2003
DOI: 10.1103/physrevd.68.066009
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Brane classical and quantum cosmology from an effective action

Abstract: Motivated by the Randall-Sundrum brane-world scenario, we discuss the classical and quantum dynamics of a (d + 1)-dimensional boundary wall between a pair of (d + 2)-dimensional topological Schwarzschild-AdS black holes. We assume there are quite general -but not completely arbitrary -matter fields living on the boundary "brane universe" and its geometry is that of an FriedmannLemaître-Robertson-Walker (FLRW) model. The effective action governing the model in the minisuperspace approximation is derived. We fin… Show more

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Cited by 28 publications
(55 citation statements)
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References 69 publications
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“…This suggests a view that FRW models with a generalized Chaplygin gas content may enable us to investigate specific aspects within brane-worlds. E.g., the quantum cosmological creation of the universe, by means of an Hamiltonian formulation, taking into account the presence of potential symmetries and conserved charges that could be related with physical quantitites in brane-world physics [35,39,40,41,42,43,44,45].…”
Section: Neverthelessmentioning
confidence: 99%
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“…This suggests a view that FRW models with a generalized Chaplygin gas content may enable us to investigate specific aspects within brane-worlds. E.g., the quantum cosmological creation of the universe, by means of an Hamiltonian formulation, taking into account the presence of potential symmetries and conserved charges that could be related with physical quantitites in brane-world physics [35,39,40,41,42,43,44,45].…”
Section: Neverthelessmentioning
confidence: 99%
“…Ref. [35,39,40,41,42,43,44,45]) can admit a phenomenological description in terms of a generalized Chaplygin gas minisuperspace cosmology. This could be investigated by means of suitable canonical transformations at the Hamiltonian formulation.…”
Section: Neverthelessmentioning
confidence: 99%
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“…That is, in both the lmw and fsw coordinates, universes are defined simply as 4-surfaces comoving in ℓ or w. And unlike standard Schwarzschild-like coordinates, the lmw or fsw 5-metrics are regular as the universe crosses the black hole horizon(s). Such coordinates may have some utility in the study of quantized braneworld models, where the bad behaviour of coordinates across horizons apparently results in a complicated canonical phase-space description of the brane's dynamics 23 . Finally, we discuss the temptation to generalize these coordinates to other types of black holes and different dimensions.…”
Section: Summary and Discussionmentioning
confidence: 99%
“…The notations as well as the geometric construction given below accord to these given in works of Paul Wesson and Sanjeev S. Seahra (1,2,3,4,5) .…”
Section: Embedding a 4d Space-time In A 5d Manifold The Formalismmentioning
confidence: 99%