A note on Maxwell’s equal area law for black hole phase transition
نویسندگان
چکیده
منابع مشابه
Schwarzschild Black Hole and Area Law
Using a graphical analysis, we show that for the horizon radius rh & 4.8 √ θ, the standard semiclassical Bekenstein-Hawking area law for noncommutative Schwarzschild black hole exactly holds for all orders of θ. We also give the corrections to the area law to get the exact nature of the Bekenstein-Hawking entropy when rh < 4.8 √ θ till the extremal point rh = 3.0 √ θ. The familiar notion of bla...
متن کاملBlack Hole Entropy: Departures from Area Law
The thermodynamic and euclidean functional integral approaches to black hole entropy are discussed. The existence of some freedom in the definition of the entropy is pointed out and the possibility of a departure from the semiclassical expression discussed in the light of quantum corrections. The semiclassical area dependence of the entropy of matter in the background of a black hole is also re...
متن کاملThe phase transition of corrected black hole with f(R) gravity
In this letter, we consider static black hole in f(R) gravity.We take advantage from corrected entropy and temperature and investigate such black hole. Finally, we study the $ P - V $ critically and phase transition of corrected black hole with respect to entropy and temperature. Here also, we obtain the heat capacity for the static black hole in $ f(R) $ gravity. This calculation help us...
متن کاملA note on the black hole remnant
Analyzing the quantum tunneling probability of a Schwarzschild black hole with a negative log-area correction to Bekenstein-Hawking entropy, I argue that this correction may be closely related to a black hole remnant. The value for the minimal black hole mass is also discussed.
متن کاملGeneralized Area Law under Multi-parameter Rotating Black Hole Spacetime
Abstract We study the statistical mechanics for quantum scalar fields under the multiparameter rotating black hole spacetime in arbitrary D dimensions. The method of analysis is general in the sense that the metric does not depend on the explicit black hole solutions. The generalized Stefan-Boltzmann’s law for the scalar field is derived by considering the allowed energy region properly. Then t...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The European Physical Journal C
سال: 2015
ISSN: 1434-6044,1434-6052
DOI: 10.1140/epjc/s10052-015-3641-0