Induced gravitational waves in a general cosmological background

Gravitational waves (GWs) are inevitably produced by second-order terms in cosmological perturbation theory. Most notably, the so-called induced (GWs) are a window to the small scales part of the primordial spectrum of fluctuations and a key counterpart to the primordial black hole (PBH) scenario. H...

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Main Author: Domènech Fuertes, Guillem (Author)
Format: Article (Journal)
Language:English
Published: 12 February 2020
In: International journal of modern physics
Year: 2020, Volume: 29, Issue: 3
ISSN:1793-6594
DOI:10.1142/S0218271820500285
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1142/S0218271820500285
Verlag, lizenzpflichtig, Volltext: https://www.worldscientific.com/doi/abs/10.1142/S0218271820500285
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Author Notes:Guillem Domènech
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Summary:Gravitational waves (GWs) are inevitably produced by second-order terms in cosmological perturbation theory. Most notably, the so-called induced (GWs) are a window to the small scales part of the primordial spectrum of fluctuations and a key counterpart to the primordial black hole (PBH) scenario. However, semi-analytical solutions are only known for matter and radiation domination eras. In this paper, we present new analytic integral formulas for the induced GWs on subhorizon scales in a general cosmological background with a constant equation-of-state. We also discuss applications to a peaked primordial scalar power spectrum and the PBH scenario.
Item Description:Gesehen am 09.04.2020
Physical Description:Online Resource
ISSN:1793-6594
DOI:10.1142/S0218271820500285