alexa Semiclassical corrections to the Bekenstein-Hawking entropy of the BTZ black hole via selfgravitation
Physics

Physics

Research & Reviews: Journal of Pure and Applied Physics

Author(s): Elias C Vagenas

Abstract Share this page

Hawking radiation is viewed as a tunnelling process. In this way the effect of self-gravitation gives rise to semiclassical corrections to the entropy of the (2+1) BTZ black hole. The modified entropy, due to specific modelling of the self-gravitation effect, of the (2+1) BTZ black hole is evaluated. To first order in ω which is a shell of energy radiated outwards the event horizon of the BTZ black hole, modified entropy is proportional to the horizon. In this semiclassical analysis, corrections to the Bekenstein-Hawking formula SBH=AH/4l2P are found to be negative and the proportionality factor connecting the modified entropy, Sbh, of the (2+1) BTZ black hole to the Bekenstein-Hawking entropy, SBH, is evaluated to first order in ω.

This article was published in Phys.Lett. and referenced in Research & Reviews: Journal of Pure and Applied Physics

Relevant Expert PPTs

Relevant Speaker PPTs

Recommended Conferences

Relevant Topics

Peer Reviewed Journals
 
Make the best use of Scientific Research and information from our 700 + peer reviewed, Open Access Journals
International Conferences 2017-18
 
Meet Inspiring Speakers and Experts at our 3000+ Global Annual Meetings

Contact Us

 
© 2008-2017 OMICS International - Open Access Publisher. Best viewed in Mozilla Firefox | Google Chrome | Above IE 7.0 version
adwords