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, Λ, 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 Λ, 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 Λ>0 and a continuous one for Λ<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.
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Acknowledgements
The work by AVY has been supported by the ESF, project 4868 “The cosmological constant as eigenvalue of Sturm-Liouville problem”, and the work by AVA has been supported by the ESF, project 4760 “Dark energy landscape and vacuum polarization account”, both within the European Network “New Trends and Applications of the Casimir Effect”. EE’s research has been partly supported by MICINN (Spain), contract PR2011-0128 and projects FIS2006-02842 and FIS2010-15640, by the CPAN Consolider Ingenio Project, and by AGAUR (Generalitat de Catalunya), contract 2009SGR-994. EE’s research was partly carried out while on leave at the Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA.
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Astashenok, A.V., Elizalde, E. & Yurov, A.V. The cosmological constant as an eigenvalue of a Sturm-Liouville problem. Astrophys Space Sci 349, 25–32 (2014). https://doi.org/10.1007/s10509-013-1606-z
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DOI: https://doi.org/10.1007/s10509-013-1606-z