58 research outputs found
On Universality of Holographic Results for (2+1)-Dimensional CFTs on Curved Spacetimes
The behavior of holographic CFTs is constrained by the existence of a bulk
dual geometry. For example, in (2+1)-dimensional holographic CFTs living on a
static spacetime with compact spatial slices, the vacuum energy must be
nonpositive, certain averaged energy densities must be nonpositive, and the
spectrum of scalar operators is bounded from below by the Ricci scalar of the
CFT geometry. Are these results special to holographic CFTs? Here we show that
for perturbations about appropriate backgrounds, they are in fact universal to
all CFTs, as they follow from the universal behavior of two- and three-point
correlators of known operators. In the case of vacuum energy, we extend away
from the perturbative regime and make global statements about its negativity
properties on the space of spatial geometries. Finally, we comment on the
implications for dynamics which are dissipative and driven by such a vacuum
energy and we remark on similar results for the behavior of the Euclidean
partition function on deformations of flat space or the round sphere.Comment: 35+4 pages, 1 figure. v2: corrected discussion of torus to deformed
flat space; additional comments adde
Flowing Funnels: Heat sources for field theories and the AdS_3 dual of CFT_2 Hawking radiation
We construct the general 2+1 dimensional asymptotically AdS_3 solution dual
to a stationary 1+1 CFT state on a black hole background. These states involve
heat transport by the CFT between the 1+1 black hole and infinity (or between
two 1+1 black holes), and so describe the AdS dual of CFT Hawking radiation.
Although the CFT stress tensor is typically singular at the past horizon of the
1+1 black hole, the bulk 2+1-dimensional solutions are everywhere smooth, and
in fact are diffeomorphic to AdS_3. In particular, we find that Unruh states of
the CFT on any finite-temperature 1+1 black hole background are described by
extreme horizons in the bulk.Comment: 24 page
A Bound on Holographic Entanglement Entropy from Inverse Mean Curvature Flow
Entanglement entropies are notoriously difficult to compute. Large-N
strongly-coupled holographic CFTs are an important exception, where the AdS/CFT
dictionary gives the entanglement entropy of a CFT region in terms of the area
of an extremal bulk surface anchored to the AdS boundary. Using this
prescription, we show -- for quite general states of (2+1)-dimensional such
CFTs -- that the renormalized entanglement entropy of any region of the CFT is
bounded from above by a weighted local energy density. The key ingredient in
this construction is the inverse mean curvature (IMC) flow, which we suitably
generalize to flows of surfaces anchored to the AdS boundary. Our bound can
then be thought of as a "subregion" Penrose inequality in asymptotically
locally AdS spacetimes, similar to the Penrose inequalities obtained from IMC
flows in asymptotically flat spacetimes. Combining the result with positivity
of relative entropy, we argue that our bound is valid perturbatively in 1/N,
and conjecture that a restricted version of it holds in any CFT.Comment: 33+7 pages, 7 figures. v2: addressed referee comment
Complex Entangling Surfaces for AdS and Lifshitz Black Holes?
We discuss the possible relevance of complex codimension-two extremal
surfaces to the the Ryu-Takayanagi holographic entanglement proposal and its
covariant Hubeny-Rangamani-Takayanagi (HRT) generalization. Such surfaces live
in a complexified bulk spacetime defined by analytic continuation. We identify
surfaces of this type for BTZ, Schwarzschild-AdS, and Schwarzschild-Lifshitz
planar black holes. Since the dual CFT interpretation for the imaginary part of
their areas is unclear, we focus on a straw man proposal relating CFT entropy
to the real part of the area alone. For Schwarzschild-AdS and
Schwarzschild-Lifshitz, we identify families where the real part of the area
agrees with qualitative physical expectations for the appropriate CFT entropy
and, in addition, where it is smaller than the area of corresponding real
extremal surfaces. It is thus plausible that the CFT entropy is controlled by
these complex extremal surfaces.Comment: 28+5 pages. v2: Addressed referee comment
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