Cosmological models with inhomogeneous viscous fluids and a logarithmic equation of state in the Friedman– Lemaitre–Robertson–Walker Universe are considered. The influence of thermal effects caused by Hawking radiation on the visible horizon of the Universe on the change in the singularity type of the dark Universe is investigated. It is shown that under the influence of thermal radiation, taking into account the viscosity property of a dark fluid, a qualitative change in the type of the Big Rip singularity is possible, which can lead to the absence of the singularity in the Universe at all.
Similar content being viewed by others
References
A. G. Riess et al., Astron. J., 116, 1009−10038 (1998).
S. Perlmutter et al., Astron. J., 517, 565−586 (1999).
K. Bamba, S. Capozziello, S. Nojiri, and S. D. Odintsov, Astrophys. Space Sci., 342, 155−310 (2012).
S. Nojiri and S. D. Odintsov, Phys. Lett. B, 562, 147−152 (2003).
K. Nakamura et al., J. Phys. G, 37, 075021−075035 (2010).
R. G. Cai and N. Ohta, Phys. Rev. D, 81, 084061−084077 (2010).
S. Nojiri and S. D. Odintsov, Phys. Dark Univ., 30, 100695−100706 (2020).
S. Capozziello, V. Cardone, E. Elizalde, et al., Phys. Rev. D, 73, 043512 (2006).
I. Brevik, E. Elizalde, S. Nojiri, and S. D. Odintsov, Phys. Rev. D, 84, 103508 (2011).
S. Nojiri and S. D. Odintsov, Int. J. Geom. Meth. Mod. Phys., 4, 115–145 (2007).
S. Nojiri and S. D. Odintsov, Phys. Rev. D, 72, 023003 (2005).
S. D. Odintsov, V. K. Oikonomou, A. V. Timoshkin, et al., Ann. Phys., 398, 238−253 (2018).
S. Capozziello, R. D’Agostino, and O. Luongo, Phys. Dark Univ., 20, 1–12 (2018).
I. Brevik, O. Gron, J. de Haro, et al., Int. J. Mod. Phys. D, 26, 1730024−1730095 (2017).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 9, pp. 128–133, September, 2021.
Rights and permissions
About this article
Cite this article
Makarenko, A.N., Timoshkin, A.V. Influence of Thermal Radiation on Singular Behavior of the Universe. Russ Phys J 64, 1724–1730 (2022). https://doi.org/10.1007/s11182-022-02513-8
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11182-022-02513-8