• [1]

    R. C. Duncan and C. Thompson, Astrophys. J 392, L9 (1992)

  • [2]

    M. Vietri, L. Stella, and G. Israel, Astrophys. J 661, 1089 (2007)

  • [3]

    S. Mereghetti, Astron. Astrophys. Rev. 15, 225 (2008)

  • [4]

    A. Tiengo et al., Nature 500, 312 (2013)

  • [5]

    S. A. Olausen and V. M. Kaspi, Astrophys. J 212, 6 (2014)

  • [6]

    V. Kaspi and A. M. Beloborodov, Ann. Rev. Astron. Astrophys. 55, 261 (2017)

  • [7]

    B. Carter, E. Chachoua, and N. Chamel, Gen. Rel. Grav. 38, 83 (2006)

  • [8]

    A. L. Watts and T. E. Strohmayer, Adv. Sp. Res. 40, 1446 (2007)

  • [9]

    L. Samuelsson and N. Andersson, Mon. Not. Roy. Astron. Soc. 374, 256 (2007)

  • [10]

    N. Andersson, K. Glampedakis, and L. Samuelsson, Mon. Not. Roy. Astron. Soc. 396, 894 (2009)

  • [11]

    A. Passamonti and S. K. Lander, Mon. Not. Roy. Astron. Soc. 438, 156 (2014)

  • [12]

    R. Nandi, P. Char, D. Chatterjee et al., Phys. Rev. C 94, 025801 (2016)

  • [13]

    D. N. Aguilera, V. Cirigliano, J. A. Pons et al., Phys. Rev. Lett. 102, 091101 (2009)

  • [14]

    D. Viganò, N. Rea, J. A. Pons et al., Mon. Not. Roy. Astron. Soc. 434, 123 (2013)

  • [15]

    A. Y. Potekhin and G. Chabrier, Astron. Astrophys. 609, A74 (2018)

  • [16]

    N. Chamel and P. Haensel, Living Rev. Relativity 11, 10 (2008)

  • [17]

    D. Lai and S.L. Shapiro, Astrophys. J 383, 745 (1991)

  • [18]

    N. Chamel, R. L. Pavlov, L. M. Mihailov et al., Phys. Rev. C 86, 055804 (2012)

  • [19]

    N. Chamel, Zh. K. Stoyanov, L. M. Mihailov et al., Phys. Rev. C 91, 065801 (2015)

  • [20]

    Y. D. Mutafchieva, N. Chamel, Zh. K. Stoyanov et al., Phys. Rev. C 99, 055805 (2019)

  • [21]

    V. Parmar, H. C. Das, M. K. Sharma et al., Phys. Rev. D 107, 043022 (2023)

  • [22]

    V. N. Kondratyev, T. Maruyama, and S. Chiba, Phys. Rev. Lett. 84, 1086 (2000)

  • [23]

    V. N. Kondratyev, T. Maruyama, and S. Chiba, Astrophys. J 546, 1137 (2001)

  • [24]

    D. Peña Arteaga, M. Grasso, E. Khan et al., Phys. Rev. C 84, 045806 (2011)

  • [25]

    M. Stein, J. Maruhn, A. Sedrakian et al., Phys. Rev. C 94, 035802 (2016)

  • [26]

    G. Baym, C. Pethick, and P. Sutherland, Astrophys. J 170, 299 (1971)

  • [27]

    D. Basilico, D. P. Arteaga, X. Roca-Maza et al., Phys. Rev. C 92, 035802 (2015)

  • [28]

    D. N. Sob'yanin, Phys. Rev. D 107, L081301 (2023)

  • [29]

    C.Y. Cardall, M. Prakash, and J.M. Lattimer, Astrophys. J 554, 322 (2001)

  • [30]

    K. Kiuchi and S. Yoshida, Phys. Rev. D 78, 044045 (2008)

  • [31]

    J. Frieben and L. Rezzolla, Mon. Not. Roy. Astron. Soc. 427, 3406 (2012)

  • [32]

    A. G. Pili, N. Bucciantini, and L. Del Zanna, Mon. Not. Roy. Astron. Soc. 439, 3541 (2014)

  • [33]

    D. Chatterjee, T. Elghozi, J. Novak et al., Mon. Not. Roy. Astron. Soc. 447, 3785 (2015)

  • [34]

    A. Tsokaros, M. Ruiz, S. L. Shapiro et al., Phys. Rev. Lett. 128, 061101 (2022)

  • [35]

    J. A. Maruhn, P.-G. Reinhard, P. D. Stevenson et al., Comput. Phys. Commun. 185, 2195 (2014)

  • [36]

    B. Schuetrumpf, P.-G. Reinhard, P. D. Stevenson et al., Comput. Phys. Commun. 229, 211 (2018)

  • [37]

    E. Chabanat, P. Bonche, P. Haensel et al., Nucl. Phys. A 635, 231 (1998)

  • [38]

    W. Greiner et al., Nuclear models (Springer, 1996)

  • [39]

    K. Sekizawa and K. Kaba, arXiv: 2302.07923 [nucl-th]