E-resources
-
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.
Journal of Cosmology and Astroparticle Physics, 06/2019, Volume: 2019, Issue: 6Journal Article
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 gaγ∼10−12 GeV−1, or to electrons gae∼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. 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.
Author
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Shelf entry
Permalink
- URL:
Impact factor
Access to the JCR database is permitted only to users from Slovenia. Your current IP address is not on the list of IP addresses with access permission, and authentication with the relevant AAI accout is required.
Year | Impact factor | Edition | Category | Classification | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Select the library membership card:
If the library membership card is not in the list,
add a new one.
DRS, in which the journal is indexed
Database name | Field | Year |
---|
Links to authors' personal bibliographies | Links to information on researchers in the SICRIS system |
---|
Source: Personal bibliographies
and: SICRIS
The material is available in full text. If you wish to order the material anyway, click the Continue button.