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...
Κύριος συγγραφέας: | |
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Συγγραφή απο Οργανισμό/Αρχή: | |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Tokyo :
Springer Japan : Imprint: Springer,
2013.
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Σειρά: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- 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.