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Potential-Density Basis Sets for Three-Dimensional Disks

Published online by Cambridge University Press:  25 May 2016

David J.D. Earn*
Affiliation:
Racah Institute of Physics The Hebrew University, Jerusalem 91904, Israel

Extract

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Poisson's equation, ∇2ψ = 4πGρ, can be solved approximately using basis sets of potential-density pairs. A given density is approximated by a truncated expansion; the computed expansion coefficients immediately yield the corresponding potential since each basis density function is paired with a basis potential function, and Poisson's equation is linear.

Type
Chapter 6: How are we to Understand the Large Scale Structure of the ISM?
Copyright
Copyright © Kluwer 1996 

References

Clutton-Brock, M. (1972) Astrophys. and Space Sci. , 16, 101119 CrossRefGoogle Scholar
Kalnajs, A.J. (1977) Astrophys. J. , 212, 637644 CrossRefGoogle Scholar
Saha, P. (1993) Mon. Not. R. astr. Soc. , 262, 10621064 CrossRefGoogle Scholar