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(anti-)de Sitter space

Renormalized black hole entropy in anti-de Sitter space via the "brick wall" method

Renormalized black hole entropy in anti-de Sitter space via the "brick wall" method

... hole space-times, so that the integrals can be performed ...Schwarzschild-anti-de Sitter and extremal Reissner- Nordstr¨om-anti-de Sitter black holes, and, for simplicity, a massless ...

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On the existence of conformally coupled scalar field hair for black holes in (anti-)de Sitter space

On the existence of conformally coupled scalar field hair for black holes in (anti-)de Sitter space

... We note, to end this section, that the proof also does not extend to the case where Λ < 0. In this situation, in the absence of a cosmological event horizon, we would integrate from the black hole event horizon out to ...

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Quantum corrections in thermal states of fermions on anti-de Sitter space-time

Quantum corrections in thermal states of fermions on anti-de Sitter space-time

... anti-de Sitter space-times using relativistic kinetic ...Minkowski space-time, the renormalized vacuum expectation value of the stress-energy tensor is by definition zero, while on ...

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Renormalised fermion vacuum expectation values on anti-de Sitter space-time

Renormalised fermion vacuum expectation values on anti-de Sitter space-time

... anti-de Sitter space–time (adS) has been of particular interest since the formulation of the adS/CFT (conformal field theory) correspondence (see [1] for a ...curved space– time, an object of ...

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Abundant Stable Gauge Field Hair for Black Holes in Anti–de Sitter Space

Abundant Stable Gauge Field Hair for Black Holes in Anti–de Sitter Space

... anti-de Sitter space (adS) [3, 4]) have, at least to date, been described by only a small number of parameters additional to the mass, angular momentum and charge of the black ...

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Vacuum for a massless quantum scalar field outside a collapsing shell in anti-de Sitter space-time

Vacuum for a massless quantum scalar field outside a collapsing shell in anti-de Sitter space-time

... collapse of a thin shell of matter in anti-de Sitter space-time. This scenario has been studied by a number of authors (see, for example, [22,23,24,25]), largely (but not exclusively) from the point ...

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Soliton and black hole solutions of SU(N) Einstein Yang Mills theory in anti de Sitter space

Soliton and black hole solutions of SU(N) Einstein Yang Mills theory in anti de Sitter space

... We present new soliton and hairy black hole solutions of su (N) Einstein-Yang-Mills theory in asymptotically anti-de Sitter space. These solutions are described by N +1 independent parameters, and ...

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Soliton and black hole solutions of su(N) Einstein-Yang-Mills theory in anti-de Sitter space

Soliton and black hole solutions of su(N) Einstein-Yang-Mills theory in anti-de Sitter space

... We present new soliton and hairy black hole solutions of su (N) Einstein-Yang-Mills theory in asymptotically anti-de Sitter space. These solutions are described by N +1 independent parameters, and ...

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Some Results on the Differential Geometry of Spacelike Curves in De Sitter Space

Some Results on the Differential Geometry of Spacelike Curves in De Sitter Space

... The differential geometry of curves on a hypersphere in the Euclidean space reflects instantaneous properties of sphere- cal motion. In this work, we give some results for differential geometry of spacelike curves ...

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Mode-sum construction of the covariant graiviton two-point function in the Poincaré patch of de Sitter space

Mode-sum construction of the covariant graiviton two-point function in the Poincaré patch of de Sitter space

... the de Sitter-noninvariant one when smeared with transverse-traceless tensors of com- pact support [38], in order to extract the gauge-invariant content ...a de Sitter-invariant state for ...

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11. On space like submanifolds with $R=aH+b$ in de Sitter space form $S_p^{n+p}(c)$

11. On space like submanifolds with $R=aH+b$ in de Sitter space form $S_p^{n+p}(c)$

... in de Sitter space have been published. For the study of space- like hypersurface with constant scalar curvature in de Sitter space, there are also many results such as ...

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Compact space like hypersurfaces in de Sitter space

Compact space like hypersurfaces in de Sitter space

... mean curvature H must be totally umbilical, which turned out to be false in this original statement, an important number of authors have considered the problem of character- izing the totally umbilical space-like ...

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Massless Interacting Scalar Fields in de Sitter space

Massless Interacting Scalar Fields in de Sitter space

... Euclidean de Sitter space, paying particular attention to the IR problems that appear for massless and light ...becomes de Sitter ...

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A New Characterization of Totally Umbilical Hypersurfaces in de Sitter Space

A New Characterization of Totally Umbilical Hypersurfaces in de Sitter Space

... S + should be the totally umbilical ones. This conjecture motivated the work of an important number of authors who considered the problem of characterizing the totally umbilical spacelike hypersurfaces of de ...

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D branes in anti de Sitter space

D branes in anti de Sitter space

... Despite this success, most of the checks on the string theory side were done in the supergravity approximation due to the difficulty of including Ramond-Ramond (RR) fields in string theory computations. Recently, it has ...

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Thermal expectation values of fermions on anti-de Sitter space-time

Thermal expectation values of fermions on anti-de Sitter space-time

... adS space-time. The maximal symmetry of the space-time enables us to derive a closed-form expression for the bispinor of parallel transport, which, when combined with the imaginary time anti-periodicity ...

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Euler-Lagrange equations for high energy actions in QCD and in gravity

Euler-Lagrange equations for high energy actions in QCD and in gravity

... other gauge models in terms of the effective degrees of freedom corresponding to the reggeized glu- ons. The gluon Regge trajectory and various reggeon couplings in upper orders of perturbation theory can be calculated ...

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On the linear stability of solitons and hairy black holes with a negative cosmological constant: the odd-parity sector

On the linear stability of solitons and hairy black holes with a negative cosmological constant: the odd-parity sector

... flat space sphaleron is most ...flat space has shown that all the modes of instability are contained within the spherically symmetric perturbations ...flat space sphalerons, where the only modes of ...

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Novel Bianchi VII Space Times and Their Properties

Novel Bianchi VII Space Times and Their Properties

... dimensional space time along with matter density and electromagnetic flux using a method similar to Majumdar-Papapetrou way of constructing extremal ...VII space-times for their relations with condensed ...

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Dirac Fermions on an Anti-de Sitter Background

Dirac Fermions on an Anti-de Sitter Background

... In this paper, we considered quantum states of fermions of arbitrary mass in anti-de Sitter space (adS) as seen by an observer rotating with a constant angular velocity Ω . In the non-rotating case ( ...

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