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Detectable and Defect-Free Dark Photon Dark Matter,

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

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2026 3 2025 1

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representative citing papers

Early Growth of Structure in Warm Wave Dark Matter

astro-ph.CO · 2025-06-13 · conditional · novelty 6.0

Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.

Dark Photons from Red Dwarfs

hep-ph · 2026-06-24 · unverdicted · novelty 5.0

Red dwarf mass-radius data from eclipsing binaries combined with dark-photon-inclusive evolution simulations produce competitive constraints on light dark photons.

citing papers explorer

Showing 4 of 4 citing papers.

  • Early Growth of Structure in Warm Wave Dark Matter astro-ph.CO · 2025-06-13 · conditional · none · ref 22

    Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.

  • Dark Photons from Red Dwarfs hep-ph · 2026-06-24 · unverdicted · none · ref 30

    Red dwarf mass-radius data from eclipsing binaries combined with dark-photon-inclusive evolution simulations produce competitive constraints on light dark photons.

  • Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves hep-ph · 2026-05-20 · unverdicted · none · ref 53

    Axion-like particles in the trapped misalignment mechanism produce observable gravitational waves while generating intergalactic magnetic fields that exceed blazar lower bounds in the parameter space promising for gravitational wave detection.

  • Dilaton-Induced Resonant Production of Ultralight Vector Dark Matter hep-ph · 2026-04-22 · unverdicted · none · ref 31

    Resonant dilatonic coupling produces ultralight vector dark matter with relic mass scaling as m_γ' ∝ r_i^{-2} for subdominant spectators in radiation-dominated backgrounds.