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Primordial non-Gaussianity (NG) affects the large scale structure (LSS) of the universe by leaving an imprint on the distribution of matter at late times.
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D. Babich, P. Creminelli and M. Zaldarriaga, “The shape of non-Gaussianities,” JCAP
2004
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N. Bartolo, S. Matarrese and A. Riotto, “On non-Gaussianity in the curvaton scenario,” Phys. Rev. D
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G. Dvali, A. Gruzinov and M. Zaldarriaga, “A new mechanism for generating density perturbations from inflation,” Phys. Rev. D
2004
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M. Alishahiha, E. Silverstein and D. Tong, “DBI in the sky,” Phys. Rev. D
2004
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N. Arkani-Hamed, P. Creminelli, S. Mukohyama and M. Zaldarriaga, “Ghost Inflation,” JCAP
2004
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D. M. Goldberg, T. D. Jones, F. Hoyle, R. R. Rojas, M. S. Vogeley and M. R. Blanton, “The Mass Function of Void Galaxies in the SDSS Data Release 2,” Astrophys. J
2005
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F. Hoyle, M. S. Vogeley and R. R. Rojas, “Void Galaxies in the Sloan Digital SKy Survey,” Bulletin of the AAS
2005
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2008
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