publication . Preprint . 2013

Thermodynamics of the apparent horizon in massive cosmology

Li, Hui; Zhang, Yi;
Open Access English
  • Published: 17 Apr 2013
Applying Clausius relation with energy-supply defined by the unified first law of thermodynamics formalism to the apparent horizon of a massive cosmological model proposed lately, the corrected entropic formula of the apparent horizon is obtained with the help of the modified Friedmann equations. This entropy-area relation, together with the identified internal energy, verifies the first law of thermodynamics for the apparent horizon with a volume change term for consistency. On the other hand, by means of the corrected entropy-area formula and the Clausius relation $\delta Q=T dS$, the modified Friedmann equations governing the dynamical evolution of the univer...
free text keywords: General Relativity and Quantum Cosmology, High Energy Physics - Theory
Related Organizations
Download from
46 references, page 1 of 4

[1] A. G. Riess et al., Astron. J. 116, 1009 (1998), astro-ph/9805201; S. Perlmutter et al., Astrophys. J. 517, 565 (1999), astro-ph/9812133.

[2] B. Ratra and P. J. E. Peebles, Phys. Rev. D37, 3406 (1988); R. Caldwell, R. Dave and P. J. Steinhardt, Phys. Rev. Lett. 80, 1582 (1998); C. Armendariz-Picon, V. Mukhanov and Paul J. Steinhardt, Phys.Rev.Lett. 85, 4438 (2000); R. J. Scherrer, Phys.Rev.Lett. 93, 011301 (2004); L. P. Chimento and R. Lazkoz, Phys.Rev. D71, 023505 (2005); H. Wei and R.G. Cai, Phys.Rev. D71, 043504 (2005); J. M. Aguirregabiria, L. P. Chimento and R. Lazkoz, astro-ph/0411258; Z.K. Guo, Y.S. Piao, X. M. Zhang and Y. Z. Zhang, Phys. Lett. B608, 177 (2005); B. Feng, M. Z. Li, Y. S. Piao and X. M. Zhang, Phys. Lett. B634, 101 (2006); H. Wei and R. G. Cai, Phys. Lett. B660, 113 (2008).

[3] S. Weinberg, Rev. Mod. Phys. 61 (1989) 1; N. Straumann, astro-ph/0203330; T. Padmanabhan, hep-th/0406060.

[4] G. Dvali, G. Gabadadze and M. Perrati, Phys. Lett. B485, 208 (2000) [hep-th/0005016].

[5] M. Fierz and W. Pauli, Proc. Roy. Soc. Lond. A173, 211 (1939).

[6] T. Damour and I.I. Kogan, Phys.Rev. D66, 104025 (2002).

[7] A. H. Chamseddine and M. S. Volkov, arXiv:1107.5504.

[8] H. van Dam and M. J. G. WVeltman, Nucl. Phus. B22, 397 (1970); V. I. Zakharov, JETP Lett. 12, 312 (1970).

[9] A.I. Vainshtein, Phys. Lett. B39, 393 (1972).

[10] D. G. Boulware and S. Deser, Ann. Phys. 89,193 (1975).

[11] C. de Rham, G. Gabadadze and A. J. Tolley, Phys. Rev. Lett. 106, 231101 (2011) [arXiv:1011.1232].

[12] S. F. Hassan and R. A. Rosen, arXiv:1106.3344.

[13] G. D' Amico, C. de Rham, G. Gabadadze, D. Pirtskhalava and A. J. Tolley, arXiv:1108.5231; Y. F. Cai, D. A. Easson, C. X. Gao and E. N. Saridakis, Phys. Rev. D87, 064001 (2013) [arXiv:1211.0563].

[14] S. W. Hawking, Commun. Math. Phys. 43, 199 (1975); J. D. Bekenstein, Phys. Rev. D7,2333 (1973); J. M. Bardeen, N. Carter adn S. W. Hawking, Commun. Math. Phys. 31, 161 (1973).

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

46 references, page 1 of 4
Powered by OpenAIRE Open Research Graph
Any information missing or wrong?Report an Issue