Generalised warped disk equations

Abstract

The manner in which warps in accretion disks evolve depends on the magnitude of the viscosity. For small viscosity (α < H/R) the warp evolves in a wave-like manner; for large viscosity H/R<α 1 it evolves diffusively. Here α is the viscosity parameter and H/R the disk aspect ratio. Currently there is no simple set of equations which describes the evolution in both regimes. In this paper we describe a possible solution to this problem and introduce a set of one-dimensional equations that describe the evolution of a warped disk that are applicable in both high and low viscosity regimes for arbitrary tilts, but small warps.

0

Turn this paper into a lesson

ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…