Physics potential of the International Axion Observatory (IAXO)

Armengaud, E.; Attié, D.; Basso, S.; Brun, P.; Bykovskiy, N.; Carmona, J. M.; Castel, J. F.; Cebrián, S.; Cicoli, M.; Civitani, M.; Cogollos, C.; Conlon, J. P.; Costa, D.; Dafni, T.; Daido, R.; Derbin, A. V.; Descalle, M. A.; Desch, K.; Dratchnev, I. S.; Döbrich, B.; Dudarev, A.; Ferrer-Ribas, E.; Fleck, I.; Galán, J.; Galanti, G.; Garrido, L.; Gascon, D.; Gastaldo, L.; Germani, C.; Ghisellini, G.; Giannotti, M.; Giomataris, I.; Gninenko, S.; Golubev, N.; Graciani, R.; Irastorza, I. G.; Jakovčić, K.; Kaminski, J.; Krčmar, M.; Krieger, C.; Lakić, B.; Lasserre, T.; Laurent, P.; Limousin, O.; Lindner, A.; Lomskaya, I.; Lubsandorzhiev, B.; Luzón, G.; Marsh, M. C.  D.; Margalejo, C.; Mescia, F.; Meyer, M.; Miralda-Escudé, J.; Mirallas, H.; Muratova, V. N.; Navick, X. F.; Nones, C.; Notari, A.; Nozik, A.; de Solórzano, A. Ortiz; Pantuev, V.; Papaevangelou, T.; Pareschi, G.; Perez, K.; Picatoste, E.; Pivovaroff, M. J.; Redondo, J.; Ringwald, A.; Roncadelli, M.; Ruiz-Chóliz, E.; Ruz, J.; Saikawa, K.; Salvadó, J.; Samperiz, M. P.; Schiffer, T.; Schmidt, S.; Schneekloth, U.; Schott, M.; Silva, H.; Tagliaferri, G.; Takahashi, F.; Tavecchio, F.; Kate, H. ten; Tkachev, I.; Troitsky, S.; Unzhakov, E.; Vedrine, P.; Vogel, J. K.; Weinsheimer, C.; Weltman, A.; Yin, W.

doi:10.1088/1475-7516/2019/06/047

Title: Physics potential of the International Axion Observatory (IAXO)

Journal Article · 24 June 2019 · Journal of Cosmology and Astroparticle Physics

DOI: https://doi.org/10.1088/1475-7516/2019/06/047 · OSTI ID:1547283

Armengaud, E.; Attié, D.; Basso, S.; Brun, P.; Bykovskiy, N.; Carmona, J. M.; Castel, J. F.; Cebrián, S.; Cicoli, M.; Civitani, M.; Cogollos, C.; Conlon, J. P.; Costa, D.; Dafni, T.; Daido, R.; Derbin, A. V.; Descalle, M. A.; Desch, K.; Dratchnev, I. S.; Döbrich, B. more »

We report on 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_aγ~ 10^–12 GeV^–1, or to electrons g_ae~10^–13, IAXO has the potential to find the QCD axion in the 1 meV~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. Similarly, 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 observed soft X-ray excess from galaxy clusters or 3) some inflationary models. Furthermore, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE; European Research Council (ERC)

Contributing Organization:: IAXO collaboration

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1547283

Journal Information:: Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 06; ISSN 1475-7516

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 137 works

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The Initial Mass–Final Luminosity Relation of Type II Supernova Progenitors: Hints of New Physics? Straniero, Oscar; Dominguez, Inma; Piersanti, Luciano The Astrophysical Journal, Vol. 881, Issue 2 https://doi.org/10.3847/1538-4357/ab3222	journal	August 2019
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