\begin{document}$ (1-\beta^2) $\end{document} and exhibits a symmetric double-peaked structure. This behavior arises primarily from the β dependence of mixing effects associated with the effective mass, in-medium scattering, and Fermi-momentum splitting, in addition to the contribution from the susceptibility. These results provide useful microscopic input for transport simulations and constraints on the nuclear symmetry energy."> Isospin diffusion coefficient for nuclear matter -
  • [1]

    B.-A. Li, L.-W. Chen, and C. M. Ko, Phys. Rep.464, 113 (2008)

  • [2]

    M. B. Tsanget al., Phys. Rev. Lett.92, 062701 (2004)

  • [3]

    M. B. Tsanget al., Phys. Rev. Lett.102, 122701 (2009)

  • [4]

    D. Page, U. Geppert, and F. Weber, Nucl. Phys. A777, 497 (2006)

  • [5]

    E. Flowers and N. Itoh, Astrophys. J.230, 847 (1979)

  • [6]

    A. W. Steiner and B.-A. Li, Phys. Rev. C72, 041601 (2005)

  • [7]

    Z. Y. Sunet al., Phys. Rev. C82, 051603 (2010)

  • [8]

    D. Yakovlev, A. Kaminker, O. Gnedinet al., Phys. Rep.354, 1 (2001)

  • [9]

    X. Shang, P. Wang, W. Zuo, and J. Dong, Phys. Lett. B811, 135963 (2020)

  • [10]

    A. Steiner, M. Prakash, J. Lattimeret al., Phys. Rep.411, 325 (2005)

  • [11]

    J. M. Lattimer and M. Prakash, Science304, 536 (2004)

  • [12]

    V. Baran, M. Colonna, V. Grecoet al., Phys. Rep.410, 335 (2005)

  • [13]

    L. Shi and P. Danielewicz, Phys. Rev. C68, 064604 (2003)

  • [14]

    L.-W. Chen, C. M. Ko, and B.-A. Li, Phys. Rev. Lett.94, 032701 (2005)

  • [15]

    J. M. Lattimer and M. Prakash, Phys. Rep.442, 109 (2007)

  • [16]

    L.-W. Chen, C. M. Ko, and B.-A. Li, Phys. Rev. C72, 064309 (2005)

  • [17]

    T. Sil, M. Centelles, X. Viñas, and J. Piekarewicz, Phys. Rev. C71, 045502 (2005)

  • [18]

    D.-H. Wen, B.-A. Li, and L.-W. Chen, Phys. Rev. Lett.103, 211102 (2009)

  • [19]

    B.-A. Li, C. M. Ko, and W. Bauer, Int. J. Mod. Phys. E07, 147 (1998)

  • [20]

    H. Tong, S. Elhatisari, U.-G. Meißneret al., arXiv: 2509.26148

  • [21]

    N.-B. Zhang and B.-A. Li, The Astrophysical Journal902, 38 (2020)

  • [22]

    N.-B. Zhang and B.-A. Li, The Astrophysical Journal893, 61 (2020)

  • [23]

    Ch en, Lie-Wen, EPJ Web of Conferences88, 00017 (2015)

  • [24]

    B.-A. Li, B.-J. Cai, W.-J. Xieet al., Universe7, 182 (2021)

  • [25]

    M. Kutschera, Phys. Lett. B340, 1 (1994)

  • [26]

    S. Kubis and M. Kutschera, Nucl. Phys. A720, 189 (2003)

  • [27]

    A. E. L. Dieperink, Y. Dewulf, D. Van Necket al., Phys. Rev. C68, 064307 (2003)

  • [28]

    A. A. Abrikosov and I. M. Khalatnikov, Reports on Progress in Physics22, 329 (1959)

  • [29]

    G. A. Brooker and J. Sykes, Annals of Physics56, 1 (1970)

  • [30]

    H. H. Jensen, H. Smith, and J. W. Wilkins, Phys. Rev.185, 323 (1969)

  • [31]

    R. H. Anderson, C. J. Pethick, and K. F. Quader, Phys. Rev. B35, 1620 (1987)

  • [32]

    O. Benhar and M. Valli, Phys. Rev. Lett.99, 232501 (2007)

  • [33]

    A. Carbone and O. Benhar, Journal of Physics: Conference Series336, 012015 (2011)

  • [34]

    H. F. Zhang, U. Lombardo, and W. Zuo, Phys. Rev. C82, 015805 (2010)

  • [35]

    H. F. Zhanget al., Phys. Rev. C76, 054001 (2007)

  • [36]

    P. S. Shternin, M. Baldo, and H.-J. Schulze, Journal of Physics: Conference Series932, 012042 (2017)

  • [37]

    P. S. Shternin and M. Baldo, Phys. Rev. D102, 063010 (2020)

  • [38]

    O. Benhar, A. Polls, M. Valliet al. Phys. Rev. C81, 024305 (2010)

  • [39]

    P. S. Shternin, M. Baldo, and P. Haensel, Phys. Rev. C88, 065803 (2013)

  • [40]

    S. Elhatisari, L. Bovermann, Y. Ma,et al., Nature630, 59 (2024)

  • [41]

    T. Wang, H. Tong, C. Wanget al., Phys. Rev. C112, 054322 (2025)

  • [42]

    Z. H. Li, U. Lombardo, H.-J. Schulzeet al., Phys. Rev. C77, 034316 (2008)

  • [43]

    W. Zuo, A. Lejeune, U. Lombardoet al., Nucl. Phys. A706, 418 (2002)

  • [44]

    W. Zuo, A. Lejeune, U. Lombardoet al., Eur. Phys. J. A14, 469 (2002)

  • [45]

    G. Baym and C. J. Pethick,Landau Fermi-Liquid Theory: Concepts and Applications(New York: Wiley, 1991)

  • [46]

    R.-J. Liu, J. Xu, and Y.-G. Ma, Phys. Lett. B868, 139703 (2025)

  • [47]

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

  • [48]

    W. Zuo, I. Bombaci, and U. Lombardo, Phys. Rev. C60, 024605 (1999)

  • [49]

    X.-L. Shang, J.-M. Dong, W. Zuoet al., Phys. Rev. C103, 034316 (2021)

  • [50]

    X. L. Shang, A. Li, Z. Q. Miaoet al., Phys. Rev. C101, 065801 (2020)

  • [51]

    R. B. Wiringa, V. G. J. Stoks, and R. Schiavilla, Phys. Rev. C51, 38 (1995)

  • [52]

    S. C. Han, X. L. Shang, W. Zuoet al., Phys. Rev. C106, 064332 (2022)

  • [53]

    J.-B. Wei, G. F. Burgio, and H.-J. Schulze, Mon. Not. R. Astron. Soc.484, 5162 (2019)

  • [54]

    D. Bugg, Nucl. Phys. A416, 227 (1984)

  • [55]

    T. C. Montgomery, B. E. Bonner, F. P. Bradyet al., Phys. Rev. C16, 499 (1977)

  • [56]

    R. Keeler, R. Dubois, E. Auldet al., Nucl. Phys. A377, 529 (1982)

  • [57]

    C. Ducoin, J. Margueron, C. Providênciaet al., Phys. Rev. C83, 045810 (2011)

  • [58]

    S. K. Saha, D. R. Entem, R. Machleidtet al., Phys. Rev. C107, 034002 (2023)

  • [59]

    E. Epelbaum, H. Krebs, and U.-G. Meißner, Eur. Phys. J. A51, 53 (2015)

  • [60]

    P. Reinert, H. Krebs, and E. Epelbaum, Eur. Phys. J. A54, 86 (2018)

  • [61]

    Z. X. Yang, X. L. Shang, G. C. Yonget al., Phys. Rev. C100, 054325 (2019)

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