activity
20102017
most citedDissipation, Energy Transfer, and Spindown Luminosity in 2.5D PIC Simulations of the Pulsar Magnetosphere

62 citations · 373 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2015★ 18 cited

The Properties of G-modes in Layered Semi-Convection

Mikhail Belyaev, Eliot Quataert, Jim Fuller

We study low frequency waves that propagate in a region of layered semi-convection. Layered semi-convection is predicted to be present in stellar and planetary interiors and can si…

astro-ph.SR2013★ 24 cited

Angular Momentum Transport by Acoustic Modes Generated in the Boundary Layer II: MHD Simulations

Mikhail A. Belyaev, Roman R. Rafikov, James. M. Stone

We perform global unstratified 3D magnetohydrodynamic simulations of an astrophysical boundary layer (BL) -- an interface region between an accretion disk and a weakly magnetized a…

astro-ph.SR2012★ 53 cited

Angular Momentum Transport by Acoustic Modes Generated in the Boundary Layer I: Hydrodynamical Theory and Simulations

Mikhail A. Belyaev, Roman R. Rafikov, James M. Stone

The nature of angular momentum transport in the boundary layers of accretion disks has been one of the central and long-standing issues of accretion disk theory. In this work we de…

astro-ph.SR2012★ 30 cited

Angular Momentum Transport and Variability in Boundary Layers of Accretion Disks Driven by Global Acoustic Modes

Mikhail A. Belyaev, Roman R. Rafikov, James M. Stone

Disk accretion onto a weakly magnetized central object, e.g. a star, is inevitably accompanied by the formation of a boundary layer near the surface, in which matter slows down fro…

astro-ph.SR2011★ 37 cited

Supersonic Shear Instabilities in Astrophysical Boundary Layers

Mikhail Belyaev, Roman Rafikov

Disk accretion onto weakly magnetized astrophysical objects often proceeds via a boundary layer that forms near the object's surface, in which the rotation speed of the accreted ga…