Gravitational instability in the presence of a reflecting boundary

Details Gravitational instability in the presence of a reflecting boundary Gravitational instability in the presence of a reflecting boundary

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..535a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, June 1987, p. 535-538. In Russian. In Russian.

Statistics

Computation

Boundary Value Problems, Gravitational Fields, Jeans Theory, Reflected Waves, Computational Astrophysics, Systems Stability

Scientific paper

The role of a reflecting wall in gravitating systems is studied
theoretically in the framework of a Jeans model. When beta ranges from
greater than 0 to less than 1/2, special increasing boundary modes are
found to exist. These modes are characterized by a discrete spectrum:
the value of the ip wavenumber turned out to be unique.

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