Stationary cylindrical anisotropic fluid and new purely magnetic GR solutions
arXiv:2004.02636 · doi:10.1103/PhysRevD.102.044026
Abstract
The properties of interior spacetimes sourced by stationary cylindrical anisotropic fluids are here analytically studied for both nonrigid and rigid rotation. As regards nonrigid rotation, this is, to our knowledge, the first work dedicated to such a study. We give here a complete equation set describing these spacetime properties. In particular, we focus our attention on both nonrigid and rigid rotation gravito-electromagnetic features and are thus led to display strong hints in favor of conjecturing purely electric Weyl tensor existence in this framework. We have also been able to characterize new purely magnetic physically consistent spacetimes and have found new rigidly rotating exact solution classes to the five Einstein's field equations pertaining to the issue and the two purely magnetic constraints we have derived for this purpose. This should be considered as a prominent result, since extremely few purely magnetic exact solutions are available in the literature.
26 pages, 0 figure
References in corpus (2)
Cited by in corpus (6)
- New classes of exact interior nonvacuum solutions to the GR field equations for spacetimes sourced by a rigidly rotating stationary cylindrical anisotropic fluid
- Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. 5. Dust limit and discussion
- Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. 4. Radial pressure
- Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids
- Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids: anisotropic pressure
- Non-rigidly rotating stationary cylindrical dust spacetimes