79127 20200716101425.0 doi 10.1103/PhysRevD.99.035037 sideral 111100 ART-2019-111100 eng (orcid)0000-0002-8921-910X Dafni, T. Universidad de Zaragoza Weighing the solar axion 2019 Access copy available to the general public Unrestricted Axion 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. info:eu-repo/grantAgreement/EC/H2020/674896/EU/The Elusives Enterprise: Asymmetries of the Invisible Universe/ELUSIVES This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 674896-ELUSIVES info:eu-repo/grantAgreement/EC/H2020/788781/EU/Towards the detection of the axion with the International Axion Observatory/IAXOplus This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 788781-IAXOplus info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2015-65745-P info:eu-repo/grantAgreement/ES/MINECO/FPA2013-41085-P info:eu-repo/grantAgreement/ES/MINECO/FPA2016-76978-C3-1-P info:eu-repo/grantAgreement/ES/MINECO/RYC-2012-10597 info:eu-repo/semantics/openAccess by http://creativecommons.org/licenses/by/3.0/es/ 4.833 2019 1.664 2019 PHYSICS, PARTICLES & FIELDS 6 / 29 = 0.207 2019 Q1 T1 Physics and Astronomy (miscellaneous) 2019 Q1 ASTRONOMY & ASTROPHYSICS 16 / 68 = 0.235 2019 Q1 T1 info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion (orcid)0000-0003-3803-9384 O'Hare, C. A. J. Universidad de Zaragoza Lakic, B. (orcid)0000-0001-7529-9834 Galán, J. Universidad de Zaragoza (orcid)0000-0001-6327-9369 Iguaz, F. J. (orcid)0000-0003-1163-1687 Irastorza, I. G. Universidad de Zaragoza Jakovcic, K. (orcid)0000-0002-5352-1884 Luzón, G. Universidad de Zaragoza (orcid)0000-0002-1044-8197 Redondo, J. Universidad de Zaragoza (orcid)0000-0002-2417-7121 Ruiz Chóliz, E. Universidad de Zaragoza 2004 405 Universidad de Zaragoza Dpto. Física Teórica Área Física Teórica 2004 390 Universidad de Zaragoza Dpto. Física Teórica Área Física Atóm.Molec.y Nucl. 99, 3 (2019), 035037 [13 pp.] Phys. rev. D Physical Review D 2470-0010 1612197 http://zaguan.unizar.es/record/79127/files/texto_completo.pdf Versión publicada 111640 http://zaguan.unizar.es/record/79127/files/texto_completo.jpg?subformat=icon icon Versión publicada oai:zaguan.unizar.es:79127 articulos driver 2020-07-16-08:44:24 ARTICLE