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Fingerprints of a Non-Inflationary Universe from Massive Fields

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arxiv 2405.11016 v2 pith:XX54PPLX submitted 2024-05-17 astro-ph.CO gr-qchep-phhep-th

classification astro-ph.COgr-qchep-phhep-th
keywords contractingfieldsprimordialsignalsslowlyuniverseclocksekpyrotic
verification ladder T0 review T1 audit T2 compute T3 formal
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We construct explicit models of classical primordial standard clocks in an alternative to inflation, namely the slowly contracting ekpyrotic scenario. We study the phenomenology of massive spectator fields added to a state-of-the-art ekpyrotic model, with coupling functions that allow for these heavy fields to be classically excited while the background is slowly contracting. We perform numerical computations of the corrections to the scalar primordial power spectrum and compare with analytical estimates. Our full numerical results reveal so-called clock signals, sharp feature signals, as well as signals that link the two together. The models are found to predict oscillatory features that are resolutely different from what is calculated in inflation, and thus, such features represent unique fingerprints of a slowly contracting universe. This confirms the capability of primordial standard clocks to model-independently discriminate among very early universe scenarios.

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Cited by 3 Pith papers

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  1. Non-Relativistic Cosmological Collider Signals

    hep-ph 2026-05 unverdicted novelty 6.0 of 10

    Non-relativistic propagation of a tilted-ghost spectator field during inflation produces boostless cosmological collider non-Gaussianity via an effective chemical-potential-like tilt parameter.

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    hep-ph 2026-04 unverdicted novelty 6.0 of 10

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    astro-ph.GA 2026-03 unverdicted novelty 6.0 of 10

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