- PII
- S30345170S0004629925060027-1
- DOI
- 10.7868/S3034517025060027
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 6
- Pages
- 468-479
- Abstract
- The purpose of the work is to build a self-consistent gas-dynamic model of the accretion disk of a compact astrophysical object, taking into account viscosity. The matter falling on a compact object consists of proton gas, electrons, and radiation arising from the braking of a rotating gas at a speed comparable to light. Physical proton viscosity is not enough in the gas-dynamic accretion model with laminar flow. It is necessary to introduce the so-called turbulent viscosity, probably arising from the development of instabilities, to explain the loss of the disk angular momentum. With a quantitative mathematical model of gas dynamics, taking into account the generally accepted turbulent viscosity, we want to demonstrate a solution with such instability.
- Keywords
- нейтронная звезда аккреционый диск гамма всплеск консервативная конечно-разностная схема
- Date of publication
- 10.03.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 36
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