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• W4293117789 abstract "Abstract We show that the contribution of the primordial trispectrum to the energy density of the scalar-induced stochastic gravitational wave background cannot exceed the one from the scalar power spectrum in conventional inflationary scenarios. Specifically, we prove in the context of scale-invariant theories that neither regular trispectrum shapes peaking in so-called equilateral configurations, nor local trispectrum shapes diverging in soft momentum limits, can contribute significantly. Indeed, those contributions are always bound to be smaller than an order-one (or smaller) number multiplying the relative one-loop correction to the scalar power spectrum, necessarily much smaller than unity in order for the theory to be under perturbative control. Since a no-go theorem is only worth its assumptions, we also briefly discuss a toy model for a scale-dependent scalar spectrum, which confirms the robustness of our no-go result." @default.
• W4293117789 created "2022-08-26" @default.
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• W4293117789 date "2023-03-01" @default.
• W4293117789 modified "2023-10-01" @default.
• W4293117789 title "No-go theorem for scalar-trispectrum-induced gravitational waves" @default.
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• W4293117789 doi "https://doi.org/10.1088/1475-7516/2023/03/057" @default.
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