\begin{document}$ \beta \approx 0-1.99 $\end{document}. For values of \begin{document}$ \beta $\end{document} near zero, the deviation between the proposed model and the \begin{document}$ \mathrm{\Lambda } $\end{document} CDM model is significant, while for \begin{document}$ \beta \to 1.99 $\end{document}, the suggested model has no conflict with the \begin{document}$ \mathrm{\Lambda } $\end{document} CDM theory. Regardless of the value of \begin{document}$ \beta $\end{document}, the model considers dark energy to behave as matter with positive pressure in high redshifts, \begin{document}$ {\omega }_{X}\approx 0.33 $\end{document}, while for present and near-future Universe, it is considered to behave similar to that in the cosmological constant model and phantom field. Comparing the model with the Ricci dark energy model, we show that our model reduces the errors of the Ricci dark energy model concerning the calculation of the age of old supernovae and evolution of different cosmic components in high redshifts. Moreover, we calculated matter structure formation parameters such as the CMB temperature and matter power spectrum of the model to consider the effects of matter-like dark energy during the matter-dominated era."> Holographic dark energy from acceleration of particle horizon -
  • [1]

    C. L. Bennett et al, ApJS208, 20 (2013)

  • [2]

    G. Hinshaw et al, ApJS208, 19 (2013)

  • [3]

    E. L. Wright, New Astro. Rev.47, 877 (2003)

  • [4]

    M. J. Mortonson, Phys. Rev. D80, 123504 (2009)

  • [5]

    M. S. Turner et al, Phys. Rev. Lett.52, 2090 (1984)

  • [6]

    A. Rajagopal et al, Phys. Lett. B737, 277 (2014)

  • [7]

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

  • [8]

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

  • [9]

    K. J. Ludwick, Phys. Rev. D92, 063019 (2015)

  • [10]

    Pao-Yu Wanget al., arXiv:1208.6579

  • [11]

    S. Weinberg, arXiv:astro-ph/0005265

  • [12]

    N. K. Sharma and J. K. Singh, Int. J. Theor. Phys. ,53, 2912 (2014)

  • [13]

    J. K. Singh, R. Nagpal, and S. K. J. Pacif, Int. J. Geom. Meth. Mod. Phys.15, 1850049 (2018)

  • [14]

    P. H. R. S. Moraeset al., Eur. Phys. J. C77, 480 (2017)

  • [15]

    A. Nath, P. K. Sahoo, and S. K. Sahu, The Eur. Phys. J. Plus,131, 18 (2016)

  • [16]

    M. F. Shamir, Commun. Theor. Phys.65, 3 (2016)

  • [17]

    M. E. S. Alves, P. H. R. S. Moraes, J. C. N. de Araujoet al., Phys. Rev. D94, 024032 (2016)

  • [18]

    Jun-Qi Guoet al., Phys. Rev. D88, 124036 (2013)

  • [19]

    A. Paliathanasiset al., Phys. Rev. D94, 023525 (2016)

  • [20]

    H. R. Fazlollahi, Phys. Dark Univ.35, 100962 (2022)

  • [21]

    G. t’ Hooft, Basics and Highlights in Fundamental Physics, 72 (2001)

  • [22]

    L. Susskind, J. Math. Phys.36, 6377 (1995)

  • [23]

    J. M. Maldacena, Adv. Theor. Math. Phys.2, 231 (1998)

  • [24]

    W. Fischler and L. Susskind, arXiv:hep-th/9806039

  • [25]

    R. Bousso, Rev. Mod. Phys.74, 825 (2000)

  • [26]

    A. Cohen, D. Kaplan, and A. Nelson, Phys. Rev. Lett.82, 4971 (1999)

  • [27]

    P. Horava and D. Minic, Phys. Rev. Lett.85, 1610 (2000)

  • [28]

    S. Thomas, Phys. Rev. Lett.89, 081301 (2002)

  • [29]

    L. N. Granda and A. Oliveros, Phys. Lett. B669, 275 (2008)

  • [30]

    M. Li et al, JCAP2009, 036 (2009)

  • [31]

    S. del Campo et al, Phys. Rev. D83, 123006 (2011)

  • [32]

    G. Ghaffari et al, Phys. Rev. D89, 123009 (2014)

  • [33]

    K. Karami and J. Fehri, Int. J. Theor. Phys.49, 1118 (2010)

  • [34]

    C. Gaoet al., Phys. Rev. D79, 043511 (2009)

  • [35]

    Xin Zhang, Phys. Rev. D79, 103509 (2009)

  • [36]

    M. BouhmadiLopezet al., Euro. Phys. J. C78, 330 (2018)

  • [37]

    Chao-Jun Feng and Xin-Zhou Li, Phys. Lett. B680(4), 355 (2009)

  • [38]

    C. P. Singh and A. Kumar, Astrophysics and Space Science364, 94 (2019)

  • [39]

    R. Bousso, JHEP1999, 004 (1999)

  • [40]

    S. D. H. Hsu, Phys. Lett. B594, 13 (2004)

  • [41]

    M. Li, Phys. Lett. B603, 1 (2004)

  • [42]

    M. Cruz and S. Lepe, Nucl. Phys. B956, 115017 (2020)

  • [43]

    N. Aghanimet al. (Planck Collaboration),Astron. & Astrophys.641, A6 (2018), [Erratum:Astron. & Astrophys. 652, C4 (2021)]

  • [44]

    D. Foreman-Mackeyet al, PASP125, 306 (2013)

  • [45]

    Z. H. Zhu, M. K. Fujimoto, and X. T. He, ApJ603, 365 (2004)

  • [46]

    J. Dunlop, J. Peacock, H. Spinradet al., Nature381, 581 (1996)

  • [47]

    H. Spinradet al., Astrophys. J.484, 581 (1997)

  • [48]

    D. Jain and A. Dev, Phys. Lett. B633(4-5), 436 (2006)

  • [49]

    B. Diemer,, ApJS239, 35 (2018), arXiv:1712.04512

  • [50]

    A. Lewis and A. Challinor,http://camb.info/

  • [51]

    P. Abrialet al., Stat. Methodology5, 289 (2008)

  • [52]

    J. Delabrouilleet al., A&A493, 835 (2009)

Baidu
map