Concluding Remarks at the 12th Potsdam Cosmology Workshop

Details Concluding Remarks at the 12th Potsdam Cosmology Workshop Concluding Remarks at the 12th Potsdam Cosmology Workshop

1998-03-05

arxiv.org/abs/astro-ph/9803052v1

in "Large Scale Structure: Tracks and Traces", eds. V. M"uller, S. Gottl"ober, J. P. M"ucket, & J. Wambsganss, (Singapore: Wor

Astronomy and Astrophysics

Astrophysics

To appear in "Large Scale Structure: Tracks and Traces", Proceedings of the 12th Potsdam Cosmology Workshop, eds. V. M"uller,

Scientific paper

Research in cosmology traditionally divided into two separate lines. On the one hand was the search for initial conditions: the cosmological parameters H, Omega, Omega_b, 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.

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