Published November 1988
| Version v1
Journal article
Mass multiplicity function from non-Gaussian primordial perturbations
Description
The mass multiplicity function of cosmic structures is considered for a general statistic of density perturbations in the framework of the hierarchical clustering scenario. In particular hierarchical and scale-invariant distributions are analyzed. The effect of the bias constraint on the mass function is also discussed. 76 references
Additional details
Publishing Information
- Journal Title
- Publications of the Astronomical Society of the Pacific
- Journal Volume
- 100
- Series
- Publ. Astron. Soc. Pac.
- Journal Page Range
- 1393-1398
- ISSN
- 0004-6280
- CODEN
- PASPA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20047620
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL MODELS; COSMOLOGY; DENSITY; GALACTIC EVOLUTION; GALAXIES; LUMINOSITY; MASS DISTRIBUTION; STATISTICS; UNIVERSE
- Descriptors DEC
- DISTRIBUTION; MATHEMATICAL MODELS; MATHEMATICS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPATIAL DISTRIBUTION