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In this paper, we propose a model in which a spectator field non-minimally couples to an inflaton field and the power spectrum of the perturbation of the spectator field at small scales is dramatically enhanced by the sharp feature in the form of non-minimal coupling.
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William H. Kinney, “Horizon crossing and inflation with large eta,” Phys. Rev. D 72
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Kari Enqvist and Sami Nurmi, “Non-gaussianity in curvaton models with nearly quadratic potential,” JCAP 10
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Carmelita Carbone and Sabino Matarrese, “A Unified treatment of cosmological perturbations from super-horizon to small scales,” Phys. Rev. D71
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Misao Sasaki, Jussi Valiviita, and David Wands, “Non-Gaussianity of the primordial perturbation in the curvaton model,” Phys. Rev. D 74
2006
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P. Tisserand et al. (EROS-2), “Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds,” Astron. Astrophys. 469
2007
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Kouji Nakamura, “Second-order gauge invariant cosmological perturbation theory: Einstein equations in terms of gauge invariant variables,” Prog. Theor. Phys. 117
2007
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Kishore N. Ananda, Chris Clarkson, and David Wands, “The Cosmological gravitational wave background from primordial density perturbations,” Phys. Rev. D75
2007
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Caner Unal, “Imprints of Primordial Non-Gaussianity on Gravitational Wave Spectrum,” Phys. Rev. D99
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Guillem Domènech, “Scalar Induced Gravitational Waves Review,” Universe 7
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