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Primordial non-Gaussianity encodes vital information of the physics of the early universe, particularly during the inflationary epoch.
P.D. Meerburg et al., Primordial Non-Gaussianity , 1903.04409
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J.M. Maldacena, Non-Gaussian features of primordial fluctuations in single field inflationary models , JHEP 05
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N. Bartolo, S. Matarrese and A. Riotto, On nonGaussianity in the curvaton scenario , Phys. Rev. D 69
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M. Zaldarriaga, Non-Gaussianities in models with a varying inflaton decay rate , Phys. Rev. D 69
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D.H. Lyth, Generating the curvature perturbation at the end of inflation , JCAP 11
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J. Crowder and N.J. Cornish, Beyond LISA: Exploring future gravitational wave missions , Phys. Rev. D 72
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K.N. Ananda, C. Clarkson and D. Wands, The Cosmological gravitational wave background from primordial density perturbations , Phys. Rev. D 75
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D. Baumann, P.J. Steinhardt, K. Takahashi and K. Ichiki, Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations , Phys. Rev. D 76
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A.M. Green and B.J. Kavanagh, Primordial Black Holes as a dark matter candidate , J. Phys. G 48
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M. Maggiore, Gravitational Waves. Vol. 2: Astrophysics and Cosmology , Oxford University Press (3, 2018)
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C. Unal, Imprints of Primordial Non-Gaussianity on Gravitational Wave Spectrum , Phys. Rev. D 99
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M. Taoso and A. Urbano, Non-gaussianities for primordial black hole formation , JCAP 08
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