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New Universal Local Feature in the Inflationary Perturbation Spectrum

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arxiv 0711.1585 v3 pith:WAXOYDMH submitted 2007-11-12 astro-ph gr-qchep-phhep-th

classification astro-phgr-qchep-phhep-th
keywords indexinflationaryinflatonsecondspectraltransitionfastinflation
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A model is developed in which the inflaton potential experiences a sudden small change in its second derivative (the effective mass of the inflaton). An exact treatment demonstrates that the resulting density perturbation has a quasi-flat power spectrum with a break in its slope (a step in n_s). The step in the spectral index is modulated by characteristic oscillations and results in large running of the spectral index localised over a few e-folds of scales. A field-theoretic model giving rise to such behaviour of the inflationary potential is based on a fast phase transition experienced by a second scalar field weakly coupled to the inflaton. Such a transition is similar to that which terminates inflation in the hybrid inflationary scenario. This scenario suggests that the observed running of the spectral index in the WMAP data may be caused by a fast second order phase transition which occurred during inflation.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Primordial Sharp Features through the Nonlinear Regime of Structure Formation

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    Sharp primordial features survive nonlinear structure formation as localised bumps or dips in the matter power spectrum, while their oscillatory patterns are erased, leaving an oscillatory imprint in the halo mass function.

  2. Reheating constraints to modulus mass for single field inflationary models

    astro-ph.CO 2019-08 reject novelty 4.0 of 10

    A scale-counting argument linking modulus mass to reheating parameters yields quoted bounds m_chi >~ 10^12 to 10^15 GeV that are not supported by the printed equations.

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