Published November 15, 1990 | Version v1
Journal article

Large-scale structure and the adhesion approximation

  • 1. Cambridge Univ. (UK). Inst. of Astronomy
  • 2. Princeton Univ., NJ (USA). Observatory

Description

The adhesion approximation greatly extends the useful range of the Zel'dovich (quasi-linear) approximation by using artificial viscosity to mimic some of the effects of non-linear gravity. We describe a fast, three-dimensional implementation of the adhesion approximation, compare adhesion simulations to N-body calculations with identical initial conditions, and present results from large simulations with scale-free and cold dark matter (CDM) initial conditions. (author)

Additional details

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
247
Journal Issue
2
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
260-286
ISSN
0035-8711
CODEN
MNRAA

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
22024720
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ADHESION; COSMOLOGICAL MODELS; GALAXIES; GALAXY CLUSTERS; GRAVITATIONAL INTERACTIONS; INSTABILITY; NONLUMINOUS MATTER; RED SHIFT; SIMULATION; STRUCTURAL MODELS; UNIVERSE
Descriptors DEC
BASIC INTERACTIONS; MATHEMATICAL MODELS; MATTER

Optional Information

Contract/Grant/Project number
Grant NSF AST86-18257