Pethick, Phys. Rev. Lett. 70, 379 (1993)
C.J. Pethick, D.G. Ravenhall, C.P. Lorenz, Nucl. Phys. A 584, 675 (1995)
Bao-An Li, Lie-Wen Chen, Che Ming Ko, Phys. Rep. 464, 113 (2008)
G. Bao, L. Engvik, M. Hjorth-Jensen, E. Osnes, E. Ostgaard, Nucl. Phys. A 575, 707 (1994)
A.W. Steiner, M. Hempel, T. Fischer, Astrophys. J. 774, 17 (2013)
T. Fischer, M. Hempel, I. Sagert, Y. Suwa, J. Schaffner-Bielich, Eur. Phys. J. A 50, 46 (2014)
S.E. Thorsett, Z. Arzoumanian, M.M. McKinnon, J.H. Taylor, Astrophys. J. 405, L29 (1993)
J. Oppenheimer, G. Volkoff, Phys. Rev. 55, 374 (1939)
R.C. Tolman, Proc. Natl. Acad. Sci. U.S.A. 20, 3 (1934)
E. Witten, Phys. Rev. D 30, 272 (1984)
C. Alcock, E. Farhi, A.V. Olinto, Astrophys. J. 310, 261 (1986)
G.E. Brown, C.H. Lee, M. Rho, V. Thorsson, Nucl. Phys. A 567, 937 (1994)
A.B. Migdal, E.E. Saperstein, M.A. Troitsky, D.N. Voskresensky, Phys. Rep. 192, 179 (1990)
M. Baldo, G.F. Burgio, H.-J. Schulze, Phys. Rev. C 58, 3688 (1998)
M. Baldo, Nuclear Methods and the Nuclear Equation of State, International Review of Nuclear Physics (World Scientific, 1999)
M. Baldo, G.F. Burgio, H.-J. Schulze, Phys. Rev. C 61, 55801 (2000)
R. Machleidt, Adv. Nucl. Phys. 19, 189 (1989)
L. Engvik, M. Hjorth-Jensen, E. Osnes, G. Bao, E. Ostgaard, Phys. Rev. Lett. 73, 2650 (1994)
E.N.E. van Dalen, C. Fuchs, A. Faessler, Eur. Phys. J. A 31, 29 (2007)
Bao Yuan Sun, Wen Hui Long, Jie Meng, U. Lombardo, Phys. Rev. C 78, 065805 (2008)
P. Gögelein, E.N.E. van Dalen, Kh. Gad, Kh.S.A. Hassaneen, H. Müther, Phys. Rev. C 79, 024308 (2009)
P.B. Demorest, T. Pennucci, S.M. Ransom, M.S.E. Roberts, J.W.T. Hessels, Nature 467, 1081 (2010)
J. Antoniadis et al., Science 340, 6131 (2013)
E. Fonseca, arXiv:1603.00545 (2016)
B.D. Serot, J.D. Walecka, Adv. Nucl. Phys. 16, 1 (1986)
S.F. Ban, J. Li, S.Q. Zhang, H.Y. Jia, J.P. Sang, J. Meng, Phys. Rev. C 69, 045805 (2004)
S. Lawley, W. Bentz, A.W. Thomas, Nucl. Phys. Proc. Suppl. 141, 29 (2005)
J.R. Stone, J.C. Miller, R. Koncewicz, P.D. Stevenson, M.R. Strayer, Phys. Rev. C 68, 034324 (2003)
M. Dutra, O. Lourenço, J.S. Sá Martins, A. Delfino, J.R. Stone, P.D. Stevenson, Phys. Rev. C 85, 035201 (2012)
P.D. Stevenson, P.M. Goddard, J.R. Stone, M. Dutra, AIP Conf. Proc. 1529, 262 (2013)
R. Machleidt, F. Sammarruca, Y. Song, Phys. Rev. C 53, R1483 (1996)
R. Machleidt, Phys. Rev. C 63, 024001 (2001)
T. Frick, Kh. Gad, H. Müther, P. Czerski, Phys. Rev. C 65, 034321 (2002)
T. Frick, Kh.S.A. Hassaneen, D. Rohe, H. Müther, Phys. Rev. C 70, 024309 (2004)
Kh.S.A. Hassaneen, H. Müther, Phys. Rev. C 70, 054308 (2004)
M. Baldo, A. Shaban, Phys. Lett. B 661, 373 (2008)
Kh. Gad, Kh.S.A. Hassaneen, Nucl. Phys. A 793, 67 (2007)
Kh.S.A. Hassaneen, Kh. Gad, J. Phys. Soc. Jpn. 77, 084201 (2008)
H. Mansour, Kh. Gad, Kh.S.A. Hassaneen, Prog. Theor. Phys. 123, 687 (2010)
M. Baldo, I. Bombaci, G.F. Burgio, Astron. Astrophys. 328, 274 (1997)
E. Khan, J. Margueron, arXiv:1304.4721v1 (2013)
J.R. Stone, N.J. Stone, S.A. Moszkowski, Phys. Rev. C 89, 044316 (2014)
H. Müther, A. Polls, Prog. Part. Nucl. Phys. 45, 243 (2000)
J.P. Jeukenne, A. Lejeunne, C. Mahaux, Phys. Rep. 25, 83 (1976)
Kh.S.A. Hassaneen, H.M. Abo-Elsebaa, E.A. Sultan, H.M.M. Mansour, Ann. Phys. 326, 566 (2011)
H.M.M. Mansour, Kh.S.A. Hassaneen, Phys. At. Nucl. 77, 290 (2014)
E. Schiller, H. Müther, P. Czerski, Phys. Rev. C 59, 2934 (1999) 60
P. Grangé, J. Cugnon, A. Lejeune, Nucl. Phys. A 473, 365 (1987)
D.S. Koltun, Phys. Rev. C 9, 484 (1974)
I. Bombaci, U. Lombardo, Phys. Rev. C 44, 1892 (1991)
P.G. Krastev, F. Sammarruca, Phys. Rev. C 74, 025808 (2006)
P.E. Haustein, At. Data Nucl. Data Tables 39, 185 (1988)
A.W. Steiner, J.M. Lattimer, E.F. Brown, Eur. Phys. J. A 52, 18 (2016)
A. Rios, A. Polls, I. Vidaña, Phys. Rev. C 79, 025802 (2009)
R.B. Wiringa, V.G.J. Stoks, R. Schiavilla, Phys. Rev. C 51, 38 (1995)
J. Carlson, V.R. Pandharipande, R.B. Wiringa, Nucl. Phys. A 401, 59 (1983)
Private communication with Professor M. Baldo
P. Bonche, D. Vautherin, Nucl Phys. A 372, 496 (1981)
E.N.E. van Dalen, P. Gögelein, H. Müther, Phys. Rev. C 80, 044312 (2009)
J.M. Lattimer, B.F. Schutz, Astrophys. J. 629, 979 (2005)
D. Blaschke, D. E. Alvarez-Castillo, T. Klähn, arXiv:1604.08575 [nucl-th]
J.M. Lattimer, Y. Lim, Astrophys. J. 771, 51 (2013)
J.M. Lattimer, C.J. Pethick, M. Prakash, P. Haensel, Phys. Rev. Lett. 66, 2701 (1991)
P. Danielewicz, R. Lacey, W.G. Lynch, Science 298, 1592 (2002)
M. Prakash, T.L. Ainsworth, J.M. Lattimer, Phys. Rev. Lett. 61, 2518 (1988)
Xuejun Wu, H. Müther, M. Soffel, H. Herold, H. Ruder, Astron. Astrophys. 246, 411 (1991)
F. Hofmann, C.M. Keil, H. Lenske, Phys. Rev. C 64, 025804 (2001)
Z.H. Li, H.J. Schulze, Phys. Rev. C 78, 028801 (2008)
Ch.C. Moustakidis, Phys. Rev. C 91, 035804 (2015)
S. Gandolfi, A. Gezerlis, J. Carlson, Annu. Rev. Nucl. Part. Sci 65, 303 (2015)
G. Baym, C. Pethick, D. Sutherland, Astrophys. J. 170, 299 (1971)
J.W. Negele, D. Vautherin, Nucl. Phys. A 207, 298 (1973)
T. Güver, F. Özel, Astrophys. J. 765, L1 (2013)
B.K. Sharma, M. Centelles, X. Vinas, M. Baldo, G.F. Burgio, Astron. Astrophys. 584, A103 (2015)
M. Dutra, O. Lourenço, D.P. Menezes, Phys. Rev. C 93, 025806 (2016) 94
M. Dutra, O. Lourenço, S.S. Avancini, B.V. Carlson, A. Delfino, D.P. Menezes, C. Providencia, S. Typel, J.R. Stone, Phys. Rev. C 90, 055203 (2014)
L. Engvik, E. Osnes, M. Hjorth-Jensen, G. Bao, E. Ostgaard, Astrophys. J. 469, 794 (1996)
W. Zuo, I. Bombaci, U. Lombardo, Eur. Phys. J. A 50, 12 (2014)
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Hassaneen, K.S.A. Asymmetric nuclear matter and neutron star properties within the extended Brueckner theory. Eur. Phys. J. A 53, 9 (2017). https://doi.org/10.1140/epja/i2017-12196-6
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DOI: https://doi.org/10.1140/epja/i2017-12196-6