Concluding Remarks at the 12th Potsdam Cosmology Workshop

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dc.creatorYahil, A.
dc.date1998-03-05
dc.date.accessioned2026-07-07T02:26:16Z
dc.date.available2026-07-07T02:26:16Z
dc.descriptionResearch 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.
dc.descriptionTo 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9803052
dc.identifierhttp://arxiv.org/abs/astro-ph/9803052
dc.identifierin "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)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12209
dc.subjectAstrophysics
dc.titleConcluding Remarks at the 12th Potsdam Cosmology Workshop
dc.typetext

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