The Robertson-Walker Metric in a Pseudo-Complex General Relativity

Abstract

We investigate the consequences of the pseudo-complex General Relativity within a pseudo-complexified Roberston-Walker metric. A contribution to the energy-momentum tensor arises, which corresponds to a dark energy and may change with the radius of the universe, i.e., time. Only when the Hubble function $H$ does not change in time, the solution is consistent with a constant $\Lambda$.

31 pages, 2 figures

References in corpus (3)

• Pseudo-complex General Relativity
• Accretion of phantom scalar field into a black hole
• Pseudo-Complex Field Theory

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• Die Reissner-Nordström-Metrik in der Pseudokomplexen Allgemeinen Relativitätstheorie
• Observable consequences of pseudo-complex General Relativity
• Consequences of a minimal length in a pseudo-complex extension of General Relativity