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Spikes in the Relic Graviton Background from Quintessential Inflation

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arxiv hep-ph/9903263 v1 pith:5QX567YU submitted 1999-03-05 hep-ph astro-phgr-qc

Massimo Giovannini (Tufts University , Institute of Cosmology) This is my paper · ORCID
classification hep-phastro-phgr-qc
keywords energyinflationarymodelsquintessentialrelicspectraspikearound
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abstract

The energy spectra of gravitational waves (GW) produced in quintessential inflationary models increase in frequency and exhibit a sharp spike around 170 GHz where the associated fraction of critical energy density today stored in relic gravitons is of the order of $10^{-6}$. We contrast our findings with the spectra of ordinary inflationary models and we comment about possible detetction strategies of the spike.

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    gr-qc 2024-12 accept novelty 6.0 of 10

    The LISA-TAIJIm configuration, with TAIJI's constellation inclined opposite to LISA's, is about an order of magnitude more sensitive to a circularly polarized stochastic gravitational wave background at low frequencie...

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