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Inflation models make specific predictions for a tensor-scalar-scalar three-point correlation, or bispectrum, between one gravitational-wave (tensor) mode and two density-perturbation (scalar) modes.
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2008
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D. Hanson and A. Lewis, “Estimators for CMB Statistical Anisotropy,” Phys. Rev. D 80
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2009
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2013
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2013
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2013
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S. Endlich, A. Nicolis and J. Wang, “Solid Inflation,” JCAP 1310
2013
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N. Bartolo, S. Matarrese, M. Peloso and A. Ricciardone, “Anisotropy in solid inflation,” JCAP 1308
2013
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2013
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2013
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2013
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2013
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2014
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2014
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A. Kehagias and A. Riotto, “Conformal Symmetries of FRW Accelerating Cosmologies,” Nucl. Phys. B 884
2014
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S. Kundu, “Non-Gaussianity Consistency Relations, Initial States and Back-reaction,” JCAP 1404
2014
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