Abstract
As early as 1902, Gibbs pointed out that systems whose partition function diverges, e.g. gravitation, lie outside the validity of the Boltzmann–Gibbs (BG) theory. Consistently, since the pioneering Bekenstein–Hawking results, physically meaningful evidence (e.g., the holographic principle) has accumulated that the BG entropy S BG of a (3+1) black hole is proportional to its area L 2 (L being a characteristic linear length), and not to its volume L 3. Similarly it exists the area law, so named because, for a wide class of strongly quantum-entangled d-dimensional systems, S BG is proportional to lnL if d=1, and to L d−1 if d>1, instead of being proportional to L d (d≥1). These results violate the extensivity of the thermodynamical entropy of a d-dimensional system. This thermodynamical inconsistency disappears if we realize that the thermodynamical entropy of such nonstandard systems is not to be identified with the BG additive entropy but with appropriately generalized nonadditive entropies. Indeed, the celebrated usefulness of the BG entropy is founded on hypothesis such as relatively weak probabilistic correlations (and their connections to ergodicity, which by no means can be assumed as a general rule of nature). Here we introduce a generalized entropy which, for the Schwarzschild black hole and the area law, can solve the thermodynamic puzzle.
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Notes
Notice that Newtonian gravitation generates a double difficulty, namely at vanishing distances and at diverging distances. The mathematical difficulty at short distances, where the potential decreases without limit, is nowadays considered to be solved due to the quantum nature of physical laws; this was of course unknown by Gibbs at his time. The mathematical difficulty at long distances remains still today in what concerns the thermostatistical properties, in fact intensively studied nowadays.
From the microscopic (classical) dynamical point of view, this anomaly is directly related to the fact that the entire Lyapunov spectrum vanishes in the N→∞ limit, which typically impeaches ergodicity (see [34, 35] and references therein). This type of difficulty is also present, sometimes in an even more subtle manner, in various quantum systems (the single hydrogen atom constitutes, among many others, an elementary such example; indeed its BG partition function diverges due to the accumulation of electronic energy levels just below the ionization energy).
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Acknowledgements
We acknowledge useful conversations with M. Jauregui. One of us (CT) also acknowledges (recent and old) conversations with L. Bergstrom, F. Caruso, H. Casini, A. Coniglio, E.M.F. Curado, M.J. Duff, A.S. Fokas, G. ’t Hooft, F.D. Nobre, N. Pinto Neto, G. Ruiz, H. Saida, I.D. Soares, L. Thorlacius and J. Zanelli. We have benefited from partial financial support from CNPq, Faperj and Capes (Brazilian agencies).
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Tsallis, C., Cirto, L.J.L. Black hole thermodynamical entropy. Eur. Phys. J. C 73, 2487 (2013). https://doi.org/10.1140/epjc/s10052-013-2487-6
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DOI: https://doi.org/10.1140/epjc/s10052-013-2487-6