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Discovery prospects with the Dark-photons & Axion-Like particles Interferometer

Javier De Miguel1,2,3,*, Juan F. Hernández-Cabrera2,3, Elvio Hernández-Suárez2,3, Enrique Joven-Álvarez2,3, Chiko Otani1, and J. Alberto Rubiño-Martín2,3 (On behalf of the DALI Collaboration)

  • 1The Institute of Physical and Chemical Research (RIKEN), Center for Advanced Photonics, 519-1399 Aramaki-Aoba, Aoba-ku, Sendai, Miyagi 980-0845, Japan
  • 2Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
  • 3Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

  • *javier.miguelhernandez@riken.jp

Phys. Rev. D 109, 062002 – Published 7 March, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.062002

Abstract

We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer in this paper. The apparatus, currently in a design and prototyping phase, will probe axion dark matter from the Teide Observatory, an environment protected from terrestrial microwave sources, reaching Dine-Fischler-Srednicki-Zhitnitsky-like axion sensitivity in the range 25–250  μeV of mass. The experimental approach shows a potential to probe dark sector photons of kinetic mixing strength in excess of several 10−16 and to establish new constraints to a stochastic gravitational wave background in its band. We identify different branches, including cosmology, stellar, and particle physics, where this next-generation halo-telescope may play a role in coming years.

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Corrections

29 March, 2024

Correction: The title and abstract contained typographical errors that have been fixed. Three author names in Ref. [80] were presented incorrectly and have been fixed. References [205]–[210] were erroneously removed from the reference list during the production cycle and have been restored. Citations for those references have been inserted in Ref. [96]. Correspondingly, the Supplemental Material has been fixed to align with the reference citations in the corrected paper.

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