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Observing axion potentials through gravitational waves
<!--HTML-->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...
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Lenguaje: | eng |
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2019
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Acceso en línea: | http://cds.cern.ch/record/2681464 |
_version_ | 1780963036848193536 |
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author | Sfakianakis, Evangelos |
author_facet | Sfakianakis, Evangelos |
author_sort | Sfakianakis, Evangelos |
collection | CERN |
description | <!--HTML-->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. |
id | cern-2681464 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | cern-26814642022-11-02T22:21:39Zhttp://cds.cern.ch/record/2681464engSfakianakis, EvangelosObserving axion potentials through gravitational wavesString Phenomenology 2019Conferences & Workshops<!--HTML-->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.oai:cds.cern.ch:26814642019 |
spellingShingle | Conferences & Workshops Sfakianakis, Evangelos Observing axion potentials through gravitational waves |
title | Observing axion potentials through gravitational waves |
title_full | Observing axion potentials through gravitational waves |
title_fullStr | Observing axion potentials through gravitational waves |
title_full_unstemmed | Observing axion potentials through gravitational waves |
title_short | Observing axion potentials through gravitational waves |
title_sort | observing axion potentials through gravitational waves |
topic | Conferences & Workshops |
url | http://cds.cern.ch/record/2681464 |
work_keys_str_mv | AT sfakianakisevangelos observingaxionpotentialsthroughgravitationalwaves AT sfakianakisevangelos stringphenomenology2019 |