2012

On solutions of loop quantum cosmology

Sadjadi, H. Mohseni

Understand

Loop quantum cosmology is considered in inflation era.

A slow roll scalar field solution with power law potential is presented in the neighborhood of transition time, i.e.
when the universe enters inflation phase from super-inflation.
The compatibility of the model with Planck 2013 data is discussed.

Built on

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Similar

R. G. Cai and S. P. Kim, J. High Energy Phys. 0502, 050 (2005)
2005
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E. J. Copeland, D. J. Mulryne, N. J. Nunes, and M. Shaeri, Phys. Rev. D 77, 023510 (2008)
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Then

G. Izquierdo and D. Pavon, Phys. Lett. B 633, 420 (2006); H. Mohseni Sadjadi, Phys. Rev. D 73, 063525 (2006); H. Mohseni Sadjadi, Europhys. Lett. 92, 50014 (2010)
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Original
2011
Later among the works it cites.
A. Ashtekar, and D. Sloan, Gen. Rel. Grav. 43, 3619 (2011)
2011
Later among the works it cites.
E. Komatsu et al., Astrophys. J. Suppl. 192, 18 (2011), arXiv:1001.4538 [astro-ph.CO]
Original
2011
Later among the works it cites.
E. W. Ewing, JCAP 1303, 026 (2013), arXiv:1211.6269 [gr-qc]
Original
2013
Closest in time.
P. A. R. Ade et al., Planck 2013 results. XVI, arXiv: 1303.5076 [astro-ph] (2013); P. A. R. Ade et al., Planck 2013 results. I, arXiv: 1303.5062 [astro-ph) (2013)
2013
Closest in time.

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