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We discuss observational consequences of the curvaton scenario, which naturally appears in the context of the simplest model of chaotic inflation in supergravity.
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A. D. Linde, Particle Physics and Inflationary Cosmology
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M. Tegmark and M. J. Rees, “Why is the CMB fluctuation level 𝟏𝟎 − 𝟓 10^{-5} ?,” Astrophys. J. 499
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M. Kawasaki, M. Yamaguchi and T. Yanagida, “Natural chaotic inflation in supergravity,” Phys. Rev. Lett. 85
2000
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K. Enqvist and M. S. Sloth, “Adiabatic CMB perturbations in pre big bang string cosmology,” Nucl. Phys. B 626
2002
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D. H. Lyth and D. Wands, “Generating the curvature perturbation without an inflaton,” Phys. Lett. B 524
2002
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T. Moroi and T. Takahashi, “Effects of cosmological moduli fields on cosmic microwave background,” Phys. Lett. B 522
2002
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D. H. Lyth, C. Ungarelli and D. Wands, “The primordial density perturbation in the curvaton scenario,” Phys. Rev. D 67
2003
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J. Garriga and A. Vilenkin, “Anthropic prediction for Lambda and the Q catastrophe,” Prog. Theor. Phys. Suppl. 163
2006
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D. H. Lyth, “Non-gaussianity and cosmic uncertainty in curvaton-type models,” JCAP 0606
2006
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S. C. Davis and M. Postma, “SUGRA chaotic inflation and moduli stabilisation,” JCAP 0803
2008
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A. D. Linde, “Inflationary Cosmology,” Lect. Notes Phys. 738
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2008
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2005
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A. D. Linde and V. Mukhanov, “The Curvaton Web,” JCAP 0604
2006
Cited alongside, same era.
Cited in the paper.
Cited in the paper.