Published 1986 | Version v1
Report Restricted

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

Restricted

The record is publicly accessible, but files are restricted to users with access.

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.