Reconstruction of density and potential fields of the Universe

Details Reconstruction of density and potential fields of the Universe Reconstruction of density and potential fields of the Universe

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991tpsu.rept....7g&link_type=abstract

In MPI für Physik und Astrophysik, Traces of the Primordial Structure in the Universe p 7-19 (SEE N92-29833 20-90)

Astronomy and Astrophysics

Astrophysics

2

Galactic Clusters, Galactic Structure, Mass Distribution, Potential Fields, Universe, Astronomical Models, Cosmology, Galactic Mass, Mathematical Models

Scientific paper

Model and galaxy samples are analyzed in an attempt to see how galaxy and cluster samples could be used to characterize the total mass distribution of the Universe. A model which satisfactorily reproduces the basic properties of the observed structure is used to investigate how the distributions for the total matter, galaxies, and clusters in this model are mutually related. The relation between the distributions of galaxies and clusters in the real Universe is studied. The potential reconstruction method to restore the spectrum density fluctuations and potential field for the total matter starting from the distribution of clusters is proposed and results of the application of this method are analyzed.

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