- 
								[1]
								L. W. Chen, C. M. Ko, and B. A. Li, Phys. Rev. Lett. 94, 032701 (2005) 
- 
								[2]
								B. A. Li and X. Han, Phys. Lett. B 727, 276 (2013) 
- 
								[3]
								B. A. Li, L. W. Chen, and C. M. Ko, Phys. Rep. 464, 113 (2008) 
- 
								[4]
								B. A. Li, P. G. Krastev, D. H. Wen et al., arXiv: 1905.13175 
- 
								[5]
								A. E. L. Dieperink, Y. Dewulf, D. Van Neck et al., Phys. Rev. C 68, 064307 (2003) 
- 
								[6]
								P. Russotto, S. Gannon, and S. Kupny, et al., Phys. Rev. C 94, 034608 (2016) 
- 
								[7]
								A. Le Fevre et al., Nucl. Phys. A 945, 112 (2016) 
- 
								[8]
								D. Adhikari et al., Phys. Rev. Lett. 126, 172502 (2021) 
- 
								[9]
								M. C. Miller et al., Astrophys. J. Lett. 918, L28 (2021) 
- 
								[10]
								T. E. Riley et al., Astrophys. J. Lett. 918, L27 (2021) 
- 
								[11]
								P. T. Pang, I. Tews, and M. W. Coughlin et al., Astrophys. J. 922, 14 (2021) 
- 
								[12]
								B. P. Abbott et al., Phys. Rev. lett. 121, 161101 (2018) 
- 
								[13]
								M. Feroci et al., Experimental Astronomy 34, 415 (2012) 
- 
								[14]
								http://www.the-athena-x-ray-observatory.eu. 
- 
								[15]
								M. Punturo et al., Classical and Quantum Gravity 27, 194002 (2010) 
- 
								[16]
								P. E. Dewdney et al., Proceedings of the IEEE 97, 1482 (2009) 
- 
								[17]
								L. Rezzolla et al., The Physics and Astrophysics of Neutron Stars (Springer International Publishing, 2018) 
- 
								[18]
								L. Lindblom, Astrophys. J. 398, 569 (1992) 
- 
								[19]
								J. Xu, Z. Zhang, and B. A. Li, Phys. Rev. C 104, 054324 (2021) 
- 
								[20]
								S. Huth et al., Nature 606, 276 (2022) 
- 
								[21]
								Y. Li, H. Chen, D. Wen et al., Eur. Phys. J. A 57, 1 (2021) 
- 
								[22]
								H. O. Silva, A. M. Holgado, A. Cardenas-Avendano et al., Phys. Rev. Lett. 126, 181101 (2021) 
- 
								[23]
								W. J. Xie and B. A. Li, Astrophys. J. 883, 174 (2019) 
- 
								[24]
								S. I. Amari and M. A. Arbib, A Neural Model for the Handling of Phenomena Associated with Trains of Light Stimuli: An Updated Version to Fit Fusion Data, p.117 (University of Massachusetts, 1977) 
- 
								[25]
								S. Gazula, J. Clark, and H. Bohr, Nucl. Phys. A 540, 1 (1992) 
- 
								[26]
								K. Gernoth, J. Clark, J. Prater et al., Phys. Lett. B 300, 1 (1993) 
- 
								[27]
								K. Gernoth and J. Clark, Neural Networks 8, 291 (1995) 
- 
								[28]
								J. W. Clark, T. Lindenau, and M. Ristig, Scientific Applications of Neural Nets, Vol. 522 (Springer-Verlag, Berlin, 1998) 
- 
								[29]
								T. Zhao and H. Zhang, Nucl. Phys. A 1021, 122420 (2022) 
- 
								[30]
								Z. M. Niu and H. Z. Liang, Phys. Lett. B 778, 48 (2018) 
- 
								[31]
								R. Utama, J. Piekarewicz, and H. B. Prosper, Phys. Rev. C 93, 014311 (2016) 
- 
								[32]
								R. Utama, W. C. Chen, J. Piekarewicz et al., Nucl. Part. Phys. 43, 114002 (2016) 
- 
								[33]
								Y. Fujimoto, K. Fukushima, and K. Murase, Phys. Rev. D 98, 023019 (2018) 
- 
								[34]
								S. Soma, L. Wang, S. Shi et al., arXiv: 2201.01756 
- 
								[35]
								P. G. Krastev, Galaxies 10, 16 (2022) 
- 
								[36]
								A. Thete, K. Banerjee, and T. Malik, arXiv: 2208.13163 
- 
								[37]
								D. Farrell, P. Baldi, J. Ott et al., arXiv: 2209.02817 
- 
								[38]
								N. B. Zhang, B. A. Li, and J. Xu, Astrophys. J. 859, 90 (2018) 
- 
								[39]
								N. B. Zhang, B. J. Cai, B. A. Li et al., Nucl. Sci. Technol. 28, 181 (2017) 
- 
								[40]
								S. Shlomo, V. M. Kolomietz, and G. Colo, Eur. Phys. J. A 30, 23 (2006) 
- 
								[41]
								J. Piekarewicz, Journal of Physics G Nuclear Physics 37, 064038 (2010) 
- 
								[42]
								M. Oertel, M. Hempel, T. Klähn et al., Rev. Mod. Phys. 89, 015007 (2017) 
- 
								[43]
								B. A. Li, Nuclear Physics News 27, 7 (2017) 
- 
								[44]
								J. W. Negele and D. Vautherin, Nucl. Phys. A 207, 298 (1973) 
- 
								[45]
								G. Baym, C. Pethick, and P. Sutherland, Astrophys. J. 170, 299 (1971) 
- 
								[46]
								J. R. Oppenheimer and G. M. Volkoff, Phys. Rev. 55, 374 (1939) 
- 
								[47]
								R. C. Tolman, Phys. Rev. 55, 364 (1939) 
- 
								[48]
								E. E. Flanagan and T. Hinderer, Phys. Rev. D 77, 021502(R) (2008) 
- 
								[49]
								T. Hinderer, Astrophys. J. 677, 1216 (2008) 
- 
								[50]
								T. Hinderer, B. D. Lackey, R. N. Lang et al., Phys. Rev. D 81, 123016 (2010) 
- 
								[51]
								H. T. Cromartie, E. Fonseca, S. M Ransom et al., Nat. Astron. 4, 72 (2020) 
- 
								[52]
								Y. Fujimoto and M. Nitta, JHEP 2021, 192 (2021) 
- 
								[53]
								P. Haensel, J. L. Zdunik, and F. Douchin, Astron. Astrophys. 385, 301 (2002) 
- 
								[54]
								V. Doroshenko et al, Nat. Astron. 6, 1444 (2022) 
- 
								[55]
								M. C. Miller, F. K. Lamb, A. J. Dittmann et al., Astrophys. J. Lett. 887, L24 (2019) 
- 
								[56]
								T. E. Riley, A. L. Watts, S. Bogdanov et al., Astrophys. J. Lett. 887, L21 (2019) 
- 
								[57]
								L. G. Wright, T. Onodera, M. M. Stein et al., Nature 601, 549 (2022) 
- 
								[58]
								K. Hornik, M. Stinchcombe, and H. White, Neural networks 3, 551 (1990) 
- 
								[59]
								M. Leshno et al., Neural Networks 6, 861 (1993) 
- 
								[60]
								J. Heaton, Genet. Program Evolvable Mach 19, 305 (2018) 
- 
								[61]
								D. P. Kingma and J. Ba Adam, arXiv: 1412.6980 
- 
								[62]
								F. Chollet, https://github.com/fchollet/keras 
- 
								[63]
								M. Abadi, A. Agarwal, P. Barham et al., arXiv: 1603.04467