Greybody factor for black string in dRGT massive gravity

Abstract

The greybody factor from the black string in the de Rham-Gabadadze-Tolley (dRGT) massive gravity theory is investigated in this study. The dRGT massive gravity theory is one of the modified gravity theories used in explaining the current acceleration in the expansion of the universe. By using cylindrical symmetry, black strings in dRGT massive gravity are shown to exist. When quantum effects are taken into account, black strings can emit thermal radiation called Hawking radiation. The Hawking radiation at spatial infinity differs from that at the source by the so-called greybody factor. In this paper, we examined the rigorous bounds on the greybody factors from the dRGT black strings. The results show that the greybody factor crucially depends on the shape of the potential characterized by model parameters. The results agree with ones in quantum mechanics, the higher the potential, the harder it is for the waves to penetrate and also lower the bound for the rigorous bounds.

18 pages, 12 figures; V2 accepted to EPJC, minor change, two column 11 pages, 12 figures

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• Greybody factors emitted by a regular black hole in a non-minimally coupled Einstein-Yang-Mills theory
• Greybody factor for massive fermion emitted by a black hole in dRGT massive gravity theory
• Probing Effective Loop Quantum Gravity on Weak Gravitational Lensing, Hawking Radiation and Bounding Greybody Factor by Black Holes
• The Dirac and Klein-Gordon equations and Greybody Radiation for the Regular Hayward Black Hole
• ISCOs and OSCOs in the presence of a positive cosmological constant in massive gravity
• Massive gravity solution of Black Holes and Entropy Bounds