On the classical confinement of test particles to a thin 3-brane in the absence of non-gravitational forces
arXiv:0802.0939 · doi:10.1142/S0217732308027503
Abstract
The classical confinement condition of test particles to a brane universe in the absence of non-gravitational forces is transformed using the Hamilton-Jacobi formalism. The transformed condition provides a direct criterion for selecting in a cosmological scenario 5D bulk manifolds wherein it is possible to obtain confinement of trajectories to 4D hypersurfaces purely due to classical gravitational effects.
arXiv comment12 pages, version to appear in MPLA
References in corpus (21)
- Extra force in modified theories of gravity
- Application of the Campbell-Magaard theorem to higher-dimensional physics
- Causality of the brane universe
- Null Geodesics in Five Dimensional Manifolds
- Extra Force in Brane Worlds
- Classical confinement of test particles in higher-dimensional models: stability criteria and a new energy condition
- Null Geodesics in Brane World Universe
- Spacetime Measurements in Kaluza-Klein Gravity
- Five dimensional relativity and two times
- Does The Force From an Extra Dimension Contradict Physics in 4D?
- Induced Matter and Particle Motion in Non-Compact Kaluza-Klein Gravity
- Mass and Charge in Brane-World and Non-Compact Kaluza-Klein Theories in 5 Dim
- The Dynamics of Test Particles and Pointlike Gyroscopes in the Brane World and Other 5D Models
- Invariant definition of rest mass and dynamics of particles in 4D from bulk geodesics in brane-world and non-compact Kaluza-Klein theories
- Fifth force from fifth dimension: a comparison between two different approaches
- Warped product spaces and geodesic motion in the neighbourhood of hypersurfaces
- The Equivalence Principle as a Symmetry
- Geodesic motion in the neighbourhood of submanifolds embedded in warped product spaces
- On extra forces from large extra dimensions
- Equations of Motion in Kaluza-Klein Gravity Revisited
- Extra force and extra mass from noncompact Kaluza-Klein theory in a cosmological model