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Thermal Misalignment of Scalar Dark Matter

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arxiv 2109.04476 v1 pith:JRIL7TNR submitted 2021-09-09 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkmattermisalignmentmechanismscalarabundanceconventionalfield
verification ladder T0 review T1 audit T2 compute T3 formal
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The conventional misalignment mechanism for scalar dark matter depends on the initial field value, which governs the oscillation amplitude and present-day abundance. We present a mechanism by which a feeble (Planck-suppressed) coupling of dark matter to a fermion in thermal equilibrium drives the scalar towards its high-temperature potential minimum at large field values, dynamically generating misalignment before oscillations begin. Unlike conventional misalignment production, the dark matter abundance is dictated by microphysics and not by initial conditions. As an application of the generic mechanism, we discuss a realistic scenario in which dark matter couples to the muon.

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Forward citations

Cited by 4 Pith papers

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

  1. Thermal History of Non-equilibrated Scalars

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    Hyperlight quadratically coupled scalars making up a few percent of dark matter are bounded to near- or sub-gravitational couplings to electrons and photons over 10^-31 to 10^-28 eV, with quasar spectra setting the st...

  3. Minimal Majoron Dark Matter from a Discrete $Z_N$ Gauge Symmetry

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Discrete Z_N-protected majoron dark matter excludes Z_5, leaves Z_7/Z_11/Z_13 viable, and predicts a 1–10 MeV Z_7 majoron testable by COSI through 511 keV and γγ lines.

  4. Coherent and Stochastic Axion Dark Matter from Thermal Relaxation

    hep-ph 2026-08 conditional novelty 4.0 of 10

    Thermal relaxation of an axion field produces a dark matter relic whose coherent and stochastic parts share one optical depth, yielding a subthermal momentum spectrum.

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