2002Unpublished venueRequires access

THE COSMOLOGICAL CONSTANT PROBLEM

Wei Wang

Open publisher page 1 citations

Abstract

In recent years there have been good reasons to believe that cosmology with a positive cosmological constrant is the best fit to observable phenomena in astronomy. The cosmological constant as a measure of the energy desity of the vacuum is too small at the particle physics level, but it is comparable to the present matter density. However,the small cosmological constant and cosmic coincidence problem cannot be resolved within the known laws of physics, which is the famous cosmological constant problem in physics and astronomy. In this review we first introduce the great progress in observational evidence for the accelerating universe with the positive cosmological constant and discuss a number of approaches to this puzzle, which at this point remains one of the most significant unsolved problems in fundamental physics.

About this research paper

What this paper is about

In recent years there have been good reasons to believe that cosmology with a positive cosmological constrant is the best fit to observable phenomena in astronomy. The cosmological constant as a measure of the energy desity of the vacuum is too small at the particle physics level, but it is comparable to the present matter density. However,the small cosmological constant and cosmic coincidence problem cannot be resolved within the known laws of physics, which is the famous cosmological constant problem in physics and astronomy. In this review we first introduce the great progress in observational evidence for the accelerating universe with the positive cosmological constant and discuss a number of approaches to this puzzle, which at this point remains one of the most significant unsolved problems in fundamental physics.

Why it matters

OpenAlex reports 1 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

In recent years there have been good reasons to believe that cosmology with a positive cosmological constrant is the best fit to observable phenomena in astronomy. The cosmological constant as a measure of the energy desity of the vacuum is too small at the particle physics level, but it is comparable to the present matter density. However,the small cosmological constant and cosmic coincidence problem cannot be resolved within the known laws of physics, which is the famous cosmological constant problem in physics and astronomy. In this review we first introduce the great progress in observational evidence for the accelerating universe with the positive cosmological constant and discuss a number of approaches to this puzzle, which at this point remains one of the most significant unsolved problems in fundamental physics.

Key concepts: Physics, Cosmological constant, Cosmological constant problem, Cosmology, Theoretical physics, Metric expansion of space, Lambda-CDM model, Dark energy

Related papers

Back to paper searchBrowse research topicsOriginal source
THE COSMOLOGICAL CONSTANT PROBLEM — Research Paper | ScholarLens