Scalar particles emission from black holes with topological defects using Hamilton-Jacobi method

Abstract

We study quantum tunneling of charged and uncharged scalar particles from the event horizon of Schwarzschild-de Sitter and Reissner-Nordström-de Sitter black holes pierced by an infinitely long spinning cosmic string and a global monopole. In order to find the Hawking temperature and the tunneling probability we solve the Klein-Gordon equation by using the Hamilton-Jacobi method and WKB approximation. We show that Hawking temperature is independent of the presence of topological defects in both cases.

References in corpus (2)

• Landau Quantization in the Spinning Cosmic String Spacetime
• Hawking Radiation of Schwarzschild-de Sitter Black Hole by Hamilton-Jacobi method

Cited by in corpus (6)

• Massive Vector Particles Tunneling From Noncommutative Charged Black Holes and its GUP-corrected Thermodynamics
• Hawking radiation of scalar and vector particles from 5D Myers-Perry black holes
• The Bekenstein-Hawking Corpuscular Cascading from the Backreacted Black Hole
• Dirac Particles Tunneling from Black Holes with Topological Defects
• Bound and Scattering States in a Spacetime with Dual Topological Defects: Cosmic String and Global Monopole
• Cornell and Coulomb potentials in the double defect spacetime