No Inv.: 11347/P/Perp/98/1c
No Inv.: 2394/Perp/89/1c~3492-3493/P/Perp/91/2c~2551-2555/P/Perp/95/5c~487-491/P/Perp/98/5c
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 perturbations and include the violation of the rotational or parity invariance. On the basis of our c…
Bibliografi : hlm. 247-287
Bibliograhi : hlm. 769-776
Bibliografi : hlm. 141-142
Bibliografi : hlm. 213-218 No Inv.: 137286,137289/P/Perp/13/5c
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