A New Solution of The Cosmological Constant Problems

Abstract

We extend the usual gravitational action principle by promoting the bare cosmological constant (CC) from a parameter to a field which can take many possible values. Variation leads to a new integral constraint equation which determines the classical value of the effective CC that dominates the wave function of the universe. In a realistic cosmological model, the expected value of the effective CC, is calculated from measurable quantities to be O(t_U), as observed, where t_U is the present age of the universe in Planck units,. Any application of our model produces a falsifiable prediction for $\Lambda$ in terms of other measurable quantities. This leads to a specific falsifiable prediction for the observed spatial curvature parameter of Omega_k0=-0.0055. Our testable proposal requires no fine tunings or extra dark-energy fields but does suggest a new view of time and cosmological evolution.

5 pages; v3: version accepted by Phys. Rev. Lett

References in corpus (2)

• The Measure Problem in Cosmology
• A Strong Constraint on Ever-Present Lambda

Cited by in corpus (1)

• Die Reissner-Nordström-Metrik in der Pseudokomplexen Allgemeinen Relativitätstheorie