The future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories
Alesini, David ; Babusci, Danilo ; Beltrame, Paolo ; Bossi, Fabio ; Ciambrone, Paolo ; D’Elia, Alessandro ; Di Gioacchino, Daniele ; Di Pirro, Giampiero ; Döbrich, Babette ; Falferi, Paolo ; Gatti, Claudio ; Giannotti, Maurizio (Universidad de Zaragoza) ; Gianotti, Paola ; Lamanna, Gianluca ; Ligi, Carlo ; Maccarrone, Giovanni ; Mazzitelli, Giovanni ; Mirizzi, Alessandro ; Mueck, Michael ; Nardi, Enrico ; Nguyen, Federico ; Rettaroli, Alessio ; Rezvani, Javad ; Teofilo, Francesco Enrico ; Tocci, Simone ; Tomassini, Sandro ; Visinelli, Luca ; Zantedeschi, Michael
Resumen: We present a proposal for a new experiment, the FINUDA magnet for Light Axion SearcH (FLASH), a large resonant-cavity haloscope in a high static magnetic field which is planned to probe new physics in the form of dark matter (DM) axions, scalar fields, chameleons, hidden photons, as well as high frequency gravitational waves (GWs). Concerning the QCD axion, FLASH will search for these particles as the DM in the mass range
, thus filling the mass gap between the ranges covered by other planned searches. A dedicated Microstrip SQUID operating at ultra-cryogenic temperatures will amplify the signal. The frequency range accessible overlaps with the Very High Frequency (VHF) range of the radio wave spectrum and allows for a search in GWs in the frequency range
MHz. The experiment will make use of the cryogenic plant and magnet of the FINUDA experiment at INFN Frascati National Laboratories near Rome (Italy); the operations needed to restore the functionalities of the apparatus are currently underway. We present the setup of the experiment and the sensitivity forecasts for the detection of axions, scalar fields, chameleons, hidden photons, and GWs.
Idioma: Inglés
DOI: 10.1016/j.dark.2023.101370
Año: 2023
Publicado en: Physics of the Dark Universe 42 (2023), 101370 [26 pp.]
ISSN: 2212-6864
Factor impacto JCR: 5.0 (2023)
Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 14 / 84 = 0.167 (2023) - Q1 - T1
Factor impacto CITESCORE: 9.6 - Space and Planetary Science (Q1) - Astronomy and Astrophysics (Q1)
Factor impacto SCIMAGO: 1.377 - Space and Planetary Science (Q1) - Astronomy and Astrophysics (Q1)
Tipo y forma: Article (PrePrint)
Área (Departamento): Área Astronomía y Astrofísica (Dpto. Física Teórica)
You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use. You may not use the material for commercial purposes. If you remix, transform, or build upon the material, you may not distribute the modified material.
Exportado de SIDERAL (2024-11-22-12:09:39)
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, thus filling the mass gap between the ranges covered by other planned searches. A dedicated Microstrip SQUID operating at ultra-cryogenic temperatures will amplify the signal. The frequency range accessible overlaps with the Very High Frequency (VHF) range of the radio wave spectrum and allows for a search in GWs in the frequency range
MHz. The experiment will make use of the cryogenic plant and magnet of the FINUDA experiment at INFN Frascati National Laboratories near Rome (Italy); the operations needed to restore the functionalities of the apparatus are currently underway. We present the setup of the experiment and the sensitivity forecasts for the detection of axions, scalar fields, chameleons, hidden photons, and GWs.
Idioma: Inglés
DOI: 10.1016/j.dark.2023.101370
Año: 2023
Publicado en: Physics of the Dark Universe 42 (2023), 101370 [26 pp.]
ISSN: 2212-6864
Factor impacto JCR: 5.0 (2023)
Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 14 / 84 = 0.167 (2023) - Q1 - T1
Factor impacto CITESCORE: 9.6 - Space and Planetary Science (Q1) - Astronomy and Astrophysics (Q1)
Factor impacto SCIMAGO: 1.377 - Space and Planetary Science (Q1) - Astronomy and Astrophysics (Q1)
Tipo y forma: Article (PrePrint)
Área (Departamento): Área Astronomía y Astrofísica (Dpto. Física Teórica)
You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use. You may not use the material for commercial purposes. If you remix, transform, or build upon the material, you may not distribute the modified material. Exportado de SIDERAL (2024-11-22-12:09:39)
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Record created 2024-02-19, last modified 2024-11-25