Axion-induced pair production: A new strategy for axion detection
Resumen: We revisit and update the axion-induced pair production process in a nuclear electric field mediated by the axion-electron coupling, a+XZA→XZA+e++e−. This process emerges as one of the most efficient channels for detecting axions with energies above a few MeV in large underground detectors. It is particularly relevant for detecting axions produced in nuclear reactions, such as the p+d→He3+a(5.5  MeV) reaction in the solar pp-chain, and for axions originating in supernovae. Despite recent interest in detecting high-energy axions, the pair production process has received limited attention, even in scenarios where it is the dominant detection channel. This study fills this gap by demonstrating that pair production is a highly effective detection mechanism for high-energy axions. We apply our results to axions from supernovae and the solar 5.5 MeV line, recasting the current bounds of Borexino and comparing the detection capabilities of the JUNO and Hyper-Kamiokande detectors.
Idioma: Inglés
DOI: 10.1103/PhysRevD.111.043021
Año: 2025
Publicado en: Physical Review D 111, 4 (2025), 043021 [13 pp.]
ISSN: 2470-0010

Financiación: info:eu-repo/grantAgreement/EUR/ERC-2017-AdG-788781
Financiación: info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21
Financiación: info:eu-repo/grantAgreement/ES/MICINN/PID2019-108122GB-C31
Tipo y forma: Article (Published version)
Área (Departamento): Área Astronomía y Astrofísica (Dpto. Física Teórica)

Creative Commons 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.


Exportado de SIDERAL (2025-10-17-14:32:33)


Visitas y descargas

Este artículo se encuentra en las siguientes colecciones:
Articles > Artículos por área > Astronomía y astrofísica



 Record created 2025-02-27, last modified 2025-10-17


Versión publicada:
 PDF
Rate this document:

Rate this document:
1
2
3
 
(Not yet reviewed)