We formulate new general-relativistic extensions of Newtonian rotation laws for self-gravitating stationary fluids. They have been used to rederive, 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 antidragging and a new effect that measures the deviation from the Keplerian motion and/or the contribution of the fluids self-gravity. One can use the rotation laws to study the uniqueness and the convergence of the post-Newtonian approximations as well as the existence of the post-Newtonian limits
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...
We integrate numerically axially symmetric stationary Einstein equations describing self-gravitating...
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...
Recent general-relativistic extensions of Newtonian rotation laws for self-gravitating stationary fl...
We obtain rotation laws for axially symmetric, self-gravitating and stationary fluids around spinnin...
We evaluate general-relativistic effects in the motion of stationary self-gravitating accretion disk...
We obtain from the first principles a general-relativistic Keplerian rotation law for self-gravitati...
We analyse the dynamics of a single disk galaxy from a general relativistic viewpoint. We investigat...
We analyse the dynamics of a single disk galaxy from a general relativistic viewpoint. We investigat...
Praca omawia wyniki prac dotyczących praw rotacji płynów w hydrodynamice ogólnorelatywistycznej. Roz...
Galaxy rotation curves are generally analyzed theoretically using Newtonian physics; however, two gr...
The effect of post-Newtonian potentials on the rotation of a nearly rigid body is shown to consist o...
The post-Newtonian effects of general relativity on the equilibrium of uniformly rotating bodies are...
Aims. We extend the classical formulation of the dynamical friction effect on a test star by Chandra...
We obtain the relativistic rotation dynamical equations by using the Hamiltonian-Lagrangian formalis...
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...
We integrate numerically axially symmetric stationary Einstein equations describing self-gravitating...
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...
Recent general-relativistic extensions of Newtonian rotation laws for self-gravitating stationary fl...
We obtain rotation laws for axially symmetric, self-gravitating and stationary fluids around spinnin...
We evaluate general-relativistic effects in the motion of stationary self-gravitating accretion disk...
We obtain from the first principles a general-relativistic Keplerian rotation law for self-gravitati...
We analyse the dynamics of a single disk galaxy from a general relativistic viewpoint. We investigat...
We analyse the dynamics of a single disk galaxy from a general relativistic viewpoint. We investigat...
Praca omawia wyniki prac dotyczących praw rotacji płynów w hydrodynamice ogólnorelatywistycznej. Roz...
Galaxy rotation curves are generally analyzed theoretically using Newtonian physics; however, two gr...
The effect of post-Newtonian potentials on the rotation of a nearly rigid body is shown to consist o...
The post-Newtonian effects of general relativity on the equilibrium of uniformly rotating bodies are...
Aims. We extend the classical formulation of the dynamical friction effect on a test star by Chandra...
We obtain the relativistic rotation dynamical equations by using the Hamiltonian-Lagrangian formalis...
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...
We integrate numerically axially symmetric stationary Einstein equations describing self-gravitating...
We study the effects of rotation on the torsional modes of oscillating relativistic stars with a sol...