Preprint Article Version 1 This version is not peer-reviewed

The Variation of G and Λ in Cosmology

Version 1 : Received: 17 October 2024 / Approved: 18 October 2024 / Online: 18 October 2024 (11:27:00 CEST)

How to cite: Beesham, A. The Variation of G and Λ in Cosmology. Preprints 2024, 2024101482. https://doi.org/10.20944/preprints202410.1482.v1 Beesham, A. The Variation of G and Λ in Cosmology. Preprints 2024, 2024101482. https://doi.org/10.20944/preprints202410.1482.v1

Abstract

The idea of varying constants of nature is very old, and has commanded a lot of attention 1 since first mooted. The variation of the gravitational parameter G and cosmological parameter Λ is still an active area of research. Since the idea of a varying G was introduced by Dirac almost a century ago, there are even theories that have variable G such as Brans-Dicke theory and the scale covariant theory. Both these theories also have a varying Λ in their full generalisations. A varying Λ was also introduced around the same time as that of varying G. It is interesting to note that a possible solution to the cosmological constant problem can be realised from a dynamic Λ. In this work, we focus on a varying Λ and G framework. In almost all studies in the simplest framework of variable Λ and G, it is found that one of them has to increase with time. However, observations and theoretical considerations indicate that both Λ and G should decrease with time. In this paper, we propose a solution to this problem, finding theories in which both Λ and G decrease with time.

Keywords

Variable Λ; Variable G; Conservation of energy momentum

Subject

Physical Sciences, Astronomy and Astrophysics

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