Abstract

We study the Hawking radiation of Dirac particles from Phantom Reissner Nordstrom ADS black hole by tunneling method. We use charge relativistic Dirac equation to study the emission of such particles. To solve Dirac equation we use WKB approximation and find the tunneling probability of outgoing particles. Finally we find the Hawking temperature for such type of black holes.

Highlights

  • Particles and anti particles are created permanently at the event horizon of the black hole due to the high gravitational fields and vacuum fluctuations

  • Hawking radiation as quantum tunneling effect at event horizons of the black holes is discussed by different authors and quantum tunneling method (Parikh and Wilczek, 2000; Padmanabhan, 2004; Srinivasan and Padmanabhan, 1999; Shankaranarayanan et al, 2002; Kraus and Wilczek, 2009; 1995; Kerner and Mann, 2006; 2007; 2008; Rehman and Saifullah, 2011; Gillani and Saifullah, 2011; Ahmed and Saifullah, 2011; Gohar and Saifullah 2012a, 2012b, 2013; Jan and Gohar, 2013) is robust method to discuss these radiation

  • For Λ > 0, It behaves as De Sitter (DS) and for Λ < 0, It behaves as Anti De Sitter (ADS)

Read more

Summary

INTRODUCITON

Particles and anti particles are created permanently at the event horizon of the black hole due to the high gravitational fields and vacuum fluctuations. Hawking radiation as quantum tunneling effect at event horizons of the black holes is discussed by different authors and quantum tunneling method (Parikh and Wilczek, 2000; Padmanabhan, 2004; Srinivasan and Padmanabhan, 1999; Shankaranarayanan et al, 2002; Kraus and Wilczek, 2009; 1995; Kerner and Mann, 2006; 2007; 2008; Rehman and Saifullah, 2011; Gillani and Saifullah, 2011; Ahmed and Saifullah, 2011; Gohar and Saifullah 2012a, 2012b, 2013; Jan and Gohar, 2013) is robust method to discuss these radiation We can apply this method to almost all type of black holes in different gravity theories from higher dimensions to lower dimensions (Ejaz et al, 2013; Vagenas, 2002; Medved and Vagenas, 2005; Matsuno and Umetsu, 2011; Kim, 2011; Hod, 2011; Wu and Peng, 2011). In this study we have used the tunneling method to discuss the emission of Dirac particles from Phantom Reissner Nordstrom ADS black hole and get the Hawking temperature for this black hole

PHANTOM REISSNER NORDSTROM ADS BLACK HOLE
QUANTUM TUNNELING
CONCLUSION

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.