Gravitational waves from fundamental axion dynamics

被引:0
作者
Anish Ghoshal
Alberto Salvio
机构
[1] I.N.F.N. — Rome Tor Vergata,Physics Department
[2] I.N.F.N.,undefined
[3] Laboratori Nazionali di Frascati,undefined
[4] University of Rome Tor Vergata,undefined
来源
Journal of High Energy Physics | / 2020卷
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Renormalization Group;
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摘要
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.
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共 232 条
[1]  
Peccei RD(1977) { Phys. Rev. Lett. 38 1440-undefined
[2]  
Quinn HR(1978)} Phys. Rev. Lett. 40 223-undefined
[3]  
Weinberg S(1983)undefined Phys. Lett. B 120 127-undefined
[4]  
Preskill J(1983)undefined Phys. Lett. B 120 133-undefined
[5]  
Wise MB(1983)undefined Phys. Lett. B 120 137-undefined
[6]  
Wilczek F(2020)undefined Phys. Rept. 870 1-undefined
[7]  
Abbott LF(2020)undefined JHEP 04 025-undefined
[8]  
Sikivie P(2020)undefined JHEP 04 195-undefined
[9]  
Dine M(2016)undefined Phys. Rev. D 93 104001-undefined
[10]  
Fischler W(2019)undefined JHEP 07 146-undefined