Wormhole solution in modified teleparallel-Rastall gravity and energy conditions
arXiv:2302.07107 · doi:10.1007/s10714-023-03093-9
Abstract
The possibility of static and spherically symmetric traversable wormhole solution in modified teleparallel Rastall gravity (MTRG) in a non-diagonal tetrad is investigated. Rastall assumption modifies the field equations and energy-momentum conservation law. These modifications lead to different exact asymptotically flat traversable wormhole solutions. By imposing different constraints on modified energy-momentum conservation law, different exact solutions are found and the obtained results for teleparallel Rastall gravity (TRG), with specific choices of , are studied. It is shown that the Rastall parameters have a key role in these models and in all of those exact traversable wormhole solutions the null energy condition (NEC) and weak energy condition (WEC) of matter or energy which has surrounded the wormhole are valid at the throat of the wormhole and through the space time as well.
10 pages, 3 figures, submitted version
References in corpus (14)
- Dynamics of dark energy
- f(R,T) gravity
- f(R,L_m) gravity
- Wormhole geometries in f(R) modified theories of gravity
- Generalized curvature-matter couplings in modified gravity
- Wormhole geometries supported by a nonminimal curvature-matter coupling
- Nonminimal curvature-matter coupled wormholes with matter satisfying the null energy condition
- Plane symmetric thin-shell wormholes: solutions and stability
- A general class of braneworld wormholes
- Cylindrical wormholes
- Evolving Lorentzian wormholes supported by phantom matter and cosmological constant
- Wormhole with varying cosmological constant
- Wormhole on DGP brane
- Wormhole and its Analogue in Brane World