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General Formalism for the CMB Bispectrum from Primordial Scalar, Vector and Tensor Non-Gaussianities

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Book cover Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum

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Abstract

In this chapter, on the basis of the formulation of the CMB anisotropy in Chap. 3, we develop the formulae for the CMB bispectrum sourced from scalar-, vector-, and tensor-mode non-Gaussianity.

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Notes

  1. 1.

    Here, we set \(0^0 = 1\).

References

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Correspondence to Maresuke Shiraishi .

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Shiraishi, M. (2013). General Formalism for the CMB Bispectrum from Primordial Scalar, Vector and Tensor Non-Gaussianities. In: Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum. Springer Theses. Springer, Tokyo. https://doi.org/10.1007/978-4-431-54180-6_5

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