Published in the International Journal of Modern Physics D, Volume 9, Issue 04, pp. 373-443 (2000).

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THE CASE FOR A POSITIVE COSMOLOGICAL LAMBDA-TERM

Varun Sahni


IUCAA - Inter-University Centre for Astronomy & Astrophysics, Post Bag 4, Ganeshkind, Pune 411007, India

and

Alexei Starobinsky


Landau Institute for Theoretical Physics, Kosygina 2, Moscow 117334, Russia


Abstract. Recent observations of Type 1a supernovae indicating an accelerating universe have once more drawn attention to the possible existence, at the present epoch, of a small positive Lambda-term (cosmological constant). In this paper we review both observational and theoretical aspects of a small cosmological Lambda-term. We discuss the current observational situation focusing on cosmological tests of Lambda including the age of the universe, high redshift supernovae, gravitational lensing, galaxy clustering and the cosmic microwave background. We also review the theoretical debate surrounding Lambda: the generation of Lambda in models with spontaneous symmetry breaking and through quantum vacuum polarization effects - mechanisms which are known to give rise to a large value of Lambda hence leading to the `cosmological constant problem'. More recent attempts to generate a small cosmological constant at the present epoch using either field theoretic techniques, or by modeling a dynamical Lambda-term by scalar fields are also extensively discussed. Anthropic arguments favouring a small Lambda-term are briefly reviewed. A comprehensive bibliography of recent work on Lambda is provided.


Table of Contents

INTRODUCTION

THE COSMOLOGICAL CONSTANT REVISITED

FRW COSMOLOGICAL MODELS WITH Lambda neq 0
Closed universe models (kappa = 1)
Spatially open and flat cosmological models

OBSERVATIONAL CONSEQUENCES OF A COSMOLOGICAL LAMBDA-TERM
H0, q0 and the Age of the Universe
The luminosity distance and gravitational lensing
Type 1a Supernovae and the value of Lambda
Constraints on Lambda from the cosmic microwave background
The Angular size - redshift relation
Clusters of galaxies and the Large Scale Structure of the Universe

THEORETICAL ISSUES: VACUUM FLUCTUATIONS AND THE COSMOLOGICAL CONSTANT

THE COSMOLOGICAL CONSTANT AND SPONTANEOUS SYMMETRY BREAKING

MECHANISMS FOR GENERATING A SMALL CURRENT VALUE OF LAMBDA
A Decaying Cosmological Constant?
Vacuum polarization and the value of Lambda
Late-time Inflation and Lambda.
Generating a small cosmological constant from Inflationary particle production

PHENOMENOLOGICAL MODELS OF A DYNAMICAL LAMBDA-TERM
Overview
When may a Lambda-term be described by a minimally coupled scalar field?
Relation between kinematic and dynamical descriptions of Lambda
Reconstructing the effective potential V(phi)

UNIVERSALITY OF LAMBDA AND ANTHROPIC ARGUMENTS FOR ITS SMALL VALUE

SUMMARY AND DISCUSSION

REFERENCES

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