Published 1986
| Version v1
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Numerical experiments on galactic halo formation
Description
We have used a hybrid N-body-FFT approach to solving Poisson's equation in a cosmological setting. Using this method, we have explored the connection between the form of the initial Gaussian density perturbations that by today have grown into galaxies and the internal properties of the individual galactic halos that are formed. 19 refs., 4 figs
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS, PC A02/MF A01 as DE87000139.
Files
Additional details
Publishing Information
- Imprint Pagination
- 13 p.
- Report number
- LA-UR--86-3113
Conference
- Title
- Workshop on the use of supercomputers in stellar dynamics.
- Dates
- 2-4 Jun 1986.
- Place
- Princeton, NJ (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18043967
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- FOURIER TRANSFORMATION; GALACTIC EVOLUTION; NUMERICAL SOLUTION; PERTURBATION THEORY; POISSON EQUATION
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; EQUATIONS; INTEGRAL TRANSFORMATIONS; PARTIAL DIFFERENTIAL EQUATIONS; TRANSFORMATIONS
Optional Information
- Secondary number(s)
- CONF-8606175--2.