Published November 15, 1990
| Version v1
Journal article
Large-scale structure and the adhesion approximation
Creators
- 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