\begin{document}$G_3(X,\phi)\neq 0$\end{document} and \begin{document}$G_5=\text{const}/X$\end{document}. A global unidirectional electromagnetic field interacts with a scalar field according to the law \begin{document}$f^2(\phi)F_{\mu\nu}F^{\mu\nu}$\end{document}. In Horndeski theory, the anisotropy can develop in different ways. The proposed reconstruction method allows us to build models with acceptable anisotropy behavior. To analyze space-time anisotropy, we use the relations \begin{document}$a_i/a$\end{document} (\begin{document}$i=1,2,3$\end{document}), where \begin{document}$a_i$\end{document} are metric functions, and \begin{document}$a\equiv(a_1a_2a_3)^{1/3}$\end{document}."> Isotropization of the magnetic universe in Horndeski theory with <i>G</i><sub>3</sub>(<i>X</i>,<i>ϕ</i>) and <i>G</i><sub>5</sub>(<i>X</i>) -
  • [1]

    A. G. Doroshkevich, Astrophys. J.1, 138 (1965)

  • [2]

    K. S. Thorne, Astrophys. J.148, 51 (1967)

  • [3]

    K. C. Jacobs, Astrophys. J.155, 379 (1969)

  • [4]

    M. Salimyx, S. L. Sautuyk, and R. Martins, Class. Quantum Grav.15, 1521 (1998)

  • [5]

    J. T. Horwood and J. Wainwright, Gen. Rel. Grav.36, 799 (2004)

  • [6]

    K. A. Bronnikov, E. N. Chudayeva, and G. N. Shikin, Class. Quantum Grav.21, 3389 (2004)

  • [7]

    M. Watanabe, S. Kanno, and J. Soda, PRL102, 191302 (2009)

  • [8]

    J. Soda, Class. Quantum Grav.29, 083001 (2012)

  • [9]

    T. Q. Do, W. F. Kao, Phys. Rev. D96, 023529 (2017)

  • [10]

    D. H. Nguyen, T. M. Pham, and T. Q. Do, Eur. Phys. J. C81, 839 (2021)

  • [11]

    R. Casadio, A. Kamenshchik, P. Petriakovaet al., Phys. Rev. D108, 084059 (2023)

  • [12]

    G. W. Horndeski, Int. J. Theor. Phys.10, 363 (1974)

  • [13]

    T. Kobayashi, M. Yamaguchi, and J. Yokoyama, Prog. Theor. Phys.126, 511 (2011)

  • [14]

    G. Hinshawet al., Astrophys. J. Suppl. Ser.208, 19 (2013)

  • [15]

    P. A. R. Adeet al., Astron. Astrophys.594, A16 (2016)

  • [16]

    B. Abareshiet al. (DESI Collaboration), AJ164, 207 (2022)

  • [17]

    A. G. Adameet al. (DESI Collaboration), arXiv: 2404.03002

  • [18]

    D. Saadeh, S. M. Feeney, A. Pontzenet al., Phys. Rev. Lett.117, 131302 (2016)

  • [19]

    G. F. R. Ellis, Gen. Relat. Gravit.38(6), 1003 (2006)

  • [20]

    E. Komatsuet al., Astrophys. J. Suppl.192, 18 (2011)

  • [21]

    M. Thorsrud, D. F. Mota, and S. Hervik, J. High. Energ. Phys.2012, 66 (2012)

  • [22]

    R. K. Muharlyamov and T. N. Pankratyeva, Mod. Phys. Lett. A34, 1950239 (2019)

  • [23]

    H. Amirhashchi and S. Amirhashchi, Phys. Rev. D99, 023516 (2019)

  • [24]

    M. Koussour, H. Filali, S. H. Shekhet al., Nucl. Phys. B978, 115738 (2022)

  • [25]

    M. Koussour and M. Bennai, Class. Quantum Grav.39, 105001 (2022)

  • [26]

    O. Akarsu, S. Kumar, S. Sharmaet al., Phys. Rev. D100, 023532 (2019)

  • [27]

    P. Sarmah and U. D. Goswami, Mod. Phys. Lett. A37, 2250134 (2022)

  • [28]

    S. W. Hawking and R. J. Taylor, Nature299, 1278 (1966)

  • [29]

    B. L. Hu and L. Parker, Phys. Rev. D17, 933 (1978)

  • [30]

    M. Jamil, D. Momeni, N. S. Serikbayevet al., Astrophys. Space Sci.339, 37 (2012)

  • [31]

    M. Jamil, S. Ali, D. Momeniet al., Eur. Phys. J. C72, 1998 (2012)

  • [32]

    M. Dehpour, Int. J. Mod. Phys. A38, 2350181 (2023)

  • [33]

    M. de Cesare and E. Wilson-Ewing, JCAP12, 039 (2019)

  • [34]

    R. Galeev, R. K. Muharlyamov, A. A. Starobinskyetet al., Phys. Rev. D103, 104015 (2021)

  • [35]

    H. W. H. Tahara, S. Nishi, T. Kobayashiet al., JCAP07, 058 (2018)

  • [36]

    S. Hawking and R. Laflamme, Phys. Lett. B209, 39 (1988)

  • [37]

    L. Campanelli, Phys. Rev. D84, 123521 (2011)

  • [38]

    W. Rahmanet al., Mon. Not. R. Astron. Soc.514, 139 (2022)

  • [39]

    K. Bhattacharya and S. Chakraborty, Phys. Rev. D99, 023520 (2019)

  • [40]

    A. Deet al., Eur. Phys. J. C82, 72 (2022)

  • [41]

    A. H. A. Alfedeel and R. K. Tiwari, Indian J. Phys.96, 1877 (2022)

  • [42]

    S. Aroraet al., JCAP09, 042 (2022)

  • [43]

    M. Sharif and A. Majid, Eur. Phys. J. Plus137, 114 (2022)

  • [44]

    F. Esposito, S. Carloni, R. Cianciet al., Phys. Rev. D105, 084061 (2022)

  • [45]

    R. Arjona, W. Cardona, and S.Nesseris, Phys. Rev. D100, 063526 (2019)

  • [46]

    R. K. Muharlyamov and T. N. Pankratyeva, Eur. Phys. J. Plus136, 590 (2021)

  • [47]

    R. K. Muharlyamov and T. N. Pankratyeva, Mod. Phys. Lett. A37, 2250108 (2022)

  • [48]

    R. K. Muharlyamov and T. N. Pankratyeva, Indian J. Phys.97, 2239 (2023)

  • [49]

    R. C. Bernardo and J. L. Said, JCAP09, 014 (2021)

  • [50]

    R. C. Bernardo, D. Grandon, J. L. Saidet al., Phys. Dark Universe36, 101017 (2022)

  • [51]

    R. C. Bernardo and I. Vega, JCAP10, 058 (2019)

  • [52]

    C. Gao, JCAP06, 023 (2010)

  • [53]

    L. N. Granda and W. Cardona, JCAP07, 021 (2010)

  • [54]

    Q. Shafi and C. Wetterich, Phys. Lett. B152, 51 (1985)

  • [55]

    Q. Shafi and C. Wetterich, Nucl. Phys. B289, 787 (1987)

  • [56]

    R. K. Muharlyamov, T. N. Pankratyeva, and S. O. A. Bashir, Mod. Phys. Lett. A39, 2450085 (2024)

  • [57]

    Q. Fang, S. Chen, and J. Jing, Int. J. Mod. Phys. D28, 1950112 (2019)

  • [58]

    O. Tattersal, P. Ferreira, and M. Lagos, Phys. Rev. D97, 084005 (2018)

  • [59]

    C. Deffayet, O. Pujolas, I. Sawickiet al., JCAP10, 026 (2010)

  • [60]

    O. Pujolas, I. Sawicki, and A. Vikman, JHEP11, 156 (2011)

Baidu
map