\begin{document}$ \Lambda_{1.4} $\end{document} of canonical NSs with different error and different lower boundaries, and with the tidal deformabilities of massive NSs. We found that it does not significantly improve the constraints on the NS EOS but has a weak effect on narrowing down the slope parameter of the symmetry energy by decreasing the measurement errors of \begin{document}$ \Lambda_{1.4} $\end{document}. Both the isospin-dependent and isospin-independent parts of the NS EOS were significantly constrained and raised as the tidal deformabilities of massive NSs were adopted in the calculations, especially in high-density regions. We also found that \begin{document}$ \Lambda_{1.4} $\end{document} is more competent to limit the curvature parameter than the slope parameter of the symmetry energy, whereas the opposite occurs for the radius of canonical NSs \begin{document}$ R_{1.4} $\end{document}. The tidal deformability of an NS with two times the solar mass \begin{document}$ \Lambda_{2.0} $\end{document} is more sensitive to skewness than the curvature parameter of the symmetry energy, and \begin{document}$ \Lambda_{1.4} $\end{document} and \begin{document}$ R_{1.4} $\end{document} have no correlation with the former."> Dependence of the tidal deformability of neutron stars on the nuclear equation of state -
  • [1]

    P. Danielewicz, R. Lacey, and W. G. Lynch, Science298, 1592 (2002)

  • [2]

    J. M. Lattimer and M. Prakash, Phys. Rep.621, 127 (2016)

  • [3]

    M. Oertel, M. Hempel, T. Klähnet al., Rev. Mod. Phys.89, 015007 (2017)

  • [4]

    M. B. Tsanget al., Phys. Rev. C86, 105803 (2012)

  • [5]

    M. Baldo and G. F. Burgio, Prog. Part. Nucl. Phys.91, 203 (2016)

  • [6]

    B. A. Li, B. J. Cai, L. W. Chenet al., Prog. Part. Nucl. Phys.99, 29 (2018)

  • [7]

    L. Baiotti, Prog. Part. Nucl. Phys.109, 103714 (2019)

  • [8]

    B. A. Li, P. G. Krastev, D. H. Wenet al., Eur. Phys. J. A55, 39 (2019)

  • [9]

    B. Honget al., Eur. Phys. J. A50, 49 (2014)

  • [10]

    A. Tamii, P. von Neumann-Cosel, and I. Poltoratska, Eur. Phys. J. A50, 28 (2014)

  • [11]

    R. Bougaultet al., Eur. Phys. J. A50, 47 (2014)

  • [12]

    Z. G. Xiaoet al., Euro. Phys. J. A50, 37 (2014)

  • [13]

    W. Trautmann, AIP Conference Proceedings2127, 020003 (2019)

  • [14]

    T. Aumann and C. A. Bertulani, Prog. Part. Nucl. Phys.112, 103753 (2020), arXiv:1910.14094

  • [15]

    The Scientifc Case for the 400 MeV/u Energy Upgrade of FRIB,https://fribusers.org/documents/2019/FRIB400-Upgrade.pdf

  • [16]

    B. P. Abbottet al. (LIGO and Virgo Collaborations), Phys. Rev. Lett.119, 161101 (2017)

  • [17]

    B. P. Abbottet al. (LIGO and Virgo Collaborations), Phys. Rev. Lett.121, 161101 (2018)

  • [18]

    A. L. Wattset al., Sci. China Phys. Mech. Astron.62, 29503 (2019)

  • [19]

    T. E. Rileyet al., Astrophys. J. Lett.887, L21 (2019)

  • [20]

    G. Raaijmakerset al., Astrophys. J. Lett.887, L22 (2019)

  • [21]

    M. C. Milleret al., Astrophys. J. Lett.887, L24 (2019)

  • [22]

    I. Bombaci and U. Lombardo, Phys. Rev. C44, 1892 (1991)

  • [23]

    F. J. Fattoyev, J. Piekarewicz, and C. J. Horowitz, Phys. Rev. Lett.120, 172702 (2018)

  • [24]

    E. Annala, T. Gorda, A. Kurkelaet al., Phys. Rev. Lett.120, 172703 (2018)

  • [25]

    E. R. Most, L. R. Weih, L. Rezzollaet al., Phys. Rev. Lett.120, 261103 (2018)

  • [26]

    P. G. Krastev and B. A. Li, J. Phys. G: Nucl. Part. Phys.46, 074001 (2019)

  • [27]

    Y. Lim and J. W. Holt, Phys. Rev. Lett.121, 062701 (2018)

  • [28]

    I. Tews, J. Margueron, and S. Reddy, Phys. Rev. C98, 045804 (2018)

  • [29]

    T. Hinderer, Astrophys. J.677, 1216 (2008)

  • [30]

    K. Yagi and N. Yunes, Phys. Rev. D88, 023009 (2013)

  • [31]

    S. Bernuzzi, A. Nagar, M. Thierfelderet al., Phys. Rev. D86, 044030 (2012)

  • [32]

    K. Hotokezaka, K. Kyutoku, Y.-i. Sekiguchiet al., Phys. Rev. D93, 064082 (2016)

  • [33]

    R. Dudi, F. Pannarale, T. Dietrichet al., Phys. Rev. D98, 084061 (2018)

  • [34]

    S. Bernuzzi, T. Dietrich, and A. Nagar, Phys. Rev. Lett.115, 091101 (2015)

  • [35]

    K. Takami, L. Rezzolla, and L. Baiotti, Phys. Rev. D91, 064001 (2015)

  • [36]

    L. Rezzolla and K. Takami, Phys. Rev. D93, 124051 (2016)

  • [37]

    N. B. Zhang, B. A. Li, and J. Xu, Astrophys. J859, 90 (2018)

  • [38]

    I. Tews, J. Margueron, and S. Reddy, Eur. Phys. J. A55, 97 (2019)

  • [39]

    P. Landry and R. Essick, Phys. Rev. D99, 084049 (2019)

  • [40]

    T. Malik, N. Alam, and M. Fortin, Phys. Rev. C98, 035804 (2018)

  • [41]

    Y. Fujimoto, K. Fukushima, and K. Murase, Phys. Rev. D101, 054016 (2020)

  • [42]

    T. Narikawa, N. Uchikata, K. Kawaguchiet al., Phys. Rev. Research1, 033055 (2019)

  • [43]

    G. Montaña, L. Tolós, and M. Hanauske, L. Rezzolla Phys. Rev. D99, 103009 (2019)

  • [44]

    S. Han and A. W. Steiner, Phys. Rev. D99, 083014 (2019)

  • [45]

    T. Zhao and J. M. Lattimer, Phys. Rev. D98, 063020 (2018)

  • [46]

    J.-E. Christian, A. Zacchi, and J. Schaffner-Bielich, Phys. Rev. D99, 023009 (2019)

  • [47]

    W. J. Xie and B. A. Li, Astrophys. J883, 174 (2019)

  • [48]

    W. J. Xie and B. A. Li, Astrophys. J899, 4 (2020)

  • [49]

    S. Shlomo, V.M. Kolomietz, and G. Colò, Eur. Phys. J. A30, 23 (2006)

  • [50]

    J. Piekarewicz, J. Phys. G37, 064038 (2010)

  • [51]

    B.A. Li and X. Han, Phys. Lett. B727, 276 (2013)

  • [52]

    I. Tews, J. M. Lattimer, A. Ohnishiet al., Astrophys. J848, 105 (2017)

  • [53]

    N. B. Zhang, B. J. Cai, B. A. Liet al., Nucl. Sci. Tech.28, 181 (2017)

  • [54]

    J. W. Negele and D. Vautherin, Nucl. Phys. A207, 298 (1973)

  • [55]

    G. Baym, C. J. Pethick, and P. Sutherland, Astrophys. J170, 299 (1971)

  • [56]

    T. Hinderer, B. D. Lackey, and R. N. Lang, Phys. Rev. D81, 123016 (2010)

  • [57]

    B. Kumar and P. Landry, Phys. Rev. D99, 123026 (2019)

  • [58]

    J. Piekarewicz and F. J. Fattoyev, Phys. Rev. C99, 045802 (2019)

  • [59]

    R. Trotta, (2017) arXiv:1701.01467

  • [60]

    >F. Douchin and P. Haensel, A&A380(1), 151-167 (2001)

  • [61]

    F. J. Fattoyev, J. Carvajal, W. G. Newtonet al., Phys. Rev. C87, 015806 (2013)

  • [62]

    J. M. Lattimer and M. Prakash, Astrophys. J550, 426 (2001)

  • [63]

    R. Nandi, P. Char, and S. Pal, Phys. Rev. C99, 052802 (2019)

  • [64]

    J. Hu, S. Bao, Y. Zhanget al., Prog. Theor. Exp. Phys.2020, 043D (2020)

  • [65]

    Y. Zhou, L. W. Chen, and Z. Zhang, Phys. Rev. D99, 121301 (2019)

  • [66]

    C. Y. Tsang, M. B. Tsang, P. Danielewiczet al., Phys. Lett. B796, 1 (2019)

  • [67]

    N. B. Zhang, B. Qi, and S. Y. Wang, Chin. Phys. C44, 064103 (2020)

  • [68]

    N. B. Zhang, B. A. Li, J. Phys. G46, 014002 (2019)

  • [69]

    Y. Lim and J. W. Holt, Eur. Phys. J. A55, 209 (2019)

Baidu
map