2 research outputs found
Thermodynamic instability of doubly spinning black objects
We investigate the thermodynamic stability of neutral black objects with (at
least) two angular momenta. We use the quasilocal formalism to compute the
grand canonical potential and show that the doubly spinning black ring is
thermodynamically unstable. We consider the thermodynamic instabilities of
ultra-spinning black objects and point out a subtle relation between the
microcanonical and grand canonical ensembles. We also find the location of the
black string/membrane phases of doubly spinning black objects.Comment: 25 pages, 7 figures v2: matches the published versio
Quasilocal formalism and thermodynamics of asymptotically flat black objects
We study the properties of 5-dimensional black objects by using the
renormalized boundary stress-tensor for locally asymptotically flat spacetimes.
This provides a more refined form of the quasilocal formalism which is useful
for a holographic interpretation of asymptotically flat gravity. We apply this
technique to examine the thermodynamic properties of black holes, black rings,
and black strings. The advantage of using this method is that we can go beyond
the `thin ring' approximation and compute the boundary stress tensor for any
general (thin or fat) black ring solution. We argue that the boundary stress
tensor encodes the necessarily information to distinguish between black objects
with different horizon topologies in the bulk. We also study in detail the susy
black ring and clarify the relation between the asymptotic charges and the
charges defined at the horizon. Furthermore, we obtain the balance condition
for `thin' dipole black rings.Comment: v2 clarifications on the advantage of using quasilocal formalism for
black rings added, CQG versio