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 Online-Ressource | |
| Verfasst von: | Armengaud, Eric [VerfasserIn]  |
| Gastaldo, Loredana [VerfasserIn] | |
| Titel: | Physics potential of the International Axion Observatory (IAXO) |
| Verf.angabe: | E. Armengaud, D. Attie, S. Basso, P. Brun, N. Bykovskiy, J.M. Carmona, J.F. Castel, S. Cebrián, M. Cicoli, M. Civitani, C. Cogollos, J.P. Conlon, D. Costa, T. Dafni, R. Daido, A.V. Derbin, M.A. Descalle, K. Desch, I.S. Dratchnev, B. Döbrich, A. Dudarev, E. Ferrer-Ribas, I. Fleck, J. Galán, G. Galanti, L. Garrido, D. Gascon, L. Gastaldo, C. Germani, G. Ghisellini, M. Giannotti, I. Giomataris, S. Gninenko, N. Golubev, R. Graciani, I.G. Irastorza, K. Jakovcic, J. Kaminski, M. Krcmar, C. Krieger, B. Lakić, T. Lasserre, P. Laurent, O. Limousin, A. Lindner, I. Lomskaya, B. Lubsandorzhiev, G. Luzón, M.C.D. Marsh, C. Mergalejo, F. Mescia, M. Meyer, J. Miralda-Escudé, H. Mirallas, V.N. Muratova, X.F. Navick, C. Nones, A. Notari, A. Nozik, A. Ortiz de Solórzano, V. Pantuev, T. Papaevangelou, G. Pareschi, K. Perez, E. Picatoste, M.J. Pivovaroff, J. Redondo, A. Ringwald, M. Roncadelli, E. Ruiz-Chóliz, J. Ruz, K. Saikawa, J. Salvadó, M.P. Samperiz, T. Schiffer, S. Schmidt, U. Schneekloth, M. Schott, H. Silva, G. Tagliaferri, F. Takahashi, F. Tavecchio, H. ten Kate, I. Tkachev, S. Troitsky, E. Unzhakov, P. Vedrine, J.K. Vogel, C. Weinsheimer, A. Weltman, W. Yin |
| E-Jahr: | 2019 |
| Jahr: | 24 June 2019 |
| Umfang: | 82 S. |
| Fussnoten: | Gesehen am 16.08.2019 |
| Titel Quelle: | Enthalten in: Journal of cosmology and astroparticle physics |
| Ort Quelle: | London : IOP, 2003 |
| Jahr Quelle: | 2019 |
| Band/Heft Quelle: | (2019), 6, Artikel-ID 047, Seite 1-82 |
| ISSN Quelle: | 1475-7516 |
| Abstract: | 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 observed soft X-ray excess from galaxy clusters or 3) some inflationary models. In addition, 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. |
| DOI: | doi:10.1088/1475-7516/2019/06/047 |
| URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt. Volltext ; Verlag: https://doi.org/10.1088/1475-7516/2019/06/047 |
| Volltext: http://arxiv.org/abs/1904.09155 | |
| DOI: https://doi.org/10.1088/1475-7516/2019/06/047 | |
| Datenträger: | Online-Ressource |
| Sprache: | eng |
| Sach-SW: | High Energy Physics - Experiment |
| High Energy Physics - Phenomenology | |
| K10plus-PPN: | 1671537009 |
| Verknüpfungen: | → Zeitschrift |
