Abstract. We briefly discuss some aspects of the problem of forming large scale structures in the Universe. The basic picture that initially small perturbations generated by inflation grow by the process of gravitational instability to give the observed structures is largely consistent with the observations. The growth of the perturbations depends crucially on the contents of the Universe, and we discuss a few variants of the cold dark matter model. Many of these models are consistent with present observations. Future observations hold the possibility of deciding amongst these models
Copyright © 2013 Mariwan A. Rasheed and Mohamad A. Brza. This is an open access article distributed ...
I discuss the use of perturbative methods to study the evolution of matter fluctuations in the conte...
In the last century, new observational techniques and discoveries such as the Cosmic Microwave Backg...
A better understanding of the formation of large-scale structure in the Universe is arguably the mos...
Abstract: Over the past three decades the established view of a nearly homogeneuous, featureless Uni...
Over the past three decades the established view of a nearly homogeneuous, featureless Universe on s...
Over the past three decades the established view of a nearly homogeneuous, featureless Universe on s...
The changes of main paradigms on the structure and evolution of the Universe are reviewed. Two puzzl...
Large-scale structures in the Universe provide crucial information about formation of structures and...
Large-scale structures in the Universe provide crucial information about formation of structures and...
With the development of more and more large scale surveys in the past few years, and the years to co...
A brief account is given of large-scale structure modelling based on the assumption that the initial...
We generalize and extend the statistical description of formation and evolution of Large Scale matt...
I will describe some of the outstanding questions in Cosmology where answers could be provided by ob...
We investigate cosmological structure formation seeded by topological defects which may form during ...
Copyright © 2013 Mariwan A. Rasheed and Mohamad A. Brza. This is an open access article distributed ...
I discuss the use of perturbative methods to study the evolution of matter fluctuations in the conte...
In the last century, new observational techniques and discoveries such as the Cosmic Microwave Backg...
A better understanding of the formation of large-scale structure in the Universe is arguably the mos...
Abstract: Over the past three decades the established view of a nearly homogeneuous, featureless Uni...
Over the past three decades the established view of a nearly homogeneuous, featureless Universe on s...
Over the past three decades the established view of a nearly homogeneuous, featureless Universe on s...
The changes of main paradigms on the structure and evolution of the Universe are reviewed. Two puzzl...
Large-scale structures in the Universe provide crucial information about formation of structures and...
Large-scale structures in the Universe provide crucial information about formation of structures and...
With the development of more and more large scale surveys in the past few years, and the years to co...
A brief account is given of large-scale structure modelling based on the assumption that the initial...
We generalize and extend the statistical description of formation and evolution of Large Scale matt...
I will describe some of the outstanding questions in Cosmology where answers could be provided by ob...
We investigate cosmological structure formation seeded by topological defects which may form during ...
Copyright © 2013 Mariwan A. Rasheed and Mohamad A. Brza. This is an open access article distributed ...
I discuss the use of perturbative methods to study the evolution of matter fluctuations in the conte...
In the last century, new observational techniques and discoveries such as the Cosmic Microwave Backg...