Published February 5, 1992 | Version v1
Journal article

N-body simulations of cold dark matter

Creators

  • 1. NASA/Fermilab Astrophysics Center, P. O. Box 500, Batavia, Illinois 60510 (United States)
  • 2. Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)

Description

We use large N-body simulations to follow the nonlinear gravitational clustering of millions of mass points representing collisionless clouds of cold dark matter (CDM) in a critically-closed universe (Ω=1). Simulated catalogs of galaxies are statistically compared with observations of spatial and velocity correlations. We show that the CDM model, normalized on large scales using recent COBE data, predicts excessive small-scale velocities; and we discuss possible modifications to the model that may help reduce this problem

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
272
Journal Issue
2
Journal Page Range
p. 1608-1613.
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
26. International Union of Pure and Applied Physics (IUPAP) conference on high energy physics.
Acronym
ICHEP-26
Dates
6-12 Aug 1992.
Place
Dallas, TX (United States).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
26034923
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COMPUTERIZED SIMULATION; CORRELATION FUNCTIONS; GALAXY CLUSTERS; GRAVITATIONAL FIELDS; GRAVITATIONAL INTERACTIONS; NONLUMINOUS MATTER; SPACE VEHICLES; STATISTICS; UNIVERSE
Descriptors DEC
BASIC INTERACTIONS; FUNCTIONS; MATHEMATICS; MATTER; SIMULATION

Optional Information

Secondary number(s)
CONF-920837--.