Iterative Relaxation Method to Obtain Global Transonic Flows around Compact Objects
arXiv:2505.07397 · doi:10.1134/S1995080224608397
Abstract
Flows around compact objects are necessarily transonic. Due to their dissipative nature, finding of sonic points is not trivial. Becker and Le in 2003 (BL03) proposed a novel methodology to obtain global transonic solutions, using iterative relaxation technique and exploiting the inner boundary conditions of the central object. In the current work, we propose a generic methodology -- IRM-SP and IRM-SHOCK to obtain any class of global accretion and wind solutions, given a set of constants of motion. We have considered viscosity in the system, which transports angular momentum outwards. In addition, it heats the system. Radiative processes like bremsstrahlung which cools the system is also incorporated. An interplay between heating and cooling process, along with gravity and centrifugal forces gives rise to multiple sonic points and hence shocks. The proposed methodology successfully generates any class of accretion as well as wind solutions, allowing us to unify them. Additionally, we report here rigorously the mathematical as well as the computational algorithm needed, to find sonic point(s) and thus obtain global transonic flows around compact objects.
14 pages, 6 figures, accepted in LOBACHEVSKII JOURNAL OF MATHEMATICS
References in corpus (21)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- Hot Accretion Flows Around Black Holes
- First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
- Radiative Models of Sgr A* from GRMHD Simulations
- Spectrum of Optically Thin Advection Dominated Accretion Flow around a Black Hole: Application to Sgr A*
- Slim disks around Kerr black holes revisited
- Radiatively Inefficient Accretion Flow in the Nucleus of NGC 1097
- Advective Accretion Disks and Related Problems Including Magnetic Fields
- Effects of Fluid Composition on Spherical Flows around Black Holes
- Dissipative advective accretion disc solutions with variable adiabatic index around black holes
- Inner Boundary Conditions for Advection-Dominated Accretion onto Black Holes
- Two temperature solutions and emergent spectra from relativistic accretion discs around black holes
- General relativistic two-temperature accretion solutions for spherical flows around black holes
- Global Transonic Solution of Hot Accretion Flow with Thermal Conduction
- Restrictions on the Physical Prescription for the Viscosity in Advection-Dominated Accretion Disks
- Two-temperature accretion flows around strongly magnetized stars and their spectral analysis
- Carter-Penrose diagrams for emergent spacetime in axisymmetrically accreting black hole systems
- Hot accretion flow around neutron stars
- Angular momentum transport and thermal stabilization of optically thin, advective accretion flows through large-scale magnetic fields