Abstract

We propose an entropy current for dynamical black holes in a theory with arbitrary four derivative corrections to Einstein’s gravity, linearized around a stationary black hole. The Einstein-Gauss-Bonnet theory is a special case of the class of theories that we consider. Within our approximation, our construction allows us to write down a completely local version of the second law of black hole thermodynamics, in the presence of the higher derivative corrections considered here. This ultra-local, stronger form of the second law is a generalization of a weaker form, applicable to the total entropy, integrated over a compact ‘time-slice’ of the horizon, a proof of which has been recently presented in [1]. We also provide a general algorithm to construct the entropy current for the four derivative theories, which may be straightforwardly generalized to arbitrary higher deriva- tive corrections to Einstein’s gravity. This algorithm highlights the possible ambiguities in defining the entropy current.

Highlights

  • Introduction and summaryIt is widely believed that Einstein’s theory of gravity must admit an adequate UV completion when we approach length scales comparable to Planck length

  • We propose an entropy current for dynamical black holes in a theory with arbitrary four derivative corrections to Einstein’s gravity, linearized around a stationary black hole

  • The limit that we shall consider here, is the one, where the length scale associated with the curvatures of the space-time and those associated with the variations of the matter fields, are much larger compared to ls

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Summary

Introduction and summary

It is widely believed that Einstein’s theory of gravity must admit an adequate UV completion when we approach length scales comparable to Planck length. This is the central result of our note. We would like to mention that, the notion of an entropy current for black hole dynamics in higher derivative theories of gravity, is not completely new in this note. This idea has been previously introduced in [33,34,35]. Given the form of the metric (2.1), let us outline the broad strategy of the proof of second law provided in [1]

Strategy of the proof of second law of black hole thermodynamics
A residual coordinate redefinition freedom
The physical process version of first law and its implications
An entropy current for four derivative theories of gravity
Ricci scalar squared theory
Ricci scalar square theory
Ricci tensor square theory
Riemann tensor square theory
The most general structure of the ‘zero boost term’ in EvHvD
Scalar Structure
Constraints on the ‘zero boost terms’ in EvHvD
Comments on entropy current for higher boost terms in EvHvD
Discussions and future directions
A A general stationary metric can have v dependent components
All metric components are independent of τ
B Arguments leading to vanishing of Tvv on any Killing horizon
The trace of the extrinsic curvatures
Expressions of Riemann tensors and Ricci tensors off the horizon
Ricci tensor squared theory
Riemann tensor squared theory
Full Text
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