Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
The non-Gaussianity in the primordial density fluctuations is a key feature to clarify the early Universe and it has been probed with the Cosmic Microwave Background (CMB) bispectrum. In recent years, we have treated the novel-type CMB bispectra, which originate from the vector- and tensor-mode pert...
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Format: | Electronic |
Language: | English |
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Tokyo :
Springer Japan : Imprint: Springer,
2013.
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Series: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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Online Access: | https://ezaccess.library.uitm.edu.my/login?url=http://dx.doi.org/10.1007/978-4-431-54180-6 |
Table of Contents:
- Introduction
- Fluctuations in the inflation
- Fluctuations in�cosmic microwave background radiation
- Primordial non-Gaussianities
- General formalism for the CMB bispectrum from primordial scalar, vector and tensor non-Gaussianities
- CMB bispectrum Induced by the two scalars and a graviton correlator
- Violation of the rotational invariance in the CMB bispectrum
- Parity violation of gravitons in the CMB bispectrum
- CMB bispectrum generated from primordial magnetic fields
- Conclusion.