Evolving Horava cosmological horizons

  • Several sets of radially propagating null congruence generators are exploited in order to form 3-dimensional marginally trapped surfaces, referred to as black hole and cosmological apparent horizons in a Hořava universe. Based on this method, we deal with the characteristics of the 2-dimensional space-like spheres of symmetry and the peculiarities of having trapping horizons. Moreover, we apply this method in standard expanding and contracting FLRW cosmological models of a Hořava universe to investigate the conditions under which the extra parameters of the theory may lead to trapped/anti-trapped surfaces both in the future and in the past. We also include the cases of negative time, referred to as the finite past, and discuss the formation of anti-trapped surfaces inside the cosmological apparent horizons.
      PCAS:
  • 加载中
  • [1] P. Horava, Physical Review D, 79:084008(2009)
    [2] C. Charmousis, G. Niz, A. Padilla, P. M. Saffin, Journal of High Energy Physics, 08:070(2009)
    [3] S. Weinfurtner, T. P. Sotiriou, M. Visser, Journal of Physics:Conference Series, 222:012054(2010)
    [4] K. Koyama, F. Arroja, Journal of High Energy Phsyics, 03:061(2010)
    [5] D. Blas, O. Pujols, S. Sibiryakov, Journal of High Energy Physics, 10:029(2009)
    [6] D. Blas, O. Pujols, S. Sibiryakov, Physical Review Letters, 104:181302(2010)
    [7] J. Klusoň, Physical Review D, 82:044004(2010)
    [8] J. Klusoň, Journal of High Energy Physics, 07:038(2010)
    [9] P. Horava, C. M. Melby-Thompson, Physical Review D, 82:064027(2010)
    [10] J. Klusoň, S. Nojiri, S. D. Odintsov, D. Sez-Gmez, European Physical Journal C, 71:1690(2011)
    [11] J. Klusoň, European Physical Journal C, 71:1820(2011)
    [12] T. Griffin, P. Horava, C. M. Melby-Thompson, Physical Review Letters, 110:081602(2013)
    [13] M. Chaichian, J. Klusoň, M. Oksanen, Physical Review D, 92:104043(2015)
    [14] A. O. Barvinsky, D. Blas, M. Herrero-Valea, S. M. Sibiryakov, C. F. Steinwachs, Physical Review D, 93:064022(2016)
    [15] M.I. Park, Journal of High Energy Physics, 0909:123(2009)
    [16] A. Kehagias, K. Sfetsos, Physics Letters B, 678:123(2009)
    [17] H. Lu, J. Mei, C.N. Pope, Physical Review Letters, 103:091301(2009)
    [18] C. Capasso, Physical Review D, 82:124058(2010)
    [19] R-G. Cai, S. P. Kim, JHEP, 0502:050(2005)
    [20] R-G. Cai, L-M. Cao, Y-P Hu, Class. Quant. Grav., 26:155018(2009)
    [21] R-G. Cai, L-M. Cao, N. Ohta, Phys. Rev. D, 80:024003(2009)
    [22] R-G. Cai, L-M. Cao, N. Ohta, Physics Letters B, 679:504(2009)
    [23] R-G. Cai, N. Ohta, Physical Review D, 81:084061(2010)
    [24] I. Radinschi, F. Rahaman, A. Banerjee, International Journal of Theoretical Physics, 50:2906(2011)
    [25] I. Radinschi, F. Rahaman, A. Banerjee, International Journal of Theoretical Physics, 51:1425(2012)
    [26] J. Chen, Y. Wang, International Journal of Modern Physics A, 25 (7):1439(2010)
    [27] A. Abdujabbarov, B. Ahmedov, A. Hakimov, Physical Review D, 83:044053(2011)
    [28] J. Sadeghi, B. Pourhassan, The European Physical Journal C, 72:1984(2012)
    [29] R. Penrose, Physical Review Letters, 14:57(1965)
    [30] S. W. Hawking, R. Penrose, Proceedings of the Royal Society A, 314:529(1970)
    [31] E. Barausse, T. Jacobson, T. P. Sotiriou, Physical Review D, 83:124043(2011)
    [32] E. Abdalla, N. Afshordi, M. Fontanini, Physical Review D, 89:104018(2014)
    [33] M. Saravani, N. Afshordi, R.B. Mann, Physical Review D, 89:084029(2014)
    [34] S. Mukohyama, Classical and Quantum Gravity, 27:223101(2010)
    [35] R. L. Arnowitt, S. Deser, C. W. Misner, The Dynamics of General Relativity, edited by Louis Witten:Wilew, New York (1962)
    [36] V. Faraoni, Galaxies, 1:114(2013)
    [37] E. Poisson:A Relativists Toolkit:The Mathematics of Black-Hole Mechanics (Cambridge:Cambridge University Press, UK 2004)
    [38] V. Mukhanov, Physical Foundations of Cosmology (Cambridge:Cambridge University Press, UK 2005)
  • 加载中

Get Citation
Mohsen Fathi and Morteza Mohseni. Evolving Horava cosmological horizons[J]. Chinese Physics C, 2016, 40(9): 095101. doi: 10.1088/1674-1137/40/9/095101
Mohsen Fathi and Morteza Mohseni. Evolving Horava cosmological horizons[J]. Chinese Physics C, 2016, 40(9): 095101.  doi: 10.1088/1674-1137/40/9/095101 shu
Milestone
Received: 2016-06-02
Article Metric

Article Views(1376)
PDF Downloads(140)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Evolving Horava cosmological horizons

    Corresponding author: Mohsen Fathi,
    Corresponding author: Morteza Mohseni,
  • 1. Department of Physics, Payame Noor University (PNU), P. O. Box 19395-3697 Tehran, I. R. of Iran

Abstract: Several sets of radially propagating null congruence generators are exploited in order to form 3-dimensional marginally trapped surfaces, referred to as black hole and cosmological apparent horizons in a Hořava universe. Based on this method, we deal with the characteristics of the 2-dimensional space-like spheres of symmetry and the peculiarities of having trapping horizons. Moreover, we apply this method in standard expanding and contracting FLRW cosmological models of a Hořava universe to investigate the conditions under which the extra parameters of the theory may lead to trapped/anti-trapped surfaces both in the future and in the past. We also include the cases of negative time, referred to as the finite past, and discuss the formation of anti-trapped surfaces inside the cosmological apparent horizons.

    HTML

Reference (38)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return