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.
Here, we set \(0^0 = 1\).
References
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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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DOI: https://doi.org/10.1007/978-4-431-54180-6_5
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