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dc.contributor.authorIrastorza, I.G.
dc.contributor.authorAvignone, F.T.
dc.contributor.authorCantatore, G.
dc.contributor.authorCaspi, S.
dc.contributor.authorCarmona, J.M.
dc.contributor.authorDafni, T.
dc.contributor.authorDavenport, M.
dc.contributor.authorDudarev, A.
dc.contributor.authorFanourakis, G.
dc.contributor.authorFerrer-Ribas, E.
dc.contributor.authorGalan, J.
dc.contributor.authorGarcia, J.A.
dc.contributor.authorGeralis, T.
dc.contributor.authorGiomataris, I.
dc.contributor.authorGninenko, S.
dc.contributor.authorGomez, H.
dc.contributor.authorHoffmann, D.H.H.
dc.contributor.authorIguaz, F.J.
dc.contributor.authorJakovcic, K.
dc.contributor.authorKrcmar, M.
dc.contributor.authorLakic, B.
dc.contributor.authorLuzon, G.
dc.contributor.authorLindner, A.
dc.contributor.authorPivovaroff, M.
dc.contributor.authorPapaevangelou, T.
dc.contributor.authorRaffelt, G.
dc.contributor.authorRedondo, J.
dc.contributor.authorRodriguez, A.
dc.contributor.authorRussenschuck, S.
dc.contributor.authorRuz, J.
dc.contributor.authorShilon, I.
dc.contributor.authorTen Kate, H.
dc.contributor.authorTomas, A.
dc.contributor.authorTroitsky, S.
dc.contributor.authorvan Bibber, K.
dc.contributor.authorVillar, J.A.
dc.contributor.authorVogel, J.
dc.contributor.authorWalckiers, L.
dc.contributor.authorZioutas, K.
dc.date.accessioned2015-04-15T01:16:49Z
dc.date.available2015-04-15T01:16:49Z
dc.date.issued2012-01
dc.identifier.urihttp://hdl.handle.net/10945/44949
dc.description.abstractThe International Axion Observatory (IAXO) is a new generation axion helioscope aiming at a sensitivity to the axion-photon coupling of ga & few × 10−12 GeV−1, i.e. 1–1.5 orders of magnitude beyond the one currently achieved by CAST. The project relies on improvements in magnetic field volume together with extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested in CAST. Additional physics cases of IAXO could include the detection of electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion- like particles (ALPs) and other novel excitations at the low-energy frontier of elementary particle physics. This contribution is a summary of our recent paper.en_US
dc.rightsThis publication is a work of the U.S. Government as defined in Title 17, United States Code, Section 101. Copyright protection is not available for this work in the United States.en_US
dc.titleThe International Axion Observatory (IAXO)en_US
dc.typeArticleen_US


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