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Cosmological Constraint on Dark Photon from $N_{\rm eff}$

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arxiv 1912.12152 v3 pith:MX7N77KI submitted 2019-12-27 hep-ph

classification hep-ph
keywords photondarkconstraintcosmologicalmathcalneutrinoaccordinglyannihilation
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

A new U(1) gauge symmetry is the simplest extension of the Standard Model and has various theoretical and phenomenological motivations. In this paper, we study the cosmological constraint on the MeV scale dark photon. After the neutrino decoupling era at $T = \mathcal{O}(1)\,$MeV, the decay and annihilation of the dark photon heats up the electron and photon plasma and accordingly decreases the effective number of neutrino $N_{\mathrm{eff}}$ in the recombination era. We derive a conservative lower-limit of the dark photon mass around 8.5 MeV from the current Planck data if the mixing between the dark photon and ordinary photon is larger than $\mathcal{O}(10^{-9})$. We also find that the future CMB stage-$\rm I\! V$ experiments can probe up to 17 MeV dark photon.

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Forward citations

Cited by 6 Pith papers

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

  1. Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    CMB-S4 forecasts: the two-site design reaches sigma(Neff)=0.029 in seven years, the Chile-only revised design reaches 0.030 in nine, and a cosmic-variance-limited survey would reach 0.0073.

  2. Light Dark Matter Discovery Potential and Model Selection at LDMX

    hep-ph 2026-07 conditional novelty 6.0 of 10

    LDMX Phase II is projected to discover R=2.5 thermal complex-scalar DM at 5σ and to discriminate dark-photon electromagnetic-moment models via 2D Bayes factors.

  3. Dark Photons in the Early Universe: From Thermal Production to Cosmological Constraints

    hep-ph 2025-12 conditional novelty 6.0 of 10

    Dark photon thermal production is computed analytically, yielding a fixed 4πe/27 ≈ 0.14 resonance-to-inverse-decay ratio and new cosmological limits down to ε~10^-12 over 0.1–6 MeV.

  4. Composite asymmetric dark matter with a dark photon portal: Multimessenger tests

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Decaying composite dark matter in the 1 to 10 GeV mass range is most strongly constrained by AMS-02 positron data, needing lifetimes above roughly 10^26 seconds.

  5. Direct Detection and Cosmological Constraints of Dark Matter with Dark Dipoles

    hep-ph 2026-02 conditional novelty 5.0 of 10

    Cosmological and direct-detection data already exclude most sub-GeV dark-matter parameter space for dark-photon magnetic dipole interactions, with semiconductor detectors needed to probe the remaining electric-dipole ...

  6. Blazar Boosted ALP and vector portal Dark matter confronting light mediator searches

    hep-ph 2025-01 conditional novelty 4.0 of 10

    Blazar-boosted dark matter scattering in Super-Kamiokande can exclude previously unconstrained parameter space for ALP- and vector-mediated sub-MeV dark matter, beating BaBar, NA64, beam dump, and stellar cooling limi...

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