15 research outputs found
Construction of Einstein-Sasaki metrics in D ≥ 7
We construct explicit Einstein-Kahler metrics in all even dimensions D=2n+4
\ge 6, in terms of a -dimensional Einstein-Kahler base metric. These are
cohomogeneity 2 metrics which have the new feature of including a NUT-type
parameter, in addition to mass and rotation parameters. Using a canonical
construction, these metrics all yield Einstein-Sasaki metrics in dimensions
D=2n+5 \ge 7. As is commonly the case in this type of construction, for
suitable choices of the free parameters the Einstein-Sasaki metrics can extend
smoothly onto complete and non-singular manifolds, even though the underlying
Einstein-Kahler metric has conical singularities. We discuss some explicit
examples in the case of seven-dimensional Einstein-Sasaki spaces. These new
spaces can provide supersymmetric backgrounds in M-theory, which play a role in
the AdS_4/CFT_3 correspondence.Comment: Latex, 18 pages, 2 figures, minor typos correcte
General Kerr-NUT-AdS Metrics in All Dimensions
The Kerr-AdS metric in dimension D has cohomogeneity [D/2]; the metric
components depend on the radial coordinate r and [D/2] latitude variables \mu_i
that are subject to the constraint \sum_i \mu_i^2=1. We find a coordinate
reparameterisation in which the \mu_i variables are replaced by [D/2]-1
unconstrained coordinates y_\alpha, and having the remarkable property that the
Kerr-AdS metric becomes diagonal in the coordinate differentials dy_\alpha. The
coordinates r and y_\alpha now appear in a very symmetrical way in the metric,
leading to an immediate generalisation in which we can introduce [D/2]-1 NUT
parameters. We find that (D-5)/2 are non-trivial in odd dimensions, whilst
(D-2)/2 are non-trivial in even dimensions. This gives the most general
Kerr-NUT-AdS metric in dimensions. We find that in all dimensions D\ge4
there exist discrete symmetries that involve inverting a rotation parameter
through the AdS radius. These symmetries imply that Kerr-NUT-AdS metrics with
over-rotating parameters are equivalent to under-rotating metrics. We also
consider the BPS limit of the Kerr-NUT-AdS metrics, and thereby obtain, in odd
dimensions and after Euclideanisation, new families of Einstein-Sasaki metrics.Comment: Latex, 24 pages, minor typos correcte
AdS and Lifshitz Black Holes in Conformal and Einstein-Weyl Gravities
We study black hole solutions in extended gravities with higher-order
curvature terms, including conformal and Einstein-Weyl gravities. In addition
to the usual AdS vacuum, the theories admit Lifshitz and Schr\"odinger vacua.
The AdS black hole in conformal gravity contains an additional parameter over
and above the mass, which may be interpreted as a massive spin-2 hair. By
considering the first law of thermodynamics, we find that it is necessary to
introduce an associated additional intensive/extensive pair of thermodynamic
quantities. We also obtain new Liftshitz black holes in conformal gravity and
study their thermodynamics. We use a numerical approach to demonstrate that AdS
black holes beyond the Schwarzschild-AdS solution exist in Einstein-Weyl
gravity. We also demonstrate the existence of asymptotically Lifshitz black
holes in Einstein-Weyl gravity. The Lifshitz black holes arise at the boundary
of the parameter ranges for the AdS black holes. Outside the range, the
solutions develop naked singularities. The asymptotically AdS and Lifshitz
black holes provide an interesting phase transition, in the corresponding
boundary field theory, from a relativistic Lorentzian system to a
non-relativistic Lifshitz system.Comment: typos corrected, references adde
A Note on Einstein Sasaki Metrics in D \ge 7
In this paper, we obtain new non-singular Einstein-Sasaki spaces in
dimensions D\ge 7. The local construction involves taking a circle bundle over
a (D-1)-dimensional Einstein-Kahler metric that is itself constructed as a
complex line bundle over a product of Einstein-Kahler spaces. In general the
resulting Einstein-Sasaki spaces are singular, but if parameters in the local
solutions satisfy appropriate rationality conditions, the metrics extend
smoothly onto complete and non-singular compact manifolds.Comment: Latex, 13 page
AdS in Warped Spacetimes
We obtain a large class of AdS spacetimes warped with certain internal spaces
in eleven-dimensional and type IIA/IIB supergravities. The warp factors depend
only on the internal coordinates. These solutions arise as the near-horizon
geometries of more general semi-localised multi-intersections of -branes. We
achieve this by noting that any sphere (or AdS spacetime) of dimension greater
than 3 can be viewed as a foliation involving S^3 (or AdS_3). Then the S^3 (or
AdS_3) can be replaced by a three-dimensional lens space (or a BTZ black hole),
which arises naturally from the introduction of a NUT (or a pp-wave) to the
M-branes or the D3-brane. We then obtain multi-intersections by performing a
Kaluza-Klein reduction or Hopf T-duality transformation on the fibre coordinate
of the lens space (or the BTZ black hole). These geometries provide further
possible examples of the AdS/CFT correspondence and of consistent embeddings of
lower-dimensional gauged supergravities in D=11 or D=10.Comment: Latex file, 26 pages, reference adde
A New Construction of Einstein-Sasaki Metrics in D >= 7
We construct explicit Einstein-Kahler metrics in all even dimensions D=2n+4 \ge 6, in terms of a -dimensional Einstein-Kahler base metric. These are cohomogeneity 2 metrics which have the new feature of including a NUT-type parameter, in addition to mass and rotation parameters. Using a canonical construction, these metrics all yield Einstein-Sasaki metrics in dimensions D=2n+5 \ge 7. As is commonly the case in this type of construction, for suitable choices of the free parameters the Einstein-Sasaki metrics can extend smoothly onto complete and non-singular manifolds, even though the underlying Einstein-Kahler metric has conical singularities. We discuss some explicit examples in the case of seven-dimensional Einstein-Sasaki spaces. These new spaces can provide supersymmetric backgrounds in M-theory, which play a role in the AdS_7/CFT_6 correspondence
Resolved Calabi-Yau Cones and Flows from L abc Superconformal Field Theories
We discuss D3-branes on cohomogeneity-three resolved Calabi-Yau cones over Labc spaces, for which a 2-cycle or 4-cycle has been blown up. In terms of the dual quiver gauge theory, this corresponds to motion along the non-mesonic, or baryonic, directions in the moduli space of vacua. In particular, a dimension-two and/or dimensionsix scalar operator gets a vacuum expectation value. These resolved cones support various harmonic (2, 1)-forms which reduce the ranks of some of the gauge groups either by a Seiberg duality cascade or by Higgsing. We also discuss higher-dimensional resolved Calabi-Yau cones. In particular, we obtain square-integrable (2, 2)-forms for eight-dimensional cohomogeneity-four Calabi-Yau metrics