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Are Chaplygin gases serious contenders to the dark energy throne?

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abstract

We study the implications on both background and perturbation evolution of introducing a Chaplygin gas component in the universe's ingredients. We perform likelihood analyses using wide-ranging, SN1a, CMB and large scale structure observations to assess whether such a component could be a genuine alternative to a cosmological constant. We find that current data favors an adiabatic Chaplygin gas with behavior akin to a cosmological constant.

fields

gr-qc 1

years

2019 1

verdicts

CONDITIONAL 1

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