Physics potential of the International Axion Observatory (IAXO)
- Armengaud, E.
- Attie, D.
- Cogollos, C.
- Conlon, J. P.
- Costa, D.
- Dafni, T.
- Daido, R.
- Derbin, A. V.
- Descalle, M. A.
- Desch, K.
- Dratchnev, I. S.
- Döbrich, B.
- Basso, S.
- Dudarev, A.
- Ferrer-Ribas, E.
- Fleck, I.
- Galán, J.
- Galanti, G.
- Garrido, L.
- Gascon, D.
- Gastaldo, L.
- Germani, C.
- Ghisellini, G.
- Brun, P.
- Giannotti, M.
- Giomataris, I.
- Gninenko, S.
- Golubev, N.
- Graciani, R.
- Irastorza, I. G.
- Jakovčí c, K.
- Kaminski, J.
- Krčmar, M.
- Krieger, C.
- Bykovskiy, N.
- Lakić, B.
- Lasserre, T.
- Laurent, P.
- Limousin, O.
- Lindner, A.
- Lomskaya, I.
- Lubsandorzhiev, B.
- Luzón, G.
- Marsh, M. C. D.
- Mergalejo, C.
- Carmona, J. M.
- Mescia, F.
- Meyer, M.
- Miralda-Escudé, J.
- Mirallas, H.
- Muratova, V. N.
- Navick, X. F.
- Nones, C.
- Notari, A.
- Nozik, A.
- Ortiz de Solórzano, A.
- Castel, J. F.
- Pantuev, V.
- Papaevangelou, T.
- Pareschi, G.
- Perez, K.
- Picatoste, E.
- Pivovaroff, M. J.
- Redondo, J.
- Ringwald, A.
- Roncadelli, M.
- Ruiz-Chóliz, E.
- Cebrián, S.
- Ruz, J.
- Saikawa, K.
- Salvadó, J.
- Samperiz, M. P.
- Schiffer, T.
- Schmidt, S.
- Schneekloth, U.
- Schott, M.
- Silva, H.
- Tagliaferri, G.
- Cicoli, M.
- Takahashi, F.
- Tavecchio, F.
- ten Kate, H.
- Tkachev, I.
- Troitsky, S.
- Unzhakov, E.
- Vedrine, P.
- Vogel, J. K.
- Weinsheimer, C.
- Weltman, A.
- Civitani, M.
- Yin., W.
- IAXO Collaboration
DOIAbstract
We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as $g_{a\gamma}\sim 10^{-12}$ GeV$^{-1}$, or to electrons $g_{ae}\sim$10$^{-13}$, IAXO has the potential to find the QCD axion in the 1 meV$\sim$1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. At the same time, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous 'transparency' of the Universe to gamma-rays, 2) the ob...
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