Gravitational waves from fundamental axion dynamics
Abstract A totally asymptotically free QCD axion model, where all couplings flow to zero in the infinite energy limit, was recently formulated. A very interesting feature of this fundamental theory is the ability to predict some low-energy observables, like the masses of the extra fermions and scala...
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Online Access: | https://doi.org/10.1007/JHEP12(2020)049 |
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doaj-8f0b051594b941479f193eccebc3d14a2020-12-13T12:05:37ZengSpringerOpenJournal of High Energy Physics1029-84792020-12-0120201212710.1007/JHEP12(2020)049Gravitational waves from fundamental axion dynamicsAnish Ghoshal0Alberto Salvio1I.N.F.N. — Rome Tor VergataI.N.F.N. — Rome Tor VergataAbstract A totally asymptotically free QCD axion model, where all couplings flow to zero in the infinite energy limit, was recently formulated. A very interesting feature of this fundamental theory is the ability to predict some low-energy observables, like the masses of the extra fermions and scalars. Here we find and investigate a region of the parameter space where the Peccei-Quinn (PQ) symmetry is broken quantum mechanically through the Coleman-Weinberg mechanism. This results in an even more predictive framework: the axion sector features only two independent parameters (the PQ symmetry breaking scale and the QCD gauge coupling). In particular, we show that the PQ phase transition is strongly first order and can produce gravitational waves within the reach of future detectors. The predictivity of the model leads to a rigid dependence of the phase transition (like its duration and the nucleation temperature) and the gravitational wave spectrum on the PQ symmetry breaking scale and the QCD gauge coupling.https://doi.org/10.1007/JHEP12(2020)049Beyond Standard ModelCosmology of Theories beyond the SMRenormalization Group |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Anish Ghoshal Alberto Salvio |
spellingShingle |
Anish Ghoshal Alberto Salvio Gravitational waves from fundamental axion dynamics Journal of High Energy Physics Beyond Standard Model Cosmology of Theories beyond the SM Renormalization Group |
author_facet |
Anish Ghoshal Alberto Salvio |
author_sort |
Anish Ghoshal |
title |
Gravitational waves from fundamental axion dynamics |
title_short |
Gravitational waves from fundamental axion dynamics |
title_full |
Gravitational waves from fundamental axion dynamics |
title_fullStr |
Gravitational waves from fundamental axion dynamics |
title_full_unstemmed |
Gravitational waves from fundamental axion dynamics |
title_sort |
gravitational waves from fundamental axion dynamics |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2020-12-01 |
description |
Abstract A totally asymptotically free QCD axion model, where all couplings flow to zero in the infinite energy limit, was recently formulated. A very interesting feature of this fundamental theory is the ability to predict some low-energy observables, like the masses of the extra fermions and scalars. Here we find and investigate a region of the parameter space where the Peccei-Quinn (PQ) symmetry is broken quantum mechanically through the Coleman-Weinberg mechanism. This results in an even more predictive framework: the axion sector features only two independent parameters (the PQ symmetry breaking scale and the QCD gauge coupling). In particular, we show that the PQ phase transition is strongly first order and can produce gravitational waves within the reach of future detectors. The predictivity of the model leads to a rigid dependence of the phase transition (like its duration and the nucleation temperature) and the gravitational wave spectrum on the PQ symmetry breaking scale and the QCD gauge coupling. |
topic |
Beyond Standard Model Cosmology of Theories beyond the SM Renormalization Group |
url |
https://doi.org/10.1007/JHEP12(2020)049 |
work_keys_str_mv |
AT anishghoshal gravitationalwavesfromfundamentalaxiondynamics AT albertosalvio gravitationalwavesfromfundamentalaxiondynamics |
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1724385335338598400 |