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Primordial non-Gaussianity encodes valuable information about the physics of inflation, including the spectrum of particles and interactions.
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V. Assassi, D. Baumann, D. Green, and M. Zaldarriaga, “Renormalized Halo Bias,” JCAP
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2014
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V. Assassi, D. Baumann, D. Green, and L. McAllister, “Planck-Suppressed Operators,” JCAP
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N. Craig and D. Green, “Testing Split Supersymmetry with Inflation,” JHEP
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L. Dai, E. Pajer, and F. Schmidt, “On Separate Universes,” JCAP
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J. Byun and R. Bean, “Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys,” JCAP
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V. Assassi, D. Baumann, and F. Schmidt, “Galaxy bias and primordial non-Gaussianity,” JCAP
2015
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M. Mirbabayi, F. Schmidt, and M. Zaldarriaga, “Biased tracers and time evolution,” JCAP
2015
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L. Senatore, “Bias in the effective field theory of large scale structures,” JCAP
2015
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