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Structure Constraints from Large Angle CMB Anisotropies

Published online by Cambridge University Press:  30 March 2016

J. Richard Bond
J. Richard Bond*
Affiliation:
CIAR Cosmology Program, Canadian Institute for Theoretical Astrophysics Univesity of Toronto, ON M5S 1A1, Canada

Abstract

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Constraints on models of cosmic structure formation that can be drawn from current limits on large angle microwave background anisotropies are now competitive with those from recent small and intermediate angle experiments and are relatively insensitive to the reheating history of the Universe. Here I give limits on Gaussian scale invariant adiabatic fluctuations and describe the role that the large angle results play in constraining models with enhanced large distance galaxy clustering power inferred from correlation function measurements is described.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 319 - 321
Copyright
Copyright © Kluwer 1992

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