Rotating cosmological cylindrical wormholes in GR and TEGR sourced by anisotropic fluids
arXiv:2012.03431 · doi:10.1016/j.dark.2021.100802
Abstract
Given an anisotropic fluid source, we determine in closed forms, upon solving the field equations of general relativity (GR) and teleparallel gravity (TEGR) coupled to a cosmological constant, cylindrically symmetric four-dimensional cosmological rotating wormholes, satisfying all local energy conditions, and cosmological rotating solutions with two axes of symmetry at finite proper distance. These solutions have the property that their angular velocity is proportional to the cosmological constant.
arXiv comment8 twocolumn pages, 2 figures, references added. Extended version
References in corpus (16)
- f(T) teleparallel gravity and cosmology
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- The teleparallel equivalent of general relativity
- The covariant formulation of f(T) gravity
- Spin Connection and Renormalization of Teleparallel Action
- Rotating cylindrical wormholes
- Localization of Energy in General Relativity
- General relativity on a null surface: Hamiltonian formulation in the teleparallel geometry
- Confined-exotic-matter wormholes with no gluing effects -- Imaging supermassive wormholes and black holes
- On the parameters of Lewis metric for the Weyl class
- Search for wormhole candidates in active galactic nuclei: radiation from colliding accreting flows
- Hollow cosmic string: the general-relativistic hollow cylinder
- Spin-spin interaction in general relativity and induced geometries with nontrivial topology
- On rigidly rotating perfect fluid cylinders
- Rotating cylinders with anisotropic fluids in general relativity