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Smoking guns of a bounce in modified theories of gravity through the spectrum of the gravitational waves

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arxiv 1210.1761 v2 pith:EGJ54D33 submitted 2012-10-05 astro-ph.CO gr-qchep-th

classification astro-ph.COgr-qchep-th
keywords gravitationalactionmodifiedspectrumasymptoticallybouncegravityhilbert-einstein
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abstract

We present an inflationary model preceded by a bounce in a metric theory a l\'{a} $f(R)$ where $R$ is the scalar curvature of the space-time. The model is asymptotically de Sitter such that the gravitational action tends asymptotically to a Hilbert-Einstein action, therefore modified gravity affects only the early stages of the universe. We then analyse the spectrum of the gravitational waves through the method of the Bogoliubov coefficients by two means: taking into account the gravitational perturbations due to the modified gravitational action in the $f(R)$ setup and by simply considering those perturbations inherent to the standard Hilbert-Einstein action. We show that there are distinctive (oscillatory) signals on the spectrum for very low frequencies; i.e. corresponding to modes that are currently entering the horizon.

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

  1. Close Hyperbolic Encounters In f(R) Gravity

    gr-qc 2025-06 reject novelty 5.0 of 10

    In f(R) gravity, close hyperbolic black-hole encounters emit a scalar gravitational-wave mode whose promised detectability is not supported by the paper's own amplitude formulas.

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