Hawking radiation of massive vector particles from a warped AdS₃ black hole

Abstract

Hawking radiation (HR) of massive vector particles from a rotating Warped Anti-de Sitter black hole in 2+1 dimensions (WAdS3BH) is studied in detail. The quantum tunneling approach with the Hamilton-Jacobi method (HJM) is applied in the Proca equation (PE), and we show that the radial function yields the tunneling rate of the outgoing particles. Comparing the result obtained with the Boltzmann factor, we satisfactorily reproduce the Hawking temperature (HT) of the WAdS3BH.

Charged vector particles tunneling from black ring and 5D black hole

“…In this paper, the Hawking temperature is discussed for three coordinate systems. Gursel and Sakalli [17] studied the Hawking radiation of massive vector particles from rotating warped anti-de Sitter BH in 3D and showed that the radial mapping gives the tunneling rate for outgoing particles. Different authors [18,19] have found the Hawking temperature for various types of particles from BHs.…”

Quantum gravity effect on the Hawking radiation of spinning dilaton black hole

“…Nowadays, various methods have been proposed to calculate the temperature of a black hole known as Hawking temperature. On the other hand, the Hamilton-Jacobi approach is an important version of the tunnelling method of the quantum mechanical point-like particles from a black hole [4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19][20]. Adopting this approach, Hawking temperature of various black holes were recovered by quantum tunnelling method of the particles across their event horizons.…”

Eruptive Massive Vector Particles of 5-Dimensional Kerr-Gödel Spacetime

“…A reader would appreciate that the most subtle black holes are the rotating ones defined in the higher dimensions. From this viewpoint, we aim to extend the Kruglov's studies (and his followers' works [54][55][56][57][58][59][60][61][62][63][64][65]) to the radiation spectrum of massive vector particles spraying from a 5-dimensional Kerr-Gödel black hole (5DKGBH). Thus, we aim to calculate Hawking temperature [66] of the 5DKGBH.…”