1998/03/05 by A. Yahil
Physics and Astronomy · #astro-ph
published as in "Large Scale Structure: Tracks and Traces", eds. V. M"uller, S. Gottl"ober, J. P. M"ucket, & J. Wambsganss, (Singapore: World Scientific), pp. 385-390 (1998) · To appear in "Large Scale Structure: Tracks and Traces", Proceedings of the 12th Potsdam Cosmology Workshop, eds. V. M"uller, S. Gottl"ober, J. P. M"ucket, J. Wambsganss, (Singapore: World Scientific), 1998. 6 LaTeX pages. Also available at ftp://sbast4.ess.sunysb.edu/pub/ayahil/papers/potsdam97_summary.tex
Research in cosmology traditionally divided into two separate lines. On the one hand was the search for initial conditions: the cosmological parameters H, Omega, Omegab, and Lambda, and the power spectrum P(k). On the other hand was the study of the formation and evolution of structures, from globular-cluster sized objects to large-scale structures. These lines of investigation are now becoming increasingly intertwined, and this tendency manifested itself in this conference. Following is my personal perspective on where we stand today. I also discuss some technological developments that I think will affect the field. My concluding remarks are very informal. They are not a review paper, and I omit references altogether rather than give a partial list.