Published in the International Journal of Modern Physics
D, Volume 9, Issue 04, pp. 373-443 (2000).
For a PDF version of the article, click
here.
For a Postscript version of the article, click
here.
and
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
-term
(cosmological constant). In this paper we
review both observational and theoretical aspects of a small cosmological
-term. We discuss
the current observational situation focusing on cosmological tests of
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
:
the generation of
in models with spontaneous symmetry breaking and
through quantum vacuum polarization effects - mechanisms
which are known to give rise to a
large value of
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
-term
by scalar fields are also extensively discussed. Anthropic
arguments favouring a small
-term are briefly
reviewed. A comprehensive bibliography of recent work
on
is provided.
Table of Contents
INTRODUCTION
THE COSMOLOGICAL CONSTANT REVISITED
FRW COSMOLOGICAL MODELS WITH
0
Closed universe models
(
= 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(
)
UNIVERSALITY OF LAMBDA AND ANTHROPIC ARGUMENTS FOR
ITS SMALL VALUE
SUMMARY AND DISCUSSION
REFERENCES