Discovery prospects with the Dark-photons & Axion-Like particles Interferometer
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| Autores principales: | , , , , , |
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| Formato: | Preprint |
| Publicado: |
2023
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| author | De Miguel, Javier Hernández-Cabrera, Juan F. Hernández-Suárez, Elvio Joven-Álvarez, Enrique Otani, Chiko Rubiño-Martín, J. Alberto |
| author_facet | De Miguel, Javier Hernández-Cabrera, Juan F. Hernández-Suárez, Elvio Joven-Álvarez, Enrique Otani, Chiko Rubiño-Martín, J. Alberto |
| contents | We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer (DALI) in this letter. 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2303_03997 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Discovery prospects with the Dark-photons & Axion-Like particles Interferometer De Miguel, Javier Hernández-Cabrera, Juan F. Hernández-Suárez, Elvio Joven-Álvarez, Enrique Otani, Chiko Rubiño-Martín, J. Alberto High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer (DALI) in this letter. 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. |
| title | Discovery prospects with the Dark-photons & Axion-Like particles Interferometer |
| topic | High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment |
| url | https://arxiv.org/abs/2303.03997 |