The cosmological constant as an eigenvalue of a Sturm-Liouville problem

TL;DR

This paper explores the cosmological constant as an eigenvalue of a Sturm-Liouville problem derived from Einstein-Friedmann equations, revealing discrete spectra and implications for cyclic cosmological models with potential singularities.

Contribution

It formulates the cosmological constant as an eigenvalue problem, linking spectral theory to cosmology and proposing conditions for universe models without anthropic reasoning.

Findings

Discrete spectrum of $\\Lambda$ for positive values under certain boundary conditions

Existence of a single eigenvalue allowing specific cosmological scenarios

Cyclic universe models with potential for sudden future singularities

Abstract

It is observed that one of Einstein-Friedmann's equations has formally the aspect of a Sturm-Liouville problem, and that the cosmological constant, $\Lambda$, plays thereby the role of spectral parameter (what hints to its connection with the Casimir effect). The subsequent formulation of appropriate boundary conditions leads to a set of admissible values for $\Lambda$, considered as eigenvalues of the corresponding linear operator. Simplest boundary conditions are assumed, namely that the eigenfunctions belong to $L^2$ space, with the result that, when all energy conditions are satisfied, they yield a discrete spectrum for $\Lambda>0$ and a continuous one for $\Lambda<0$. A very interesting situation is seen to occur when the discrete spectrum contains only one point: then, there is the possibility to obtain appropriate cosmological conditions without invoking the anthropic principle. This possibility is shown to be realized in cyclic cosmological models, provided the potential of the matter field is similar to the potential of the scalar field. The dynamics of the universe in this case contains a sudden future singularity.