Stable Galaxy Configurations

Y. Guo ()
Additional contact information
Y. Guo: Brown University, Division of Applied Mathematics Box F

A chapter in Hyperbolic Problems: Theory, Numerics, Applications, 2008, pp 35-43 from Springer

Abstract: Dynamics of galaxies can be described by the Vlasov–Poisson system, where stars interact only with the gravitational field they create collectively. In this note, recent developments in mathematical study of stability of galaxy configurations are discussed.

Date: 2008
References: Add references at CitEc
Citations:

There are no downloads for this item, see the EconPapers FAQ for hints about obtaining it.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:spr:sprchp:978-3-540-75712-2_3

Ordering information: This item can be ordered from
http://www.springer.com/9783540757122

DOI: 10.1007/978-3-540-75712-2_3

Access Statistics for this chapter

More chapters in Springer Books from Springer
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().