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Dark energy and inhomogeneity

G F R Ellis

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The standard understanding that distant supernova data implies existence of either dark energy or a cosmological constant Λ relies on the assumption of spatial homogeneity of the universe. A large-scale smoothed-out model of the universe ignores small-scale inhomogeneities, but the averaged effects of those inhomogeneities may alter both observational and dynamical relations at the larger scale, mimicking the effect of a cosmological constant. Alternatively large scale spatial inhomogeneity with zero Λ might mimic the effect of a positive cosmological constant. Whether this is the case or not is open to direct observational testing.


PACS

95.36.+x Dark energy

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

97.60.Bw Supernovae

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 1 (2009)



  1. Dark energy and inhomogeneity

    G F R Ellis 2009 J. Phys.: Conf. Ser. 189 012011

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