Wide-band full-wave electromagnetic modal analysis of the coupling between dark-matter axions and photons in microwave resonators

Navarro, P. ; Gimeno, Benito ; Álvarez Melcón, A. ; Arguedas Cuendis, S. ; Cogollos, C. ; Díaz-Morcillo, A. ; Gallego, J.D. ; García Barceló, J.M. ; Golm, J. ; Irastorza, I.G. (Universidad de Zaragoza) ; Lozano Guerrero, A.J. ; Peña Garay, C.

Resumen: The electromagnetic coupling axion–photon in a microwave cavity is revisited with the Boundary Integral-Resonant Mode Expansion (BI-RME) 3D technique. Such full-wave modal technique has been applied for the rigorous analysis of the excitation of a microwave cavity with an axion field. In this scenario, the electromagnetic field generated by the axion–photon coupling can be assumed to be driven by equivalent electrical charge and current densities. These densities have been inserted in the general BI-RME 3D equations, which express the RF electromagnetic field existing within a cavity as an integral involving the Dyadic Green''s functions of the cavity (under Coulomb gauge) as well as such densities. This method is able to take into account any arbitrary spatial and temporal variation of both magnitude and phase of the axion field. Next, we have obtained a simple network driven by the axion current source, which represents the coupling between the axion field and the resonant modes of the cavity. With this approach, it is possible to calculate the extracted and dissipated RF power as a function of frequency along a broad band and without Cauchy–Lorentz approximations, obtaining the spectrum of the electromagnetic field generated in the cavity, and dealing with modes relatively close to the axion resonant mode. Moreover, with this technique we have a complete knowledge of the signal extracted from the cavity, not only in magnitude but also in phase. This can be an interesting issue for future analysis where the axion phase is an important parameter.

Idioma: Inglés

DOI: 10.1016/j.dark.2022.101001

Año: 2022

Publicado en: Physics of the Dark Universe 36 (2022), 101001 [14 pp.]
ISSN: 2212-6864

Factor impacto JCR: 5.5 (2022)

Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 13 / 69 = 0.188 (2022) - Q1 - T1

Factor impacto CITESCORE: 9.4 - Earth and Planetary Sciences (Q1) - Physics and Astronomy (Q1)

Factor impacto SCIMAGO: 1.431 - Space and Planetary Science (Q1) - Astronomy and Astrophysics (Q1)

Financiación: info:eu-repo/grantAgreement/ES/AEI/BES-2017-079787
Financiación: info:eu-repo/grantAgreement/ES/AEI/PID2019-108122GB-C32
Financiación: info:eu-repo/grantAgreement/EUR/ERC-2018-StG-802836-AxScale
Financiación: info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2016-76978-C3-2-P

Tipo y forma: Artículo (Versión definitiva)

Área (Departamento): Área Física Atóm.Molec.y Nucl. (Dpto. Física Teórica)