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Gauge-flation: Inflation From Non-Abelian Gauge Fields · Around

2011

Gauge-flation: Inflation From Non-Abelian Gauge Fields

Maleknejad, A., Sheikh-Jabbari, M. M.

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Inflationary models are usually based on dynamics of one or more scalar fields coupled to gravity.

In this work we present a new class of inflationary models, gauge-flation or non-Abelian gauge field inflation, where slow-roll inflation is driven by a non-Abelian gauge field.
This class of models are based on a gauge field theory with a generic non-Abelian gauge group minimally coupled to gravity.
We then focus on a particular gauge-flation model by specifying the action for the gauge theory which allows for a successful slow-roll inflation.

Built on

A. Maleknejad and M. M. Sheikh-Jabbari, “Non-Abelian Gauge Field Inflation,” [arXiv:1102.1932 [hep-ph]]
Original
1932
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D. V. Galtsov and M. S. Volkov,“Yang-Mills cosmology: Cold matter for a hot universe,” Phys. Lett. B 256
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S. Weinberg, “The quantum theory of fields. Vol. 2: Modern applications,” Cambridge, UK: Univ. Pr. (1996)
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V. Mukhanov, “Physical Foundations of Cosmology,” Cambrdige Uni. Press (2005)
2005
Earlier work this paper cites.

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S. Weinberg, “Cosmology,” SPIRES entry Oxford, UK: Oxford Univ. Pr. (2008)
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F. L. Bezrukov and M. Shaposhnikov, “The Standard Model Higgs boson as the inflaton,” Phys. Lett. B 659
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B. Himmetoglu, C. R. Contaldi, M. Peloso, “Instability of anisotropic cosmological solutions supported by vector fields,” Phys. Rev. Lett. 102
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P. Adshead, E. Martinec and M. Wyman, “A Sinister Universe: Chiral gravitons lurking, and Lyth un-bound,” arXiv:1301.2598 [hep-th]
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A. Maleknejad, M. M. Sheikh-Jabbari and J. Soda, “Gauge Fields and Inflation,” arXiv:1212.2921 [hep-th]
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Cited in the paper.

Then

E. Komatsu et al
Original
2011
Closest in time.
M. M. Sheikh-Jabbari, “Gauge-flation Vs Chromo-Natural Inflation,” Phys. Lett. B 717
Original
2012
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A. Golovnev, V. Mukhanov and V. Vanchurin, “Vector Inflation,” JCAP 0806, 009 (2008), [arXiv:0802.2068[astro-ph]]
Original
2068
Closest in time.

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