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20062010
most citedEinstein's equations as a thermodynamic identity: The cases of stationary axisymmetric horizons and evolving spherically symmetric horizons

169 citations · 479 across the 7 of their papers we have counts for

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gr-qc201031 cited

The thermodynamic structure of Einstein tensor

Dawood Kothawala

We analyze the generic structure of Einstein tensor projected onto a 2-D spacelike surface S defined by unit timelike and spacelike vectors u_i and n_i respectively, which describe…

gr-qc200988 cited

Thermodynamic structure of Lanczos-Lovelock field equations from near-horizon symmetries

Dawood Kothawala, T. Padmanabhan

It is well known that, for a wide class of spacetimes with horizons, Einstein equations near the horizon can be written as a thermodynamic identity. It is also known that the Einst…

gr-qc2008114 cited

Is gravitational entropy quantized ?

Dawood Kothawala, T. Padmanabhan, Sudipta Sarkar

In Einstein's gravity, the entropy of horizons is proportional to their area. Several arguments given in the literature suggest that, in this context, both area and entropy should…

gr-qc200751 cited

Hawking radiation as tunneling for spherically symmetric black holes: A generalized treatment

Sudipta Sarkar, Dawood Kothawala

We present a derivation of Hawking radiation through tunneling mechanism for a general class of asymptotically flat, spherically symmetric spacetimes. The tunneling rate $Γ\sim \ex…

gr-qc2006169 cited

Einstein's equations as a thermodynamic identity: The cases of stationary axisymmetric horizons and evolving spherically symmetric horizons

Dawood Kothawala, Sudipta Sarkar, T. Padmanabhan

There is an intriguing analogy between the gravitational dynamics of the horizons and thermodynamics. In case of general relativity, as well as for a wider class of Lanczos-Loveloc…