Stability of cylindrical thin shell wormhole during evolution of universe from inflation to late time acceleration
arXiv:1412.8666 · doi:10.1007/JHEP03(2015)079
Abstract
In this paper, we consider the stability of cylindrical wormholes during evolution of universe from inflation to late time acceleration epochs. We show that there are two types of cylindrical wormholes. The first type is produced at the corresponding point where k black F-strings are transited to BIon configuration. This wormhole transfers energy from extra dimensions into our universe, causes inflation, loses it's energy and vanishes. The second type of cylindrical wormhole is created by a tachyonic potential and causes a new phase of acceleration. We show that wormhole parameters grow faster than the scale factor in this era, overtake it at ripping time and lead to the destruction of universe at big rip singularity.
arXiv comment18 pages, 6 figures.v2, accepted in JHEP
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- Cylindrical Systems in General Relativity
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- Cosmology from quantum potential in brane-anti-brane system
- Stability of a -dimensional thin-shell wormhole surrounded by quintessence
- Emergence and expansion of cosmic space as due to M0-branes
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