The Finslerian wormhole models
arXiv:1607.04329 · doi:10.1140/epjc/s10052-016-4066-0
Abstract
We present models of wormhole under the Finslerian structure of spacetime. This is a sequel of our previous work (Eur Phys J 75:564, 2015) where we constructed a toy model for compact stars based on the Finslerian spacetime geometry. In the present investigation, a wide variety of solutions are obtained that explore wormhole geometry by considering different choices for the form function and energy density. The solutions, like the previous work, are revealed to be physically interesting and viable models for the explanation of wormholes as far as the background theory and literature are concerned.
9 pages and 7 figues
References in corpus (7)
- Modified Newton's gravity in Finsler Space as a possible alternative to dark matter hypothesis
- Wormhole with varying cosmological constant
- Modified Friedmann model in Randers-Finsler space of approximate Berwald type as a possible alternative to dark energy hypothesis
- A class of solutions for anisotropic stars admitting conformal motion
- Classical kinematics and Finsler structures for nonminimal Lorentz-violating fermions
- Cyclic and Ekpyrotic Universes in Modified Finsler Osculating Gravity on Tangent Lorentz Bundles
- Critical Remarks on Finsler Modifications of Gravity and Cosmology by Zhe Chang and Xin Li
Cited by in corpus (9)
- Traversable Wormholes Supported by GUP Corrected Casimir Energy
- Traversable Wormholes in Gravity
- Non violation of energy conditions in wormholes modelling
- Gravitational lensing effect in traversable wormholes
- Traversable wormhole models in gravity
- Weak deflection angle by Casimir wormhole using Gauss-bonnet theorem and its shadow
- Investigating the Physical Properties of Traversable Wormholes in the Modified Gravity
- On axiomatic formulation of gravity and matter field theories with MDRs and Finsler-Lagrange-Hamilton geometry on (co)tangent Lorentz bundles
- Casimir Wormholes in Brans-Dicke Theory