Non UBC
DSpace
Gianmassimo Tasinato
2019-10-27T09:07:13Z
2019-04-29T09:30
Cosmological inflation predicts the existence of a stochastic background of gravitational waves, whose features depend on the model of inflation under consideration. There exist well motivated frameworks predicting an enhancement of the primordial gravity wave spectrum at frequency scales testable with gravitational wave experiments, with distinctive features as parity violation and non-Gaussianity. I will explain the properties of such scenarios, and their distinctive predictions for what respect the gravity wave power spectrum and bispectrum. I will then discuss how to quantitatively test these predictions with current and future interferometers.
https://circle.library.ubc.ca/rest/handle/2429/72070?expand=metadata
50.0 minutes
video/mp4
Author affiliation: Swansea University Physics Department
Oaxaca (Mexico : State)
10.14288/1.0384856
eng
Unreviewed
Vancouver : University of British Columbia Library
Banff International Research Station for Mathematical Innovation and Discovery
Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
Researcher
BIRS Workshop Lecture Videos (Oaxaca (Mexico : State))
Mathematics
Relativity and gravitational theory
Quantum theory
String theory
Probing the Physics of the Early Universe with Gravitational Interferometers
Moving Image
http://hdl.handle.net/2429/72070