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

Bibcode
2024PhRvD.109f2002D
DOI
10.1103/PhysRevD.109.062002
De Miguel, Javier; Hernández-Cabrera, Juan F.; Hernández-Suárez, Elvio; Joven-Álvarez, Enrique; Otani, Chiko; Alberto Rubiño-Martín, J.; DALI Collaboration
Referencia bibliográfica

Physical Review D

Fecha de publicación:
3
2024
Revista
Physical Review D
Número de autores
7
Número de autores del IAC
5
Número de citas
6
Número de citas referidas
4
Descripción
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 μ eV 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.
Tipo
Con árbitro

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