General-relativistic rotation laws in rotating fluid bodies
arXiv:1501.04539 · doi:10.1103/PhysRevD.91.124053
Abstract
We formulate new general-relativistic extensions of Newtonian rotation laws for self-gravitating stationary fluids. They have been used to re-derive, in the first post-Newtonian approximation, the well known geometric dragging of frames. We derive two other general-relativistic weak-field effects within rotating tori: the recently discovered dynamic anti-dragging and a new effect that measures the deviation from the Keplerian motion and/or the contribution of the fluids selfgravity. One can use the rotation laws to study the uniqueness and the convergence of the post-Newtonian approximations, and the existence of the post-Newtonian limits.
5 pages, to appear in the Physical Review D
References in corpus (1)
Cited by in corpus (10)
- Modeling differential rotations of compact stars in equilibriums
- Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles
- Self-gravitating magnetised tori around black holes in general relativity
- Rotating systems, universal features in dragging and anti-dragging effects, and bounds onto angular momentum
- Relativistic effects cannot explain galactic dynamics
- Toroidal magnetic fields in self-gravitating disks around black holes
- Modelling general-relativistic disk in OJ 287
- Stationary massive disks around black holes: realistic equation of state and bifurcation
- On extensions of the Penrose inequality with angular momentum
- Oscillation properties of relativistic tori in the vicinity of a distorted deformed compact object