Three-dimensional gas dynamics in a sphere

Details Three-dimensional gas dynamics in a sphere Three-dimensional gas dynamics in a sphere

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jcoph..87..201b&link_type=abstract

Journal of Computational Physics (ISSN 0021-9991), vol. 87, March 1990, p. 201-230. Research supported by CNRS.

Astronomy and Astrophysics

Astronomy

27

Black Holes (Astronomy), Gas Dynamics, Gravitational Collapse, Gravitational Waves, Stellar Evolution, Supernovae, Chebyshev Approximation, Legendre Functions, Partial Differential Equations, Spectrum Analysis, Spheres, Wave Equations

Scientific paper

The present numerical method for solving three-dimensional PDFs in a sphere subject to various boundary conditions was developed with a view to the characterization of the gravitational-collapse process for a star which ends in either the formation of a supernova or a black hole, with subsequent gravitational radiation emissions. Attention is given to the application of a spectral analysis-based numerical method to the solution of three-dimensional waveequations, as well as to the solutions of gas-dynamics equations for various pertinent cases.

Affiliated with

Also associated with

No associations

Rating

Three-dimensional gas dynamics in a sphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Three-dimensional gas dynamics in a sphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-dimensional gas dynamics in a sphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1887814