We evaluate general-relativistic effects in the motion of stationary self-gravitating accretion
disks around a Schwarzschild black hole, assuming the first post-Newtonian (1PN) …

We consider stationary, axially symmetric toroids rotating around spinless black holes,
assuming the general-relativistic Keplerian rotation law, in the first post-Newtonian …

We obtain a new exact solution of the 5D Einstein equations in vacuum describing a
distorted Myers-Perry black hole with a single angular momentum. Locally, the solution is …

Stationary, axisymmetric, vacuum, solutions of Einstein's equations are obtained as critical
points of the total mass among all axisymmetric and (t, ϕ) symmetric initial data with fixed …

We study two types of axially symmetric, stationary and asymptotically flat spacetimes using
highly accurate numerical methods. One type contains a black hole surrounded by a perfect …

General-relativistic models of self-gravitating tori around black holes are constructed with a
self-consistent-field method in compactified coordinates. The numerical code is highly …

Abstract Perturbations in the Main Belt Asteroids (MBAs) are the major obstacle for
achieving increased prediction accuracy in planetary ephemerides, especially for Mars, as …

We study the quasiperiodic oscillations from the accretion disk around the distorted
Schwarzschild black hole in the framework of the resonant models. We confine ourselves to …

Will, in 1974, treated the perturbation of a Schwarzschild black hole due to a slowly rotating,
light, concentric thin ring by solving the perturbation equations in terms of a multipole …

In modeling a relativistic disk around a compact object, the self-gravity of the disk is often
neglected while it needs to be incorporated for more accurate descriptions in several …