A Null Test of the Metric Nature of the Cosmic Acceleration
A.Buzzi (1), C.Marinoni (1), S.Colafrancesco (2) ((1) CPT, Universite, de Provence, France, (2) Osservatorio di Roma, Italy)

TL;DR
This paper proposes a test to distinguish between metric and non-gravitational causes of cosmic acceleration by examining environmental effects on supernova observations, potentially challenging dark energy models.
Contribution
It introduces a novel environmental test based on the dependence of supernova brightness on host galaxy mass to differentiate between acceleration mechanisms.
Findings
Supernova brightness depends on host galaxy environment in non-gravitational models.
Absence of environmental effects would support the metric dark energy explanation.
The proposed test offers a new way to validate the nature of cosmic acceleration.
Abstract
We discuss the testable predictions of a phenomenological model in which the accelerated expansion of the universe is the result of the action of a non-gravitational force field, rather than the effect of a negative-pressure dark-energy fluid or a modification of general relativity. We show, through the equivalence principle, that in such a scenario the cosmic acceleration felt by distant standard candles like SNIa depends on the mass of the host system, being larger in galaxies than in rich clusters. As a consequence, the scatter in the observed SNIa Hubble diagram has mostly a physical origin in this scenario: in fact, the SNIa distance modulus is increasing, at fixed redshift, for SNe that are hosted in isolated galaxies with respect to the case of SNe hosted in rich galaxy clusters. Due to its strong dependence on the astrophysical environments of standard candles, we conclude that…
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Taxonomy
TopicsCosmology and Gravitation Theories · Gamma-ray bursts and supernovae · Solar and Space Plasma Dynamics
