On the role of on accretion disks
arXiv:2105.03226 · doi:10.1140/epjp/s13360-021-01455-3
Abstract
The dynamics of accretion disk is considered taking into account the Lense-Thirring precession in the presence of cosmological constant of Schwarzschild-de Sitter. The nodal and apsidal frequencies are obtained, and the role of is revealed in their properties, including the consequences for the Bardeen-Petterson effect.
arXiv comment6 pages, 1 fig., Eur. Phys. J. Plus
References in corpus (16)
- Planck 2015 results. XIII. Cosmological parameters
- Enhanced Angular Momentum Transport in Accretion Disks
- Solar system effects in Schwarzschild--de Sitter spacetime
- On the Bardeen-Petterson Effect in black hole accretion discs
- Hydrodynamic Simulations of the Bardeen-Petterson Effect
- Standard Clocks, Orbital Precession and the Cosmological Constant
- The cosmological constant derived via galaxy groups and clusters
- Two fundamental constants of gravity unifying the dark matter and the dark energy
- On the common nature of dark matter and dark energy: galaxy groups
- Porosity criterion for hyperbolic voids and the cosmic microwave background
- H_0 tension: clue to common nature of dark sector?
- Cosmological constant as a fundamental constant
- On the Lambda-evolution of galaxy clusters
- Gravity lens critical test for gravity constants and dark sector
- Lense-Thirring precession and modified gravity constraints
- Lense-Thirring precession and gravito-gyromagnetic ratio