A model of accelerating dark energy in decelerating gravity
M. Roos

TL;DR
This paper explores a cosmological model combining Chaplygin gas dark energy with DGP braneworld gravity, showing it fits supernova data well without fine-tuning and may suggest a five-dimensional universe.
Contribution
It introduces a novel model integrating Chaplygin gas with DGP gravity that fits supernova data without fine-tuning and addresses the coincidence problem.
Findings
Self-decelerating branch fits supernova data as well as ΛCDM.
Model requires only one additional parameter.
Potential indication of a five-dimensional universe.
Abstract
The expansion of the Universe is accelerated as testified by observations of SNeIa at varying redshifts. Explanations of this acceleration are of two kinds: modifications of Einstein gravity or new forms of energy. An example of modified gravity is the braneworld Dvali-Gabadadze-Porrati (DGP) model, an example of dark energy is Chaplygin gas. Both are characterized by a cross-over length scale which marks the transition between physics occurring on our four-dimensional brane, and in a five-dimensional bulk space. Assuming that the scales in the two models are the same, we study Chaplygin gas dark energy in flat DGP geometries. The self-accelerating branch does not give a viable model, it causes too much acceleration. We derive the Hubble function and the luminosity distance for the self-decelerating branch, and then fit a compilation of 192 SNeIa magnitudes and redshifts in…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
