000112192 001__ 112192
000112192 005__ 20250113143110.0
000112192 0247_ $$2doi$$a10.1140/epjc/s10052-022-10061-1
000112192 0248_ $$2sideral$$a128097
000112192 037__ $$aART-2022-128097
000112192 041__ $$aeng
000112192 100__ $$aDi Luzio, L.
000112192 245__ $$aProbing the axion-nucleon coupling with the next generation of axion helioscopes
000112192 260__ $$c2022
000112192 5060_ $$aAccess copy available to the general public$$fUnrestricted
000112192 5203_ $$aA finite axion–nucleon coupling, nearly unavoidable for QCD axions, leads to the production of axions via the thermal excitation and subsequent de-excitation of 57Fe isotopes in the sun. We revise the solar bound on this flux adopting the up to date emission rate, and investigate the sensitivity of the proposed International Axion Observatory IAXO and its intermediate stage BabyIAXO to detect these axions. We compare different realistic experimental options and discuss the model dependence of the signal. Already BabyIAXO has sensitivity far beyond previous solar axion searches via the nucleon coupling and IAXO can improve on this by more than an order of magnitude.
000112192 536__ $$9info:eu-repo/grantAgreement/EC/H2020/788781/EU/Towards the detection of the axion with the International Axion Observatory/IAXOplus$$9This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 788781-IAXOplus$$9info:eu-repo/grantAgreement/EC/H2020/860881/EU/Revealing how hidden symmetries shape the universe/HIDDeN$$9This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 860881-HIDDeN$$9info:eu-repo/grantAgreement/ES/MINECO/PID2019-108122GB-C33
000112192 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000112192 590__ $$a4.4$$b2022
000112192 592__ $$a1.526$$b2022
000112192 591__ $$aPHYSICS, PARTICLES & FIELDS$$b8 / 29 = 0.276$$c2022$$dQ2$$eT1
000112192 593__ $$aPhysics and Astronomy (miscellaneous)$$c2022$$dQ1
000112192 593__ $$aEngineering (miscellaneous)$$c2022$$dQ1
000112192 594__ $$a8.3$$b2022
000112192 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000112192 700__ $$0(orcid)0000-0001-7529-9834$$aGalan, J.$$uUniversidad de Zaragoza
000112192 700__ $$0(orcid)0000-0001-9823-6262$$aGiannotti, M.
000112192 700__ $$0(orcid)0000-0003-1163-1687$$aGarcía Irastorza, I.$$uUniversidad de Zaragoza
000112192 700__ $$aJaeckel, J.
000112192 700__ $$aLindner, A.
000112192 700__ $$0(orcid)0000-0002-3253-7027$$aRuz, J.$$uUniversidad de Zaragoza
000112192 700__ $$aSchneekloth, U.
000112192 700__ $$aSohl, L.
000112192 700__ $$aThormaehlen, L. J.
000112192 700__ $$aVogel, J. K.
000112192 7102_ $$12004$$2390$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Atóm.Molec.y Nucl.
000112192 773__ $$g82, 2 (2022), 120 [15 pp.]$$pEur. phys. j., C$$tThe European Physical Journal C$$x1434-6044
000112192 8564_ $$s879641$$uhttps://zaguan.unizar.es/record/112192/files/texto_completo.pdf$$yVersión publicada
000112192 8564_ $$s2400586$$uhttps://zaguan.unizar.es/record/112192/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000112192 909CO $$ooai:zaguan.unizar.es:112192$$particulos$$pdriver
000112192 951__ $$a2025-01-13-14:30:24
000112192 980__ $$aARTICLE