Titlebook: Generation of Cosmological Large-Scale Structure; David N. Schramm,P. Galeotti Book 1997 Kluwer Academic Publishers 1997 Astronomical Obse

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https://doi.org/10.1007/978-94-009-0053-0Astronomical Observation; Cosmology; Dark matter; Redshift; Universe; astronomy; astrophysics

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https://doi.org/10.1007/978-3-031-19127-5Dynamical and redshift distortion studies can give Ω. only in the combination . = Ω./.. The determination of the density parameter Ω. by such methods is therefore impossible without a measurement of the bias parameter ..

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Harmonizing the Babel of VoicesEver since the first high-quality galaxy catalogues became available, statistics of large-scale structure has been an important tool to gain insight into the underlying physical processes and to allow for comparison of observations and predictions, both through theory and numerical experiment.

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Conversations on Optimal TransportWe study the evolution of the mass autocorrelation function in the Zel’dovich approximation and we compare the results with the predictions of the scaling ansatz for the growth of gravitational clustering formulated by Jain, Mo & White [7].

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On the Cosmological Mass FunctionThe theoretical determination of the mass function is performed by means of Lagrangian perturbation theory and ellipsoidal collapse. The statistical framework necessary to determine the mass function is briefly described. The main results and future applications are outlined.

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High Redshift Galaxiesexcitement in current cosmology, as mentioned also by J. Peebles sometime before 1983, is that we have opened an observational and theoretical window in the world of mathematical models and we are now looking in them, confronting them with the observations with the feeling that the prospects are exc