Author(s):
1. Muhammad Sadiq:
Department of Physics, University of Tabuk, P.O. Box 2072, Tabuk 71451, Saudi Arabia
Abstract:
A holographic version of the equipartition of energy was derived for a general diffeomorphism invariant theory by Padhmanabhan (2010). We discerned that Hawking's temperature is the equipartition law, or vice versa, granted that the horizon area is measured in Planck units (2017). Under the equipartition law, we wish to point out that the semi-classical holographic setup, including the Bekenstein-Hawking entropy, is consistent only when the horizon is quantized in exact Planck units. This is in clear contrast to the previously obtained values of the minimal area from theories such as loop quantum gravity and others. It becomes evident that the previously determined values though good for the entropy formula, are inconsistent with the equipartition law, hence with Hawking's temperature.
Page(s):
405-408
DOI:
DOI not available
Published:
Journal: Science International, Volume: 33, Issue: 5, Year: 2021
Keywords:
black hole
,
Immirzi parameter
,
loop quantum gravity
,
quantum gravity
,
Equipartition
References:
References are not available for this document.
Citations
Citations are not available for this document.