Journal article 90 views 22 downloads
Non-Gaussianities and the large |η| approach to inflation
Physical Review D, Volume: 109, Issue: 6
Swansea University Author:
Gianmassimo Tasinato
-
PDF | Version of Record
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.
Download (1.24MB)
DOI (Published version): 10.1103/physrevd.109.063510
Abstract
The physics of primordial black holes can be affected by the non-Gaussian statistics of the density fluctuations that generate them. Therefore, it is important to have good theoretical control of the higher-order correlation functions for primordial curvature perturbations. By working at leading ord...
| Published in: | Physical Review D |
|---|---|
| ISSN: | 2470-0010 2470-0029 |
| Published: |
American Physical Society (APS)
2024
|
| Online Access: |
Check full text
|
| URI: | https://cronfa.swan.ac.uk/Record/cronfa65789 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| Abstract: |
The physics of primordial black holes can be affected by the non-Gaussian statistics of the density fluctuations that generate them. Therefore, it is important to have good theoretical control of the higher-order correlation functions for primordial curvature perturbations. By working at leading order in a 1/|η| expansion, we analytically determine the bispectrum of curvature fluctuations for single field inflationary scenarios producing primordial black holes. The bispectrum has a rich scale and shape dependence, and its features depend on the dynamics of the would-be decaying mode. We apply our analytical results to study gravitational waves induced at second order by enhanced curvature fluctuations. Their statistical properties are derived in terms of convolution integrals over wide momentum ranges, and they are sensitive on the scale and shape dependence of the curvature bispectrum we analytically computed. |
|---|---|
| College: |
Faculty of Science and Engineering |
| Funders: |
Funded by SCOAP |
| Issue: |
6 |