Observable Gravitational Waves from Hyperkination in Palatini Gravity and Beyond
Samuel S\'anchez L\'opez, Konstantinos Dimopoulos, Alexandros Karam,, and Eemeli Tomberg

TL;DR
This paper explores how a period of hyperkination in Palatini gravity affects primordial gravitational wave spectra, potentially making them observable without disrupting Big Bang Nucleosynthesis.
Contribution
It introduces the concept of hyperkination driven by quartic kinetic terms in Palatini gravity and analyzes its impact on gravitational wave spectra.
Findings
Hyperkination truncates the gravitational wave spectrum peak.
Kinetic domination enhances the gravitational wave amplitude.
Observable gravitational wave signals are possible within parameter space.
Abstract
We consider cosmology with an inflaton scalar field with an additional quartic kinetic term. Such a theory can be motivated by Palatini modified gravity. Assuming a runaway inflaton potential, we take the Universe to become dominated by the kinetic energy density of the scalar field after inflation. Initially, the leading kinetic term is quartic and we call the corresponding period hyperkination. Subsequently, the usual quadratic kinetic term takes over and we have regular kination, until reheating. We study, both analytically and numerically, the spectrum of primordial gravitational waves generated during inflation and re-entering the horizon during the subsequent eras. We demonstrate that the spectrum is flat for modes re-entering during radiation domination and hyperkination and linear in frequency for modes re-entering during kination: kinetic domination boosts the spectrum,…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
