1,184 research outputs found
Higher order gravities and the Strong Equivalence Principle
We show that, in all metric theories of gravity with a general covariant
action, gravity couples to the gravitational energy-momentum tensor in the same
way it couples to the matter energy-momentum tensor order by order in the weak
field approximation around flat spacetime. We discuss the relation of this
property to the Strong Equivalence Principle. We also study the gauge
transformation properties of the gravitational energy-momentum tensor.Comment: Additional resulting the gauge transformation of the gravitational
energy-momentum tensor and references added. 18 pages, no figure
Supersymmetric solutions of 4-dimensional supergravities
We review some general and recent results on the characterization and
construction of timelike supersymmetric solutions of 4-dimensional supergravity
theories.Comment: Latex2e, 14 pages. Contribution to the Proceedings of the IV Mexican
Meeting in Mathematical and Experimental Physics held at El Colegio Nacional,
M\'exico DF. July 19th to 23rd, 201
A Note on Supersymmetric Godel Black Holes, Strings and Rings of Minimal d=5 Supergravity
We show how any asymptotically flat supersymmetric solution of minimal d=5
supergravity with flat base space can be deformed into another supersymmetric
asymptotically-Godel solution and apply this procedure to the recently found
supersymmetric black-ring and black-string solutions.Comment: 9 pages, Latex2e. Additional references include
Extremality Versus Supersymmetry in Stringy Black Holes
We study general black-hole solutions of the low-energy string effective
action in arbitrary dimensions using a general metric that can describe them
all in a unified way both in the extreme and non-extreme cases. We calculate
the mass, temperature and entropy and study which relations amongst the charges
and the mass lead to extremality. We find that the temperature always vanishes
in the extreme limit and we find that, for a set of n charges (no further
reducible by duality) there are 2^{(n-1)} combinations of the charges that
imply extremality. Not all of these combinations can be central charge
eigenvalues and, thus, there are in general extreme black holes which are not
supersymmetric (or ``BPS-saturated''). In the N=8 supergravity case we argue
that the existence of roughly as many supersymmetric and non-supersymmetric
extreme black holes suggests the existence of an underlying twelve-dimensional
structure.Comment: Latex2e file with optional macros for small versions. References to
Kutasov and Martinec's work adde
O(n,n) invariance and Wald entropy formula in the Heterotic Superstring effective action at first order in alpha'
We perform the toroidal compactification of the full Bergshoeff-de Roo
version of the Heterotic Superstring effective action to first orderin
. The dimensionally-reduced action is given in a
manifestly-O(n,n)-invariant form which we use to derive a
manifestly-O(n,n)-invariant Wald entropy formula which we then use to compute
the entropy of -corrected, 4-dimensional, 4-charge, static, extremal,
supersymmetric black holes.Comment: References and comments added. Version to be published in Journal of
High Energy Physic
Non-Supersymmetric (but) Extreme Black Holes, Scalar Hair and Other Open Problems
We give a brief overview of black-hole solutions in four-dimensional
supergravity theories and their extremal and supersymmetric limits. We also
address problems like cosmic censorship and no-hair theorems in supergravity
theories. While supergravity by itself seems not to be enough to enforce cosmic
censorship and absence of primary scalar hair, superstring theory may be.Comment: Latex file, 18 pages (or less with optional macros included) Enhanced
Version of the Contribution to the Proceedings of the XXXIII Karpacz Winter
School of Theoretical Physics Duality, Strings and Fields, 13-22 February,
Karpacz, Polan
On timelike supersymmetric solutions of gauged minimal 5-dimensional supergravity
We analyze the timelike supersymmetric solutions of minimal gauged
5-dimensional supergravity for the case in which the K\"ahler base manifold
admits a holomorphic isometry and depends on two real functions satisfying a
simple second-order differential equation. Using this general form of the base
space, the equations satisfied by the building blocks of the solutions become
of, at most, fourth degree and can be solved by simple polynomic ansatzs. In
this way we construct two 3-parameter families of solutions that contain almost
all the timelike supersymmetric solutions of this theory with one angular
momentum known so far and a few more: the (singular) supersymmetric
Reissner-Nordstr\"om-AdS solutions, the three exact supersymmetric solutions
describing the three near-horizon geometries found by Gutowski and Reall, three
1-parameter asymptotically-AdS black-hole solutions with those three
near-horizon geometries (Gutowski and Reall's black hole being one of them),
three generalizations of the G\"odel universe and a few potentially homogenous
solutions. A key r\^ole in finding these solutions is played by our ability to
write AdS's K\"ahler base space ( or
SUU) is three different, yet simple, forms associated to three
different isometries. Furthermore, our ansatz for the K\"ahler metric also
allows us to study the dimensional compactification of the theory and its
solutions in a systematic way.Comment: 57 pages. References and comments adde
T duality and Wald entropy formula in the Heterotic Superstring effective action at first order in
We consider the compactification on a circle of the Heterotic Superstring
effective action to first order in the Regge slope parameter and
re-derive the -corrected Buscher rules first found in
arXiv:hep-th/9506156 , proving the T duality invariance of the
dimensionally-reduced action to that order in . We use Iyer and Wald's
prescription to derive an entropy formula that can be applied to black-hole
solutions which can be obtained by a single non-trivial compactification on a
circle and discuss its invariance under the -corrected T duality
transformations. This formula has been successfully applied to
-corrected 4-dimensional non-extremal Reissner-Nordstr\"om black holes
in arXiv:1910.14324 and we apply it here to a heterotic version of the
Strominger-Vafa 5-dimensional extremal black hole.Comment: Version published in the journa
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