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...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριος συγγραφέας: Shiraishi, Maresuke (Συγγραφέας)
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: Tokyo : Springer Japan : Imprint: Springer, 2013.
Σειρά:Springer Theses, Recognizing Outstanding Ph.D. Research,
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.