Eruptive Massive Vector Particles of 5-Dimensional Kerr-Gödel Spacetime
arXiv:1705.00061 · doi:10.1007/s10773-017-3564-7
Abstract
In this paper, we investigate Hawking radiation of massive spin-1 particles from 5-dimensional Kerr-Gödel spacetime. By applying the WKB approximation and the Hamilton-Jacobi ansatz to the relativistic Proca equation, we obtain the quantum tunneling rate of the massive vector particles. Using the obtained tunneling rate, we show how one impeccably computes the Hawking temperature of the 5-dimensional Kerr-Gödel spacetime.
5 pages; 2-columns; will appear in International Journal of Theoretical Physics (IJTP)
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- Hawking radiation from cubic and quartic black holes via tunneling of GUP corrected scalar and fermion particles
- Gravity Effects on Hawking Radiation from Charged Black Strings in Rastall Theory
- Gravitational Analysis of Rotating Charged Black Hole-Like Solution in Einstein-Gauss-Bonnet Gravity
- Quantum Tunneling and Quasinormal Modes in the Spacetime of Alcubierre Warp Drive
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- Asymptotically-Flat Black Hole Solutions in Symmergent Gravity
- Emergent GUP from Modified Hawking Radiation in Einstein-NED Theory