000079127 001__ 79127
000079127 005__ 20200716101425.0
000079127 0247_ $$2doi$$a10.1103/PhysRevD.99.035037
000079127 0248_ $$2sideral$$a111100
000079127 037__ $$aART-2019-111100
000079127 041__ $$aeng
000079127 100__ $$0(orcid)0000-0002-8921-910X$$aDafni, T.$$uUniversidad de Zaragoza
000079127 245__ $$aWeighing the solar axion
000079127 260__ $$c2019
000079127 5060_ $$aAccess copy available to the general public$$fUnrestricted
000079127 5203_ $$aAxion helioscopes search for solar axions and axionlike particles via inverse Primakoff conversion in strong laboratory magnets pointed at the Sun. While helioscopes can always measure the axion coupling to photons, the conversion signal is independent of the mass for axions lighter than around 0.02 eV. Masses above this value on the other hand have suppressed signals due to axion-photon oscillations which destroy the coherence of the conversion along the magnet. However, the spectral oscillations present in the axion conversion signal between these two regimes are highly dependent on the axion mass. We show that these oscillations are observable given realistic energy resolutions and can be used to determine the axion mass to within percent-level accuracies. Using projections for the upcoming helioscope International Axion Observatory, we demonstrate that >3s sensitivity to a nonzero axion mass is possible between 3×10-3 and 10-1¿¿eV for both the Primakoff and axion-electron solar fluxes.
000079127 536__ $$9info:eu-repo/grantAgreement/EC/H2020/674896/EU/The Elusives Enterprise: Asymmetries of the Invisible Universe/ELUSIVES$$9This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 674896-ELUSIVES$$9info:eu-repo/grantAgreement/EC/H2020/788781/EU/Towards the detection of the axion with the International Axion Observatory/IAXOplus$$9This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 788781-IAXOplus$$9info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2015-65745-P$$9info:eu-repo/grantAgreement/ES/MINECO/FPA2013-41085-P$$9info:eu-repo/grantAgreement/ES/MINECO/FPA2016-76978-C3-1-P$$9info:eu-repo/grantAgreement/ES/MINECO/RYC-2012-10597
000079127 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000079127 590__ $$a4.833$$b2019
000079127 592__ $$a1.664$$b2019
000079127 591__ $$aPHYSICS, PARTICLES & FIELDS$$b6 / 29 = 0.207$$c2019$$dQ1$$eT1
000079127 593__ $$aPhysics and Astronomy (miscellaneous)$$c2019$$dQ1
000079127 591__ $$aASTRONOMY & ASTROPHYSICS$$b16 / 68 = 0.235$$c2019$$dQ1$$eT1
000079127 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000079127 700__ $$0(orcid)0000-0003-3803-9384$$aO'Hare, C. A. J.$$uUniversidad de Zaragoza
000079127 700__ $$aLakic, B.
000079127 700__ $$0(orcid)0000-0001-7529-9834$$aGalán, J.$$uUniversidad de Zaragoza
000079127 700__ $$0(orcid)0000-0001-6327-9369$$aIguaz, F. J.
000079127 700__ $$0(orcid)0000-0003-1163-1687$$aIrastorza, I. G.$$uUniversidad de Zaragoza
000079127 700__ $$aJakovcic, K.
000079127 700__ $$0(orcid)0000-0002-5352-1884$$aLuzón, G.$$uUniversidad de Zaragoza
000079127 700__ $$0(orcid)0000-0002-1044-8197$$aRedondo, J.$$uUniversidad de Zaragoza
000079127 700__ $$0(orcid)0000-0002-2417-7121$$aRuiz Chóliz, E.$$uUniversidad de Zaragoza
000079127 7102_ $$12004$$2405$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Teórica
000079127 7102_ $$12004$$2390$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Atóm.Molec.y Nucl.
000079127 773__ $$g99, 3 (2019), 035037 [13 pp.]$$pPhys. rev. D$$tPhysical Review D$$x2470-0010
000079127 8564_ $$s1612197$$uhttps://zaguan.unizar.es/record/79127/files/texto_completo.pdf$$yVersión publicada
000079127 8564_ $$s111640$$uhttps://zaguan.unizar.es/record/79127/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000079127 909CO $$ooai:zaguan.unizar.es:79127$$particulos$$pdriver
000079127 951__ $$a2020-07-16-08:44:24
000079127 980__ $$aARTICLE