3 research outputs found
Phase transition and scaling behavior of topological charged black holes in Horava-Lifshitz gravity
Gravity can be thought as an emergent phenomenon and it has a nice
"thermodynamic" structure. In this context, it is then possible to study the
thermodynamics without knowing the details of the underlying microscopic
degrees of freedom. Here, based on the ordinary thermodynamics, we investigate
the phase transition of the static, spherically symmetric charged black hole
solution with arbitrary scalar curvature in Ho\v{r}ava-Lifshitz gravity at
the Lifshitz point . The analysis is done using the canonical ensemble
frame work; i.e. the charge is kept fixed. We find (a) for both and
, there is no phase transition, (b) while case exhibits the second
order phase transition within the {\it physical region} of the black hole. The
critical point of second order phase transition is obtained by the divergence
of the heat capacity at constant charge. Near the critical point, we find the
various critical exponents. It is also observed that they satisfy the usual
thermodynamic scaling laws.Comment: Minor corrections, refs. added, to appear in Class. Quant. Grav.
arXiv admin note: text overlap with arXiv:1111.0973 by other author
SYK/AdS duality with Yang-Baxter deformations
In this paper, based on the notion of SYK/AdS duality we explore the effects
of Yang-Baxter (YB) deformations on the SYK spectrum at strong coupling. In the
first part of our analysis, we explore the consequences of YB deformations
through the Kaluza-Klein (KK) reduction on .
It turns out that the YB effects (on the SYK spectrum) starts showing off at
\textit{quadratic} order in expansion. For the rest of the analysis, we
provide an interpretation for the YB deformations in terms of
bi-local/collective field excitations of the SYK model. Using large
techniques, we evaluate the effective action upto quadratic order in the
fluctuations and estimate corrections to the correlation function at
strong coupling.Comment: Revised version, To Appear in JHE
