Energy conditions for a wormhole at the center
arXiv:1905.00296 · doi:10.1103/PhysRevD.100.084008
Abstract
Within general relativity, we determine the energy conditions needed for the existence of a toroidal wormhole. For this purpose, we employ the conditions of the positiveness of the second derivatives of the relevant components of the metric, which describe an increase in the linear sizes (or the area) of the cross section of the throat. The corresponding inequalities for the central energy density and pressures of the matter and for the metric are obtained.
9 pages
References in corpus (13)
- Wormhole geometries in f(R) modified theories of gravity
- Modified-gravity wormholes without exotic matter
- Wormholes in Dilatonic Einstein-Gauss-Bonnet Theory
- Stable Lorentzian Wormholes in Dilatonic Einstein-Gauss-Bonnet Theory
- Warp drive basics
- Wormhole throats in gravity
- Cylindrical wormholes
- Rotating Ellis Wormholes in Four Dimensions
- Geometry of Spinning Ellis Wormholes
- Rotating cylindrical wormholes
- Slowly rotating scalar field wormholes: the second order approximation
- Potentially observable cylindrical wormholes without exotic matter in general relativity
- Thin-shell toroidal wormhole