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Inhomogeneous Dark Energy · Around

2016

Inhomogeneous Dark Energy

Chamseddine, Ali H., Mukhanov, Viatcheslav

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We modify Einstein General Relativity by adding non-dynamical scalar fields to account simultaneously for both dark matter and dark energy.

The dark energy in this case can be distributed in-homogeneously even within horizon scales.
Its inhomogeneities can contribute to the late time integrated Sachs-Wolfe effect, possibly removing some of the low multipole anomalies in the temperature fluctuations of the CMB spectrum.
The presence of the inhomogeneous dark matter also influences structure formation in the universe.

Built on

Viatcheslav Mukhanov, Physical Foundations of Cosmology,
2005
Earlier work this paper cites.
Ali H. Chamseddine and Viatcheslav Mukhanov, Mimetic Dark Matter,
2013
Earlier work this paper cites.

Similar

A. Golovnev, On the recently proposed Mimetic Dark Matter
2014
Cited alongside, same era.
A. Barvinsky, Dark matter as a ghost free conformal extension of Einstein theory
2014
Cited alongside, same era.
L. D. Landau and E. M. Lifshitz, The Classical Theory of Fields, Fourth Edition, Butterworth, Heineman
Cited in the paper.

Then

Ali H. Chamseddine, Viatcheslav Mukhanov and Alexander Vikman, Cosmology with Mimetic Matter,
2014
Later among the works it cites.
R. G. Crittenden and N. Turok, Looking for a Cosmological Constant with the Rees-Sciama Effect
2015
Later among the works it cites.

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