\begin{document}$ H(z) $\end{document}, SNe) and gravitational wave data (Tianqin) to constrain the interacting dark energy (IDE) model and investigate the Hubble tension and coincidence problems. By combining these four types of data (Tianqin+H0LiCOW+SNe+\begin{document}$ H(z) $\end{document}), we obtained the following parameter values with a confidence interval of \begin{document}$ 1\sigma $\end{document}: \begin{document}$ \Omega_m=0.36\pm0.18 $\end{document}, \begin{document}$ \omega_x=-1.29^{+0.61}_{-0.23} $\end{document}, \begin{document}$ \xi=3.15^{+0.36}_{-1.1} $\end{document}, and \begin{document}$H_0=70.04\pm $\end{document}\begin{document}$ 0.42~ {\rm kms}^{-1}{\rm Mpc}^{-1}$\end{document}. According to our results, the best value of \begin{document}$ H_0 $\end{document} shows that the Hubble tension problem can be alleviated to some extent. In addition, the center value of \begin{document}$ \xi+3\omega_x = -0.72^{+2.19}_{-1.19}(1\sigma) $\end{document} indicates that the coincidence problem is slightly alleviated. However, \begin{document}$ \xi+3\omega_x = 0 $\end{document} is still within the \begin{document}$ 1\sigma $\end{document} error range, which indicates that the ΛCDM model is still the model in best agreement with the observational data at present. Finally, we compared the constraint results of the electromagnetic and gravitational waves on the model parameters and found that the constraint effect of electromagnetic wave data on model parameters is better than that of simulated Tianqin gravitational wave data."> Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem -
  • [1]

    A. G. Riesset al., Astron. J.116, 1009 (1998)

  • [2]

    D. H. Weinberget al., Phys. Rep.530, 87 (2013)

  • [3]

    D. Scolnicet al., Astrophys. J.859, 101 (2018)

  • [4]

    S. Perlmutteret al., Astrophys. J.517, 565 (1999)

  • [5]

    M. Tegmark, M. R. Blanton , M. A. Strausset al., Astrophys. J.606, 70 (2004)

  • [6]

    D. Spergelet al., Astrophys. J. Suppl.148, 175 (2003)

  • [7]

    N. Aghanimet al. (Planck Collaboration), Astron. Astrophys.641, A6 (2020)

  • [8]

    P. J. Peebles and B. Ratra, Rev. Mod. Phys.75, 559 (2003)

  • [9]

    P. Bullet al., Phys. Dark Universe12, 56 (2016)

  • [10]

    J. S. Bullock and M. Boylan-Kolchin, ARAA55, 343 (2017)

  • [11]

    S. Weinberg, Rev. Mod. Phys61, 1 (1989)

  • [12]

    S. M. Carroll, W. H. Press, and E. L. Turner, ARAA30, 499 (1992)

  • [13]

    Riess. A. G., S. Casertano, W. Yuanet al., ApJ876, 85 (2019)

  • [14]

    Lan Mingjian, Pan Jicheng, Pan Yuet al., SCIENTIA SINICA Physica, Mechanica & Astronomica50, 079501 (2020)

  • [15]

    I. Zlatev, L. Wang, and P. J. Steinhardt, Phys. Rev. Lett.82, 896 (1999)

  • [16]

    S. M. Carroll, Phys. Rev. Lett.81, 3067 (1998)

  • [17]

    R. R. Caldwell , R. Dave, and P. J. Steinhardt, Phys. Rev. Lett.80, 1582 (1998)

  • [18]

    A. R. Liddle and R. J. Scherrer, Phys. Rev. D59, 023509 (1998)

  • [19]

    R. R. Caldwell, Phys. Lett. B545, 23 (2002)

  • [20]

    S. M. Carroll , M. Hoffman, and M. Trodden, Phys. Rev. D68, 023509 (2003)

  • [21]

    B. Feng, X. Wang, and X. Zhang, Phys. Lett. B607, 35 (2005)

  • [22]

    M. Li and Y. Wang, Phys. Lett. B687, 243 (2010)

  • [23]

    T. Yang, Z. K. Guo, R. G. Cai, Phys. Rev. D91, 123533 (2015)

  • [24]

    H. Wei, Nucl. Phys. B845, 381 (2011)

  • [25]

    B. Wang, Y. Gong, and E. Abdalla, Phys. Lett. B624, 141 (2005)

  • [26]

    B. P. Abbottet al., Nature551, 85 (2017)

  • [27]

    R.-G. Cai and T. Yang, Phys. Rev. D95, 4 (2017)

  • [28]

    X.-N. Zhanget al., Phys. Rev. D99, 063510 (2019)

  • [29]

    J.-F. Zhanget al., JCAP09, 068 (2019)

  • [30]

    J. Zheng, Y. Chen, T. P. Xuet al., Eur. Phys. J. Plus137, 509 (2022)

  • [31]

    O. Bertolami, F. Gil Pedro, and M. Le Delliou, Phys. Lett. B654, 165 (2007)

  • [32]

    O. Bertolami, F. G. Pedro Morgan, and L. Delliou, Gen. Relat. Gravit.41, 2839 (2009)

  • [33]

    M. L. Delliou, O. Bertolami, and F. G. Pedro, AIP Conf. Proc.957, 421 (2007)

  • [34]

    A. Oscoz, E. Mediavilla, M. Serra-Ricartet al., EAS Publications Ser.30, 161 (2008)

  • [35]

    E. Abdalla, L. R. Abramo, and L. Sodre Jr.et al., Phys. Lett. B673, 107 (2009)

  • [36]

    E. Abdalla, L. R. Abramo, and J. C. C. de Souza, Phys. Rev. D82, 023508 (2010)

  • [37]

    Y. Chen, Z. H. Zhu, J. S. Alcanizet al., Astrophys. J.711, 439 (2010)

  • [38]

    S. Cao and N. Liang, Int. J. Mod. Phys. D22, 1350082 (2013)

  • [39]

    S. Cao, Y. Chen, J. Zhanget al., Int. J. Theor. Phys.54, 1492 (2015)

  • [40]

    Y. Pan, S. Cao, and L. Li, Int. J. Mod. Phys. D25, 1650003 (2016)

  • [41]

    S. Liu, Y.-M. Hu, J.-D. Zhanget al., Phys. Rev. D101, 103027 (2020)

  • [42]

    J. Mei, Y.-Z. Bai, J. Baoet al., PTEP2021, 05A107 (2021)

  • [43]

    T. E. Strohmayer, Astrophys. J.627, 920 (2005)

  • [44]

    H. Wan, Z. Jiang, A. Sesanaet al., Phys. Rev. D100, 043003 (2019)

  • [45]

    Y.-M. Hu, J. Mei, and J. Luo, Natl. Sci. Rev.4, 683 (2017)

  • [46]

    X. C. Hu, X. H. Li, Y. Wanget al., Class. Quant. Grav.35, 095008 (2018)

  • [47]

    S. Cao, X. Li, M. Biesiadaet al., Astrophys. J.835, 92 (2017)

  • [48]

    S. Cao, J. Qi, M. Biesiadaet al., Astrophys. J.867, 50 (2018)

  • [49]

    J.-W. Diao, Y. Pan, and W. Xu, Res. Astron. Astrophys.22, 115019 (2022)

  • [50]

    W.-F. Feng, H.-T. Wang, X.-C. Huet al., Phys. Rev. D99, 123002 (2019)

  • [51]

    S. A. Hughes, Class. Quant. Grav.18, 4067 (2001), arXiv:gr-qc/0008058

  • [52]

    A. Sesana, Phys. Rev. Lett.116, 231102 (2016)

  • [53]

    H. Di and Y. Gong, JCAP07, 007 (2018), arXiv:1707.09578

  • [54]

    S. Ölmez, V. Mandic, and X. Siemens, Phys. Rev. D81, 104028 (2010), arXiv:1004.0890

  • [55]

    Bennett, c. L.et al., Astrophys. J.794, 135 (2014)

  • [56]

    B. F. Schutz, Nature323, 310 (1986)

  • [57]

    J. Luo, L.-S. Chen, H.-Z. Duanet al., Class. Quant. Grav.33, 035010 (2016)

  • [58]

    W. Zhao, C. Van Den Broeck, D. Baskaranet al., Phys. Rev. D83, 023005 (2011)

  • [59]

    B. S. Sathyaprakash, B. F. Schutz, and C. Van den Broeck, Class. Quant. Grav.27, 215006 (2010)

  • [60]

    N. Suzuki, D. Rubin, C. Lidmanet al., Astrophys. J.746, 85 (2012)

  • [61]

    J. J. Wei and X. F. Wu, Astrophys. J.838, 160 (2017)

  • [62]

    K. C. Wong, S. H. Suyu, M. W. Augeret al., Mon. Not. R. Astron. Soc.465, 4895 (2017)

  • [63]

    C. E. Rusu, C. D. Fassnacht, D. Sluseet al., Mon. Not. R. Astron. Soc.467, 4220 (2017)

  • [64]

    D. Sluse, A. Sonnenfeld, N. Rumbaet al., Mon. Not. R. Astron. Soc.470, 4838 (2017)

  • [65]

    V. Bonvin, F. Courbin, S. H. Suyuet al., Mon. Not. R. Astron. Soc.465, 4914 (2017)

  • [66]

    P. A. R. Adeet al. (Planck Collaboration), Astron. Astrophys.571, A16 (2014)

Baidu
map