We derive the time evolution of the density contrast to all orders of perturbation theory, by solving the Einstein equation for scale-invariant fluctuations. These fluctuations are represented by an infinite series in inverse powers of the radial parameter. In addition to the standard growing modes, we find infinitely many more new growing modes for open and closed universes
We investigate the transfer of power between different scales and the coupling of modes during the n...
Abstract. We inquire the phenomena of clustering of galaxies in an expanding universe from a theoret...
Here we rederive the hierarchy of equations for the evolution of distribution functions of various o...
We derive the time evolution of the density contrast to all orders of perturbation theory, by solvin...
We derive the time evolution of the density contrast to all orders of perturbation theory, by solvin...
We investigate the properties of the standard perturbative expansions which describe the early stage...
We discuss the late-time evolution of the gravitational clustering in an expanding universe, based o...
Gravitational perturbations in the expanding universe are analyzed within the framework of Newtonian...
The evolution of inhomogeneities in a spherical collapse model is studied by expanding the Einstein ...
Sorry, the full text of this article is not available here. Please click on the alternative location...
We apply topological measures of clustering such as percolation and genus curves (PC & GC) and s...
The description of gravitational clustering is essentially statistical but its origin is dynamical. ...
We apply topological measures of clustering such as percolation and genus curves (PC & GC) a...
We present the Covariant and Gauge Invariant theory of scalar perturbations of a Friedmann-Lemaître-...
Hamilton et al. recently proposed the idea that the growth of density perturbations in an expanding ...
We investigate the transfer of power between different scales and the coupling of modes during the n...
Abstract. We inquire the phenomena of clustering of galaxies in an expanding universe from a theoret...
Here we rederive the hierarchy of equations for the evolution of distribution functions of various o...
We derive the time evolution of the density contrast to all orders of perturbation theory, by solvin...
We derive the time evolution of the density contrast to all orders of perturbation theory, by solvin...
We investigate the properties of the standard perturbative expansions which describe the early stage...
We discuss the late-time evolution of the gravitational clustering in an expanding universe, based o...
Gravitational perturbations in the expanding universe are analyzed within the framework of Newtonian...
The evolution of inhomogeneities in a spherical collapse model is studied by expanding the Einstein ...
Sorry, the full text of this article is not available here. Please click on the alternative location...
We apply topological measures of clustering such as percolation and genus curves (PC & GC) and s...
The description of gravitational clustering is essentially statistical but its origin is dynamical. ...
We apply topological measures of clustering such as percolation and genus curves (PC & GC) a...
We present the Covariant and Gauge Invariant theory of scalar perturbations of a Friedmann-Lemaître-...
Hamilton et al. recently proposed the idea that the growth of density perturbations in an expanding ...
We investigate the transfer of power between different scales and the coupling of modes during the n...
Abstract. We inquire the phenomena of clustering of galaxies in an expanding universe from a theoret...
Here we rederive the hierarchy of equations for the evolution of distribution functions of various o...
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