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Emergent dark energy from unparticles

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arxiv 2010.02998 v2 pith:BMA3R627 submitted 2020-10-06 hep-ph astro-ph.COgr-qchep-th

classification hep-phastro-ph.COgr-qchep-th
keywords modelunparticlesbehavioremergentenergieslimitingtemperatureyielding
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A limiting temperature of a species can cause the Universe to asymptote to it yielding a deSitter (dS) phase due to macroscopic emergent behavior. The limiting temperature is generic for theories slightly shifted from their conformal point. We demonstrate such behavior in the example of unparticles/Banks-Zaks theory. The unparticles behave like radiation at high energies reducing the Hubble tension, and a cosmological constant (CC) at low energies yielding a model that follows closely {\Lambda}CDM model but due to collective phenomenon. It is technically natural and avoids the no-dS conjecture. The model is free of the coincidence and initial conditions problems, of scalar fields and of modified gravity.

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  1. Evidence for non-cold dark matter from DESI DR2 measurements

    astro-ph.CO 2025-04 reject novelty 5.0 of 10

    DESI BAO plus DES-Y5 supernovae favor a slightly negative dark matter equation of state at 2.4 sigma, but combining with Planck moves the best fit to a positive value, exposing a dataset-dependent tension.

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