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PreprintarXiv licencearXiv

Constraining Multiple Kinetically Mixed Dark Photons

Abstract

Extra U(1) gauge bosons under which Standard Model particles are uncharged, aka dark photons, are a simple and well-motivated extension of the Standard Model. There could be a single, but also several or even many such dark photons. However, most studies consider only a single dark photon. Here, we want to look at the more general case of multiple dark photons interacting with the Standard Model via kinetic mixing. We consider a range of standard probes, Cavendish experiments, light-shining-through-walls experiments, as well as energy loss in stars. To explore the rather high-dimensional parameter space of the masses and the kinetic mixing matrix, we pursue a statistical approach, considering different distributions for the kinetic mixing parameters.

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BibTeX
@misc{jaeckel2026constraining,
  title = {{Constraining Multiple Kinetically Mixed Dark Photons}},
  author = {Joerg Jaeckel and Sebastian Monath},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2606.26240},
  eprint = {2606.26240},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2606.26240},
}
RIS
TY  - UNPB
TI  - Constraining Multiple Kinetically Mixed Dark Photons
AU  - Joerg Jaeckel
AU  - Sebastian Monath
PY  - 2026
DA  - 2026/10/22
PB  - arXiv
DO  - 10.48550/arxiv.2606.26240
UR  - https://arxiv.org/abs/2606.26240
AB  - Extra U(1) gauge bosons under which Standard Model particles are uncharged, aka dark photons, are a simple and well-motivated extension of the Standard Model. There could be a single, but also several or even many such dark photons. However, most studies consider only a single dark photon. Here, we want to look at the more general case of multiple dark photons interacting with the Standard Model via kinetic mixing. We consider a range of standard probes, Cavendish experiments, light-shining-through-walls experiments, as well as energy loss in stars. To explore the rather high-dimensional parameter space of the masses and the kinetic mixing matrix, we pursue a statistical approach, considering different distributions for the kinetic mixing parameters.
ER  -