Entropy of a self-gravitating electrically charged thin shell and the black hole limit

Abstract

A static self-gravitating electrically charged spherical thin shell embedded in a (3+1)-dimensional spacetime is used to study the thermodynamic and entropic properties of the corresponding spacetime. Inside the shell, the spacetime is flat, outside it is Reissner-Nordström, and this establishes the energy density, the pressure, and the electric charge in the shell. Imposing that the shell is at a given local temperature and that the first law of thermodynamics holds on the shell one can find the integrability conditions for the temperature and for the thermodynamic electric potential, the thermodynamic equilibrium states, and the thermodynamic stability conditions. Through the integrability conditions and the first law of thermodynamics an expression for the shell's entropy can be calculated. It is found that the shell's entropy is a function of the shell's gravitational and Cauchy radii alone. A plethora of sets of temperature and electric potential equations of state can be given. One set of equations of state is related to the Hawking temperature and a precisely given electric potential. Then, as one pushes the shell to its own gravitational radius and the temperature is set precisely equal to the Hawking temperature, so that there is a finite quantum backreaction, one finds that the entropy of the shell equals the Bekenstein-Hawking entropy for a black hole. Other set of equations of state are given and the thermodynamic properties analyzed. Whatever the initial equation of state for the temperature, as the shell radius approaches its own gravitational radius, the quantum backreaction imposes the Hawking temperature for the shell in this limit. Thus, when the shell's radius is sent to the shell's own gravitational radius the formalism developed allows to find the precise form of the Bekenstein-Hawking entropy of the correlated black hole.

arXiv comment15 pages, no figures, minor changes

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• An Entropy-Area Law for Neutron Stars Near the Black Hole Threshold
• Entropy of extremal black holes: horizon limits through charged thin shells, a unified approach
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• All fundamental electrically charged thin shells in general relativity: From star shells to tension shell black holes and regular black holes and beyond
• Thermodynamics of extremal rotating thin shells in an extremal BTZ spacetime and the extremal black hole entropy
• Thermodynamics and entropy of self-gravitating matter shells and black holes in $d$ dimensions
• Compact objects in general relativity: From Buchdahl stars to quasiblack holes
• Electrically charged spherical matter shells in higher dimensions: Entropy, thermodynamic stability, and the black hole limit
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• Classical and Quantum Thermodynamic Systems in Curved Spacetime
• The canonical ensemble of a self-gravitating matter thin shell in AdS
• Thermodynamical and dynamical stability of Einstein-Maxwell and extremal Einstein-Born-Infeld thin shells in $(2+1)$ dimensions
• Thermodynamics of spherically symmetric thin-shell spacetimes