Non-Gaussianities in extended D-term inflation
APA
Bernardeau, F. (2008). Non-Gaussianities in extended D-term inflation. Perimeter Institute. https://pirsa.org/08060132
MLA
Bernardeau, Francis. Non-Gaussianities in extended D-term inflation. Perimeter Institute, Jun. 03, 2008, https://pirsa.org/08060132
BibTex
@misc{ pirsa_PIRSA:08060132, doi = {10.48660/08060132}, url = {https://pirsa.org/08060132}, author = {Bernardeau, Francis}, keywords = {Quantum Fields and Strings, Particle Physics, Cosmology}, language = {en}, title = {Non-Gaussianities in extended D-term inflation}, publisher = {Perimeter Institute}, year = {2008}, month = {jun}, note = {PIRSA:08060132 see, \url{https://pirsa.org}} }
Institut d'Astrophysique de Paris
Collection
Talk Type
Abstract
I will present extensions of hybrid inflationary models in the context of supersymmetric D-term in- flation. I will show that there exists a large domain of parameters in which significant primordial non-Gaussianities can be produced while preserving a scale free power spectrum for the metric fluctuations. In particular I will explicitly present the expected bi- and trispectrum for such models and compared the results to the current and expected observational constraints. It is to be noticed that it is necessary to use both the bi- and tri-spectra of CMB anisotropies to efficiently reduce the parameter space of such models.