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We study features in the bispectrum of the primordial curvature perturbation correlated with the reconstructed primordial power spectrum from the observed cosmic microwave background temperature data.
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For previous studies, see e.g. A. Achucarro, V. Atal, P. Ortiz and J. Torrado, Phys. Rev. D 89
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D. K. Hazra, L. Sriramkumar and J. Martin, JCAP 1305
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A. Achucarro, J. O. Gong, G. A. Palma and S. P. Patil, Phys. Rev. D 87
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See e.g. D. Baumann and L. McAllister, arXiv:1404.2601 [hep-th]
Cited in the paper.
In a recent article [ 27 ] a one-parameter formula for the correlation of the bispectrum and the power spectrum has been derived for the case of both a non-trivial sound speed and potential features upon certain assumptions
Cited in the paper.
See [ 13 ] for complementary results, where next-to-leading order GSR corrections are shown to improve the bispectrum estimate for sharper departures from slow-roll
Cited in the paper.
2015
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S. Mooij, G. A. Palma, G. Panotopoulos and A. Soto, JCAP 1510
2015
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See also P. D. Meerburg, M. Münchmeyer and B. Wandelt, Phys. Rev. D 93
2016
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