Home > Observing axion potentials through gravitational waves |
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Title | Observing axion potentials through gravitational waves | ||||||||||
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Author(s) | Sfakianakis, Evangelos (speaker) (University of Illinois at Urbana-Champaign) | ||||||||||
Corporate author(s) | CERN. Geneva | ||||||||||
Imprint | 2019-06-25. - 0:17:57. | ||||||||||
Series | (Conferences & Workshops) (String Phenomenology 2019) | ||||||||||
Lecture note | on 2019-06-25T16:45:00 | ||||||||||
Subject category | Conferences & Workshops | ||||||||||
Abstract | I will discuss the the production of gravitational waves which are sourced by the tensor perturbation of SU(2) gauge fields coupled to a spectator axion field. Even though string theory constructions provide a variety of potentials, they can be categorized based on the number of non-stationary inflection points. I will present the resulting GW templates arising from each potential type. I will focus on the case of a modulated (axion monodromy) potential and show how future observations of CMB B-modes can probe the oscillatory behavior of an axion potential, thus shedding light into the underlying string theory construction. | ||||||||||
Copyright/License | © 2019-2024 CERN | ||||||||||
Submitted by | elena.gianolio@cern.ch |