000136307 001__ 136307
000136307 005__ 20240731105612.0
000136307 0247_ $$2doi$$a10.1088/1475-7516/2024/06/070
000136307 0248_ $$2sideral$$a139181
000136307 037__ $$aART-2024-139181
000136307 041__ $$aeng
000136307 100__ $$aO'Shea, T.
000136307 245__ $$aProspects on the detection of solar dark photons by the International Axion Observatory
000136307 260__ $$c2024
000136307 5060_ $$aAccess copy available to the general public$$fUnrestricted
000136307 5203_ $$aDark (hidden) photons are widely recognised as well motivated candidates for physics beyond the standard model, and have been invoked for the solution of several outstanding problems, including to account for the dark matter in the universe. In this paper, we consider a simple model for dark photons, which is coupled to ordinary matter only through kinetic mixing with ordinary photons. Within this framework, we calculate the flux of solar dark photons on Earth and revise the potential to detect it with the next generation of axion helioscopes, particularly with the International AXion Observatory (IAXO). This paper extends on previous theoretical analyses in two main ways. Firstly, it includes a more complete analysis of the possible sources of dark photons from the sun, including the contribution of the solar magnetic field and of nuclear processes, and secondly it includes predictions on the parameter space accessible in the gas-filled phase of IAXO
000136307 536__ $$9info:eu-repo/grantAgreement/ES/AEI/PID2019-108122GB-C32$$9info:eu-repo/grantAgreement/EUR/ERC-2017-AdG-788781$$9info:eu-repo/grantAgreement/ES/MCIN/AEI/10.13039/501100011033$$9info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21
000136307 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000136307 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000136307 700__ $$aGiannotti, M.$$uUniversidad de Zaragoza
000136307 700__ $$0(orcid)0000-0003-1163-1687$$aGarcia Irastorza, I.$$uUniversidad de Zaragoza
000136307 700__ $$aPlasencia, L.M.
000136307 700__ $$aRedondo, J.
000136307 700__ $$0(orcid)0000-0002-3253-7027$$aRuz, J.$$uUniversidad de Zaragoza
000136307 700__ $$0(orcid)0000-0002-5850-5517$$aVogel, J.K.$$uUniversidad de Zaragoza
000136307 7102_ $$12004$$2038$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Astronomía y Astrofísica
000136307 7102_ $$12004$$2390$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Atóm.Molec.y Nucl.
000136307 773__ $$g2024, 06 (2024), 26 pp.$$pJ. Cosmol. Astropart. Phys.$$tJournal of Cosmology and Astroparticle Physics$$x1475-7516
000136307 8564_ $$s1931406$$uhttps://zaguan.unizar.es/record/136307/files/texto_completo.pdf$$yVersión publicada
000136307 8564_ $$s624371$$uhttps://zaguan.unizar.es/record/136307/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000136307 909CO $$ooai:zaguan.unizar.es:136307$$particulos$$pdriver
000136307 951__ $$a2024-07-31-09:22:39
000136307 980__ $$aARTICLE