Topics
viscositySoftware
magnetic fieldDisease
A possible origin of viscosity in Keplerian accretion disks due to secondary perturbation: Turbulent transport without magnetic field
Accretion disks are ubiquitous in the universe. Although difficult to observe directly, their presen...
A major uncertainty in accretion disk theory is the nature and properties of gas turbulence, which d...
After the initial stage of fast expanding of the hot Universe comes epoch of temperature fall and su...
The origin of hydrodynamic turbulence in rotating shear flow is a long standing puzzle. Resolving it...
The origin of hydrodynamic turbulence in rotating shear flow is a long standing puzzle. Resolving it...
Recently, in a series of papers, Mukhopadhyay and his collaborators have argued for possible pure hy...
Recently, in a series of papers, Mukhopadhyay and his collaborators have argued for possible pure hy...
We consider the accretion process in a disk with magnetic fields that are dragged in from the inters...
We consider the accretion process in a disk with magnetic fields that are dragged in from the inters...
Accretion disks are observed in young stars, cataclysmic variables, binary X-ray sources et al. Accr...
We use well–established observational evidence to draw conclusions about the fundamental nature of t...
We use well–established observational evidence to draw conclusions about the fundamental nature of t...
I review recent work on the radial transport of angular momentum in ionized, Keplerian accretion dis...
Origin of turbulence in cold accretion disks, particularly in 3D, which is expected to be hydrodynam...
Accretion disks are ubiquitous in the universe. Although difficult to observe directly, their presen...
Accretion disks are ubiquitous in the universe. Although difficult to observe directly, their presen...
A major uncertainty in accretion disk theory is the nature and properties of gas turbulence, which d...
After the initial stage of fast expanding of the hot Universe comes epoch of temperature fall and su...
The origin of hydrodynamic turbulence in rotating shear flow is a long standing puzzle. Resolving it...
The origin of hydrodynamic turbulence in rotating shear flow is a long standing puzzle. Resolving it...
Recently, in a series of papers, Mukhopadhyay and his collaborators have argued for possible pure hy...
Recently, in a series of papers, Mukhopadhyay and his collaborators have argued for possible pure hy...
We consider the accretion process in a disk with magnetic fields that are dragged in from the inters...
We consider the accretion process in a disk with magnetic fields that are dragged in from the inters...
Accretion disks are observed in young stars, cataclysmic variables, binary X-ray sources et al. Accr...
We use well–established observational evidence to draw conclusions about the fundamental nature of t...
We use well–established observational evidence to draw conclusions about the fundamental nature of t...
I review recent work on the radial transport of angular momentum in ionized, Keplerian accretion dis...
Origin of turbulence in cold accretion disks, particularly in 3D, which is expected to be hydrodynam...
Accretion disks are ubiquitous in the universe. Although difficult to observe directly, their presen...
Accretion disks are ubiquitous in the universe. Although difficult to observe directly, their presen...
A major uncertainty in accretion disk theory is the nature and properties of gas turbulence, which d...
After the initial stage of fast expanding of the hot Universe comes epoch of temperature fall and su...
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