Numerical Study of Polytropes with n = 1 and Differential Rotation
The solution space of differentially rotating polytropes with $$n = 1$$ has been studied numerically. The existence of three different types of configurations: from spheroids to thick tori, hockey puck-like bodies and spheroids surrounded by a torus, separate from or merging with the central body has been proved. It has been shown that the last two types appear only at moderate degrees of rotation differentiality, $$\sigma \simeq 2$$ . Rigid-body or weakly differential rotation, as well as strongly differential, have not led to any “exotic” types of configurations. Many calculated configurations have had extremely large values of parameter $$\tau $$ , which has raised the question of their stability with respect to fragmentation.
Authors
- T. L. Razinkova
- С. И. Блинников (ORCID: https://orcid.org/0000-0002-5726-538X)
- A. V. Yudin (ORCID: https://orcid.org/0000-0002-0986-4257)
Institutions
- Novosibirsk State University (RU)
- Kurchatov Institute (RU)
- Kavli Institute for the Physics and Mathematics of the Universe (JP)
Publication Details
- Journal
- Astronomy Reports
- Published
- 2024-12-01
- DOI
- https://doi.org/10.1134/s1063772925701367
- Primary Topic
- Structural Analysis and Optimization
- Type
- article
- Field-Weighted Citation Impact
- 0.00