Key factor for determining relation between radius and tidal deformability of neutron stars: Slope of symmetry energy

[1]
P. B. Demorest, T. Pennucci, S. M. Ransom et al., Nature, 467: 1081 (2010)
[2]
Z. Arzoumanian et al., Astrophys. J. Supp., 235: 37 (2018)
[3]
J. Antoniadis et al., Science, 340: 448 (2013)
[4]
H. T. Cromartie et al., Nature Astronomy, (2019)
[5]
N. B. Zhang and B. A. Li, Astrophys. J., 879: 99 (2019)
[6]
S. Campana and L. Stella, Nucl. Phys. B Proc. Suppl., 132: 427 (2004)
[7]
C. O. Heinke, PhD thesis, Harvard University
[8]
S. Mereghetti, Astrophys. Space Sci. Proc., 21: 345 (2011)
[9]
S. Guillot, M. Servillat, N. A. Webb et al., Astrophys. J., 772: 7 (2013)
[10]
A. W. Steiner, J. M. Lattimer, and E. F. Brown, Astrophys. J. Lett., 765: 5 (2013)
[11]
S. Guillot and R. E. Rutledge, Astrophys. J. Lett., 796: 3 (2014)
[12]
J. M. Lattimer and A. W. Steiner, Eur. Phys. J. A, 50: 40 (2014)
[13]
S. Bogdanov, C. O. Heinke, F. Özel et al., Astrophys. J., 831: 184 (2016)
[14]
Guillot S’ s talk in Nusym2016
[15]
F. Özel, D. Psaltis, T. Güver et al., Astrophys. J., 820: 28 (2016)
[16]
J. Nättilä, M. C. Miller, A. W. Steiner et al., A&A, 608: A31 (2017)
[17]
A. W. Shaw et al., Mon. Not. R. Astron. Soc., 476: 4713 (2018)
[18]
A. W. Steiner et al., Mon. Not. R. Astron. Soc., 476: 421 (2018)
[19]
M. C. Miller, arXiv: 1312.0029
[20]
F. Özel, Rep. Prog. Phys., 76: 016901 (2013)
[21]
M. C. Miller and F. K. Lamb, Eur. Phys. J. A, 52: 63 (2016)
[22]
V. F. Suleimanov, J. Poutanen, D. Klochkov et al., Eur. Phys. J. A, 52: 20 (2016)
[23]
B. P. Abbott et al., Phys. Rev. Lett., 119: 161101 (2017)
[24]
B. P. Abbott et al., Astrophys. J. Lett., 848: 12 (2017)
[25]
J. Piekarewicz, Proceedings of the XIV International Workshop on Hadron Physics, Florianópolis, 18-23 March 2018 pages 12-37, arXiv: 1805.04780
[26]
B. A. Li, P. G. Krastev, D. H. Wen et al., Eur. Phys. J. A, 55: 117 (2019)
[27]
C. A. Raithel, Eur. Phys. J. A, 55: 80 (2019)
[28]
L. Baiotti, Prog. Part. Nucl. Phys., 109: 103714 (2019)
[29]
B. P. Abbott et al., Phys. Rev. Lett., 121: 161101 (2018)
[30]
E. Annala, T. Gorda, A. Kurkela et al., Phys. Rev. Lett., 120: 172703 (2018)
[31]
E. R. Most, L. R. Weih, L. Rezzolla et al., Phys. Rev. Lett., 120: 261103 (2018)
[32]
F. J. Fattoyev, J. Piekarewicz, and C. J. Horowitz, Phys. Rev. Lett., 120: 172702 (2018)
[33]
R. Nandi, P. Char, and S. Pal, Phys. Rev. C, 99: 052802 (2019)
[34]
H. Tong, P. W. Zhao, and J. Meng, arXiv: 1903.05938
[35]
O. Lourenço, M. Dutra, C. H. Lenzi et al., arXiv: 1901.04529
[36]
C. A. Raithel, F. Özel, and D. Psaltis, Astrophys. J. Lett., 857: 23 (2018)
[37]
T. Malik, N. Alam, M. Fortin et al., Phys. Rev. C, 98: 035804 (2018)
[38]
Y. Zhou, L. W. Chen, and Z. Zhang, Phys. Rev. D, 99: 121301 (2019)
[39]
Y. Lim and J. W. Holt, Phys. Rev. Lett., 121: 062701 (2018)
[40]
D. Radice and L. Dai, Eur. Phys. J. A, 55: 50 (2019)
[41]
I. Tews, J. Margueron, and S. Reddy, Phys. Rev. C, 98: 045804 (2018)
[42]
S. De, D. Finstad, J. M. Lattimer et al., Phys. Rev. Lett, 121: 091102 (2018)
[43]
A. Bauswein A, O. Just, H. Janka et al., Astrophys. J. Lett, 850: L34 (2017)
[44]
B. Margalit and B. D. Metzger, Astrophys. J. Lett., 850: 19 (2017)
[45]
M. Shibata, S. Fujibayashi, K. Hotokezaka et al., Phys. Rev. D, 96: 123012 (2017)
[46]
L. Rezzolla, E. R. Most, and L. R. Weih, Astrophys. J. Lett., 852: 25 (2018)
[47]
M. Ruiz, S. L. Shapiro, and A. Tsokaros, Phys. Rev. D, 97: 021501 (2018)
[48]
E. P. Zhou, X. Zhou, and A. Li, Phys. Rev. D, 97: 083015 (2018)
[49]
G. Baym, S. Furusawa, T. Hatsuda et al., arXiv: 1903.08963
[50]
M. Shibata, E. Zhou, K. Kiuchi et al., Phys. Rev. D, 100: 023015 (2019)
[51]
N. B. Zhang and B. A. Li, Eur. Phys. J. A, 55: 39 (2019)
[52]
T. Hinderer, Astrophys. J., 677: 1216 (2008)
[53]
T. Hinderer, B. D. Lackey, R. N. Lang et al., Phys. Rev. D, 81: 123016 (2010)
[54]
R. C. Tolman, Proc. Natl. Acad. Sci. U.S.A., 20: 3 (1934)
[55]
J. Oppenheimer and G. Volkoff, Phys. Rev., 55: 374 (1939)
[56]
O. Lourenço, M. Dutra, C. H. Lenzi et al., Phys. Rev. C, 99: 045202 (2019)
[57]
C. Y. Tsang, M. B. Tsang, Pawel Danielewics et al., Phys. Lett. B, 796: 10 (2019)
[58]
Y. M. Kim, Y. Lim, K. Kwak et al., Phys. Rev. C, 98: 065805 (2018)
[59]
N. B. Zhang, B. A. Li, and J. Xu, Astrophys. J., 859: 90 (2018)
[60]
N. B. Zhang and B. A. Li, J. Phys. G: Nucl. Part. Phys., 46: 014002 (2019)
[61]
I. Bombaci and U. Lombardo, Phys. Rev. C, 44: 1892 (1991)
[62]
B. A. Brown and A. Schwenk, Phys. Rev. C, 89: 011307 (2014)
[63]
B. A. Li and X. Han, Phys. Lett. B, 727: 276 (2013)
[64]
M. Oertel, M. Hempel, T. Klähn et al., Rev. Mod. Phys., 89: 015007 (2017)
[65]
B. A. Li, Nuclear Physics News, 27: 7 (2017)
[66]
S. Shlomo, V. M. Kolomietz, and G. Colò, Eur. Phys. J. A, 30: 23 (2006)
[67]
J. Piekarewicz, J. Phys. G: Nucl. Part. Phys, 37: 064038 (2010)
[68]
I. Tews, J. M. Lattimer, A. Ohnishi et al., Astrophys. J., 848: 105 (2017)
[69]
N. B. Zhang, B. J. Cai, B. A. Li et al., Nucl. Sci. Tech., 28: 181 (2017)
[70]
G. Baym, C. J. Pethick, and P. Sutherland, Astrophys. J., 170: 299 (1971)
[71]
J. W. Negele and D. Vautherin, Nucl. Phys. A, 207: 298 (1973)
[72]
S. Kubis, Phys. Rev. C, 70: 065804 (2004)
[73]
S. Kubis, Phys. Rev. C, 76: 025801 (2007)
[74]
J. M. Lattimer and M. Prakash, Phys. Rep., 442: 109 (2007)
[75]
J. Xu, L. W. Chen, B. A. Li et al., Astrophys. J., 697: 1549 (2009)
[76]
J. Piekarewicz and F. J. Fattoyev, Phys. Rev. C, 99: 045802 (2019)
[77]
R. Gamba, J. S. Read, and L. E. Wade, arXiv: 1902.04616
[78]
F. Ji, J. N. Hu, S. S. Bao et al., Phys. Rev. C, 100: 045801 (2019)
[79]
J. M. Lattimer and M. Prakash, Phys. Rep., 333: 121 (2000)
[80]
J. M. Lattimer and M. Prakash, Astrophys. J., 550: 426 (2001)
[81]
F. J. Fattoyev, J. Carvajal, W. G. Newton et al., Phys. Rev. C, 87: 015806 (2013)
[82]
F. J. Fattoyev, W. G. Newton, and B. A. Li, Eur. Phys. J. A, 50: 45 (2014)
[83]
N. Hornick, L. Tolos, A. Zacchi et al., Phys. Rev. C, 98: 065804 (2018)
[84]
B. A. Li and A. W. Steiner, Phys. Lett. B, 642: 436 (2006)
[85]
T. E. Riley et al., Astrophys. J. Lett., 887: L21 (2019)
[86]
M. C. Miller et al., Astrophys. J. Lett., 887: L24 (2019)