ar X iv : a st ro - p h / 94 11 01 3 v 1 3 N ov 1 99 4 Application of Gradient Expansion to Inflationary Universe

ar X iv : a st ro - p h / 96 11 14 3 v 1 1 9 N ov 1 99 6 A high deuterium abundance in the early Universe

ar X iv : a st ro - p h / 99 11 49 7 v 1 2 9 N ov 1 99 9 Cosmic Microwave Background Anisotropies : Inflation versus Topological Defects

I present a briefly summary of the current status of inflationary models versus topological defects scenarios, as the mechanisms which could have induced the initial density perturbations, which left an imprint on the cosmic microwave backgound radiation anisotropies.

ar X iv : a st ro - p h / 94 01 02 3 v 1 1 4 Ja n 19 94 AZPH - TH / 93 - 5 Stochastic Fluctuations and Structure Formation in the Universe

It is shown that the evolution of the density perturbations during certain eras of substantial entropy generation in the universe can be described in the scheme of the KPZ equation. Therefore, the influence on cosmological structure formation by stochastic forces arising from various dissipations can be studied through the universal characteristics of surface growth in d = 3 + 1 dimensions. We ...

ar X iv : a st ro - p h / 97 11 24 4 v 1 2 0 N ov 1 99 7 POPULATION SYNTHESIS OF HIGH ENERGY TRANSIENTS RELATIVISTIC BINARY MERGING RATES

ar X iv : a st ro - p h / 99 11 43 8 v 1 2 3 N ov 1 99 9 H 2 molecules and cold clouds in cooling flow clusters †