The mass multiplicity function from non-Gaussian primordial perturbations

Details The mass multiplicity function from non-Gaussian primordial perturbations The mass multiplicity function from non-Gaussian primordial perturbations

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1393l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Nov. 1988, p. 1393-1398.

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Astronomical Models, Computational Astrophysics, Cosmology, Perturbation, Density (Mass/Volume), Galactic Evolution, Luminosity, Power Spectra, Spectral Methods

Scientific paper

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.

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