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Stasis Combs: Gravitational-Wave Signatures of Recurrent Cosmological Stasis

Gabriela Barenboim, Anne-Katherine Burns

hep-pharXiv:2609.20280

Abstract

Cosmological stasis can recur multiple times, and each occurrence imprints a characteristic feature on the inflationary gravitational wave background (IGWB). We extend the single-epoch spectral template to an arbitrary number N of consecutive stasis epochs, deriving a closed-form N-epoch piecewise template that factorizes cleanly: the amplitude steps at each break are determined entirely by the local equation of state ws(i) of that epoch, while the inter-epoch plateau levels encode the accumulated spectral tilt from all prior epochs. Each resolved spectral feature yields an independent test of the Bessel-function consistency relation C2 = C2(α) established in~BarenboimBurns:paper1, and the probability that N such tests are simultaneously satisfied by a non-stasis spectrum falls sharply with N, making a confirmed multi-epoch comb the strongest available discriminator against constant-w alternatives. We apply the formalism to the triple-stasis scenario of~Dienes:2023ziv, which chains three pairwise stasis mechanisms (matter/radiation, vacuum-energy/matter, vacuum-energy/radiation) sequentially. For each block we derive the conditions under which the epoch lies within the template's validity range ws > -1/3. We show that the Fig.~3 benchmark of~Dienes:2023ziv falls outside this range and identify parameter choices that are both physically realizable and accessible to the template. We validate the inter-plateau ratio predictions numerically for representative two- and three-block chains, and work out the touching-epoch limit in which consecutive blocks share a break frequency without an intervening radiation-dominated interval. Finally, we discuss the detectability of a variety of multi-epoch stasis scenarios and give the minimum detectable tensor-to-scalar ratio as a function of the number of recurrent stasis epochs.

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