A note on low energy effective theory of chromo-natural inflation in the light of BICEP2 results
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
0103 physical sciences
FOS: Physical sciences
01 natural sciences
Astrophysics - Cosmology and Nongalactic Astrophysics
DOI:
10.1142/s0217732315500406
Publication Date:
2015-03-18T02:05:15Z
AUTHORS (3)
ABSTRACT
Recent result of BICEP2, revealing a larger value of tensor to scalar ratio (r), has opened up new investigations of the inflationary models to fit the experimental data. The experiment needs to reconfirm the results, specifically the consistency between Planck and BICEP2. On the other hand, the combined analysis of Planck and BICEP2, including the dust polarization uncertainty, brings down the upper limit on r. In this paper, we re-examine the low energy effective theory of chromo-natural inflation model and its generalization in view of such observational data. We find that the parameter space of the model admits a large value of r as well as other cosmological observables consistent with data.
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