Moving Domain Walls in and Graceful Exit from Inflation
arXiv:hep-th/0005013 · doi:10.1016/S0370-2693(00)00668-7
Abstract
We consider moving-brane-solutions in AdS type back ground. In the first Randall-Sundrum configuration, there are two branes at fixed points of the orbifold symmetry. We point out that if one brane is fixed and the other brane is moving, the configuration is still a solution provided the moving brane has a specific velocity determined by its tension and bulk cosmological constant. In the absence of the symmetry, we can construct multi-brane configurations by patching AdS-Schwarzshild solutions. In this case, we show that the 4-dimensional effective cosmological constant on the brane world is not well defined. We find a condition for a brane to be stationary. Using the brane scattering, we suggest a scenario of inflation on the brane universe during a finite time, i.e, a scenario of a graceful exit of inflation.
10 pages, figure included, reference added
References in corpus (4)
Cited by in corpus (16)
- The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang
- Radion Dynamics and Electroweak Physics
- D-branes in Standard Model building, Gravity and Cosmology
- Brane-World Cosmology of Modulus Stabilization with a Bulk Scalar Field
- The radion in brane cosmology
- Kasner-AdS spacetime and anisotropic brane-world cosmology
- Dynamics of false vacuum bubbles with nonminimal coupling
- Brane inflation in tachyonic and non-tachyonic type 0B string theories
- Domain wall cosmology and multiple accelerations
- Time Evolution of Entanglement Entropy in Holographic FLRW Cosmologies
- Time-dependent quantum correlations in two-dimensional expanding spacetime
- Holographic time-dependent entanglement entropy in -brane gas geometries
- New Perspectives on Moving Domain Walls in (A)dS_(5) Space
- Holographic entanglement entropy and complexity for the cosmological braneworld model
- Correlation functions in expanding universes
- Entanglement Entropy and Complexity of Multicomponent Universe from Holography