Criticality and surface tension in rotating horizon thermodynamics

@article{Hansen2016CriticalityAS,
  title={Criticality and surface tension in rotating horizon thermodynamics},
  author={Devin Hansen and David Kubizň{\'a}k and Robert B. Mann},
  journal={Classical and Quantum Gravity},
  year={2016},
  volume={33}
}
We study a modified horizon thermodynamics and the associated criticality for rotating black hole spacetimes. Namely, we show that under a virtual displacement of the black hole horizon accompanied by an independent variation of the rotation parameter, the radial Einstein equation takes a form of a ‘cohomogeneity two’ horizon first law, δ E = T δ S + Ω δ J − σ δ A , where E and J are the horizon energy (an analogue of the Misner–Sharp mass) and the horizon angular momentum, Ω is the horizon… 

Universality of P − V criticality in horizon thermodynamics

A bstractWe study P − V criticality of black holes in Lovelock gravities in the context of horizon thermodynamics. The corresponding first law of horizon thermodynamics emerges as one of the

Modifying horizon thermodynamics by surface tensions

The modified first laws of thermodynamics at the black hole horizon and the cosmological horizon of the Schwarzschild de Sitter black hole and the apparent horizon of the Friedmann-Robertson-Walker

Thermodynamic Property of Schwarzschild Black Hole in Non-Commutative Gauge Theory of Gravity

: In this paper, we constructed the deformed Schwarzschild black hole in the non-commutative (NC) gauge theory of gravity. Where the singularity at the origin is shifted by the non-commutativity to

On Modified First Law of Black hole Thermodynamics in The Non-Commutative Gauge Theory

In this paper, we investigated the thermodynamic properties of Schwarzschild black hole (SBH) in the non-commutative (NC) gauge theory of gravity. According to our previous work, we modify the first

Surface tensions in horizon thermodynamics of Anti-de Sitter and de Sitter spacetimes

Adopting the surface tensions, we review the horizon thermodynamics of a Reissner-Nordstrom Anti-de Sitter black hole and a pure de Sitter spacetime. The modified first laws, which obeys the

Thermodynamic Properties of Schwarzschild Black Hole in Non-Commutative Gauge Theory of Gravity

: In this paper, we used the non-commutative (NC) gauge theory of gravity to investigate the thermodynamic properties of a deformed Schwarzschild black hole (SBH). Our results present a new scenario

Black hole chemistry: thermodynamics with Lambda

We review recent developments on the thermodynamics of black holes in extended phase space, where the cosmological constant is interpreted as thermodynamic pressure and treated as a thermodynamic

References

SHOWING 1-10 OF 18 REFERENCES

Universality of P − V criticality in horizon thermodynamics

A bstractWe study P − V criticality of black holes in Lovelock gravities in the context of horizon thermodynamics. The corresponding first law of horizon thermodynamics emerges as one of the

Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes

A general formalism for understanding the thermodynamics of horizons in spherically symmetric spacetimes is developed. The formalism reproduces known results in the case of black-hole spacetimes and

Enthalpy and the mechanics of AdS black holes

We present geometric derivations of the Smarr formula for static AdS black holes and an expanded first law that includes variations in the cosmological constant. These two results are further related

Stability of black holes based on horizon thermodynamics

Black-hole thermodynamics and the Euclidean Einstein action.

  • York
  • Physics
    Physical review. D, Particles and fields
  • 1986
TLDR
It is shown that the canonical ensemble with elements of radius r and temperature T(r) for hot gravity with black holes is well defined and the direct nucleation of black holes from hot flat space can be given a thermodynamically consistent description.

Connections between gravitational dynamics and thermodynamics

We have briefly summarized three aspects of connections between gravitational dynamics and thermodynamics by focusing on three kinds of spacetime horizon: Causal Rindler horizon of spacetime, black

Thermodynamical Aspects of Gravity: New insights

The fact that one can associate thermodynamic properties with horizons brings together principles of quantum theory, gravitation and thermodynamics and possibly offers a window to the nature of

Thermodynamical interpretation of the geometrical variables associated with null surfaces

The emergent gravity paradigm interprets gravitational field equations as describing the thermodynamic limit of the underlying statistical mechanics of microscopic degrees of freedom of the

Dirty black holes: Symmetries at stationary nonstatic horizons

We establish that the Einstein tensor takes on a highly symmetric form near the Killing horizon of any stationary but non-static (and non-extremal) black hole spacetime. [This follows up on a recent