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Part of the book series: Springer Theses ((Springer Theses))

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Abstract

In this thesis, we studied the role of the second-order vector mode in the cosmological perturbation theory. The vector mode has been paid less attention so far since the vector mode has only decaying solution in the first-order perturbation theory.

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Reference

  1. BICEP2, Keck Array Collaboration, P.A.R. Ade et al., BICEP2/Keck Array VIII: measurement of gravitational lensing from large-scale B-mode polarization, arXiv:1606.01968

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Correspondence to Shohei Saga .

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Saga, S. (2018). Summary of This Thesis. In: The Vector Mode in the Second-order Cosmological Perturbation Theory. Springer Theses. Springer, Singapore. https://doi.org/10.1007/978-981-10-8007-4_6

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