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Accelerated cosmic expansion, mass creation, and the QCD axion

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arxiv 2405.00090 v2 pith:SOOJBMEP submitted 2024-04-30 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords creationvarphiaxioncosmicaccelerationenergyexpansioninitial
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abstract

We propose a mechanism in which the current acceleration of cosmic expansion is driven by continuous creation of energy density $\rho_b$ for a certain field $\varphi_b$. We accordingly modify Einstein equation, derive modified Friedmann equations and analyze the regimes in which cosmic acceleration occurs. The creation process requires $\rho_b\neq 0$ as initial condition, which we enforce by identifying $\varphi_b$ with the axion of a hidden gauge group that confined in recent cosmological times, leading to a level crossing between $\varphi_b$ and the QCD axion, which is assumed to comprise dark matter. The conversion of a small fraction of QCD axions into $\varphi_b$ shortly before matter-dark energy equality generates the initial $\rho_b$ needed to trigger the creation process and offers a solution to the coincidence puzzle.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Resonant Landau-Zener Conversion In Multi-Axion Systems

    hep-ph 2025-07 conditional novelty 6.0 of 10

    The paper derives a Landau-Zener conversion probability for non-adiabatic axion mass-level crossings and uses it to predict two-axion dark matter abundances and haloscope targets.

  2. Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters

    astro-ph.CO 2025-11 conditional novelty 5.0 of 10

    A two-cosine axion dark energy potential fits CMB+BAO+supernova data better than the standard one-cosine potential, while preferring a sub-Planckian decay constant and a feeble dark-matter coupling.

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