Published in Nuclear Physics B Proceedings Supplements, Volume 87, Issue 1-3, p. 3-12, 2000. astro-ph/0007187

COSMOLOGICAL PARAMETERS

Joel R. Primack


Physics Department, University of California, Santa Cruz, CA 95064 USA

Abstract. The cosmological parameters that I will emphasize are the Hubble parameter H0 ident 100h km s-1 Mpc-1, the age of the universe t0, the average matter density Omegam, the baryonic matter density Omegab, the neutrino density Omeganu, and the cosmological constant OmegaLambda. The evidence currently favors t0 approx 13 Gyr, h approx 0.65, Omegam approx 0.4 ± 0.1, Omegab = 0.02h-2, 0.001 < Omeganu < 0.1, and OmegaLambda approx 0.7.

Table of Contents

INTRODUCTION

AGE OF THE UNIVERSE t0

HUBBLE PARAMETER H0
Relative Distance Methods
Fundamental Physics Approaches
Conclusions on H0

HOT DARK MATTER DENSITY Omeganu

COSMOLOGICAL CONSTANT Lambda

MEASURING Omegam

CONCLUSION

REFERENCES

For a postscript version of the article, click here.

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