Abstract

We study the electromagnetic field equation along with the WKB approximation. The boson tunneling phenomenon from charged rotating black ring (CRBR) is analyzed. It is examined that reserve radiation consistent with CRBR can be computed in general by neglecting back reaction and self-gravitational of the radiated boson particle. The calculated temperature depends upon quantum gravity and CRBR geometry. We also examine the corrected tunneling rate/probability of boson particles by assuming charge as well as energy conservation laws and the quantum gravity. Furthermore, we study the graphical behavior of the temperature and check the stability and instability of CRBR.

Highlights

  • Hawking studied the emission rate of radiation of all particles from black holes (BHs) and computed the temperature of the BH horizon.Tunneling is the semiclassical method in which boson particles have ability to cross the black ring and BH horizon

  • In order to study the tunneling probability for boson particles through the charged rotating black ring (CRBR) horizon y+, we will assume the Lagrangian equation with gravity and electromagnetic effects

  • The TH increases due to quantum gravity and remains constant when 0 ≤ y ≤ 0.65 and CRBR remains stable in this range

Read more

Summary

Introduction

Hawking studied the emission rate of radiation of all particles (photons, neutrinos, gravitons, positrons, etc.) from black holes (BHs) and computed the temperature of the BH horizon. Tunneling is the semiclassical method in which boson particles have ability to cross the black ring and BH horizon. The key component for examining modified tunneling radiation in the classical behavior of imaginary portion that includes the boson particles from the black ring horizon. Sharif and Javed analyzed [3] radiation spectrum through tunneling fermions in the BHs horizon family. Many authors have analyzed tunneling approach for different type particles with various spin such as fermions, scalar and bosons through the horizons of different black rings, wormholes and BHs, they studied their corresponding modified Hawking temperature.

Rotating Black Ring
Gravitational Stability Analysis
Conclusions

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.