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A Cosmological Solution to Mimetic Dark Matter · Around

2014

A Cosmological Solution to Mimetic Dark Matter

Saadi, Hassan

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In this paper, a cosmological solution to Mimetic Dark Matter (MDM) for an exponential potential is provided.

Then, a solution for the $0-i$ perturbed Einstein's differential equation of MDM is obtained based on an exponential potential that satisfies inflation for some initial conditions.
Another general potential is suggested that incorporates inflation too.
Then, quantum perturbations are included.

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A. H. Chamseddine and V. Mukhanov, Mimetic dark matter, JHEP 1311 (2013) 135
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Similar

A. Vikman, Europhys. Lett. 101 (2013) 34001 [arXiv:1208.3647 [hep-th]]
Original
2013
Cited alongside, same era.
P. Ade et al. (Planck Collaboration) (2013), arXiv:1303.5082
Original
2013
Cited alongside, same era.
A. H. Chamseddine, V. Mukhanov and A. Vikman, Cosmology with Mimetic Matter, JCAP 1406 (2014) 017
2014
Cited alongside, same era.
A. Barvinsky, Dark matter as a ghost free conformal extension of Ein- stein theory, arXiv:1311.3111 [hep-th]
Original
Cited in the paper.
V. Mukhanov, Physical foundations of cosmology. Cambridge University
Cited in the paper.

Then

A. Golovnev, On the recently proposed Mimetic Dark Matter, Phys. Lett. B728 (2014) 39–40, arXiv:1310.2790 [gr-qc]
Original
2014
Closest in time.
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Closest in time.
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Closest in time.

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