Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 26, Issue 8, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/26/8/085010
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Funding
- Council of Scientific and Industrial Research (CSIR), Government of India
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Using a graphical analysis, we show that for the horizon radius r(h) greater than or similar to 4.8 root theta, the standard semiclassical Bekenstein-Hawking area law for a noncommutative Schwarzschild black hole exactly holds for all orders of theta. We also give the corrections to the area law to get the exact nature of the Bekenstein-Hawking entropy when r(h) < 4.8 root theta till the extremal point r(h) = 3.0 root theta.
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