Abstract
Classical general relativity allows for compact objects—“monsters”—with more entropy than black holes of equal mass. We construct examples of such configurations and describe their general properties. Monsters are problematic for certain versions of the AdS/CFT duality, and possibly even for the application of statistical mechanics to quantum gravity. It is possible that they are somehow excluded from the Hilbert space of quantum gravity, although this would be in contrast to the usual case in which coarse-grained, semiclassical configurations have (many) quantum counterparts.
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Notes
- 1.
Note, we need to restrict the size of the object as well as its total energy. An object with fixed total energy \(E = T^4 R^3\), but no restriction on \(R\), can have infinite entropy: we can take \(R\rightarrow \infty \) and \(T\rightarrow 0\) with \(E\) fixed, so that \(S = T^3 R^3 = E / T \rightarrow \infty \).
- 2.
Of course, it is also possible that the initial pure state is atypical and subsequent dynamics somehow keeps the state in a very atypical region of the Hilbert space over very long time scales, so that the highly entropic configurations are essentially never sampled. In that case one cannot deduce the thermodynamic properties of the system from the concentration of measure phenomenon (i.e., typicality) alone: the system does not actually reach ultimate equilibrium.
References
Marolf, D.: Gen. Rel. Grav. 41, 903 (2009). arXiv:0810.4886 [gr-qc]
Hossenfelder, S., Smolin, l.: Phys. Rev. D 81, 064009 (2010). arXiv:0901.3156 [gr-qc]
Strominger, A., Vafa, C.: Phys. Lett. B 379, 99 (1996)
Maldacena, J.M., Strominger, A., Witten, E.: JHEP 12, 002 (1997)
Hawking, S.W.: Commun. Math. Phys. 43, 199 (1975)
Bekenstein, J.D.: Phys. Rev. D 7, 2333 (1973)
Jacobson, T. arXiv:gr-qc/9908031
Hooft, G.’t.: In:Ali et al. (eds.) Salamfestschrift. World Scientific (1994)
Thorne, K.S.: In: Klauder, J.R. (eds.) Magic Without Magic. Freeman (1973)
Eardley, D.M., Giddings, S.B.: Phys. Rev. D 66, 044011 (2002)
Hsu, S.D.H.: Phys. Lett. B 555, 92 (2003)
Hawking, S.W.: Phys. Rev. D 14, 2460 (1976)
Hsu, S.D.H.: Phys. Lett. B 644, 67 (2007)
Hsu, S.D.H. arXiv:gr-qc/9801106
Sorkin, R.D., Wald, R.M., Zhang, Z.J.: Gen. Rel. Grav. 13, 1127 (1981)
Hsu, S.D.H., Reeb, D.: Phys. Lett. B 658, 244 (2008)
Aharony, O., Gubser, S.S., Maldacena, J.M., Ooguri, H., Oz, Y.: Phys. Rept. 323, 183 (2000)
Bousso, R.: JHEP 07, 004 (1999)
Flanagan, E.E., Marolf, D., Wald, R.M.: Phys. Rev. D 62, 084035 (2000)
Hsu, S.D.H., Reeb, D.: Class. Quant. Grav. 25, 235007 (2008)
Popescu, S., Short, A.J., Winter, A.: Nat. Phys. 2, 754 (2006). See also. arXiv:quant-ph/0511225
Gemmer, J., Michel, M., Mahler, G.: Quantum Thermodynamics: Emergence of Thermodynamic Behavior Within Composite Quantum Systems, Springer, Berlin (2004)
Ledoux, M.: The Concentration of Measure Phenomenon. American Mathematical Society, Providence (2001)
Linden, N., Popescu, S., Short, A.J., Winter, A. arXiv:0812.2385 [quant-ph]
Hayden, P., Leung, D.W., Winter, A.: Comm. Math. Phys. 265, 95 (2006)
Misner, C.W., Thorne, K.S., Wheeler, J. A.: Gravitation. Freeman (1973)
Kiefer, C.: Quantum Gravity, 2nd edn. Oxford University Press, Oxford (2007)
Acknowledgments
The author acknowledges support from the Office of the Vice-President for Research and Graduate Studies at Michigan State University.
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Hsu, S.D.H. (2015). Monsters, Black Holes and Entropy. In: Calmet, X. (eds) Quantum Aspects of Black Holes. Fundamental Theories of Physics, vol 178. Springer, Cham. https://doi.org/10.1007/978-3-319-10852-0_4
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