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Power Spectrum in the Chaotic Regime of Axionic Blue Isocurvature Perturbations

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arxiv 2309.17010 v1 pith:PM33I32E submitted 2023-09-29 astro-ph.CO hep-ph

classification astro-ph.COhep-ph
keywords isocurvaturesymmetryanalyticbluebreakingfieldperturbationspotential
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Large blue tilted spectral index axionic isocurvature perturbations can be produced when the axion sector is far out of equilibrium during inflation through an initial Peccei-Quinn (PQ) symmetry breaking field displacement along a nearly flat direction in the effective potential. As a companion to a previous work, we present analytic formulae for the blue isocurvature spectrum for the case of the kinetic energy density of the PQ symmetry breaking field being larger than the quartic power of the final spontaneous PQ symmetry breaking scale. It corresponds to a regime in which the nonlinearities of the classical potential become important many times during the formation of the axion isocurvature quantum perturbations leading to interesting resonant behavior. One consequence of this nonlinearity-driven resonance is the chaotic nature of the map that links the underlying Lagrangian parameters to the isocurvature amplitudes. We point out an accidental duality symmetry between the perturbation equations and the background field equations that can be used to understand this. Finally, we present two types of analytic results. The first relies on a computation utilizing an effective potential wherein fast time scale fluctuations have been integrated out. The second is grounded in a functional ansatz, requiring only a limited set of fitting parameters. Both analytic results should be useful for carrying out forecasts and fits to the data.

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Cited by 2 Pith papers

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  2. Inflationary Axion Isocurvature in the CMB across All Ultralight Masses

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    Accurate axion-isocurvature evolution across the full ultralight mass range converts Planck and BICEP bounds into inflation-scale limits and reveals a small discovery window near m_a ~ 10^-25 eV.

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