CERN Axion Solar Telescope

A warehouse interior containing a long blue cylinder surrounded by scaffolding and plumbing.
CAST. The telescope magnet (blue) pivots about the right-hand side, while the yellow gantry on the left of the picture rolls along a circular track in the floor and raises and lowers the left-hand side to track the sun.

The CERN Axion Solar Telescope (CAST) is an experiment in astroparticle physics to search for axions originating from the Sun. The experiment, sited at CERN in Switzerland, came online in 2002 with the first data-taking run starting in May 2003. The successful detection of solar axions would constitute a major discovery in particle physics, and would also open up a brand new window on the astrophysics of the solar core.

If the axions exist, they may be produced in the Sun's core when X-rays scatter off electrons and protons in the presence of strong electric fields. The experimental setup is built around a 9.26 m long decommissioned test magnet for the LHC capable of producing a field of up to 9.5 T. This strong magnetic field is expected to convert solar axions back into X-rays for subsequent detection by X-ray detectors. The telescope observes the Sun for about 1.5 hours at sunrise and another 1.5 hours at sunset each day. The remaining 21 hours, with the instrument pointing away from the Sun, are spent measuring background axion levels.

CAST began operation in 2003 searching for axions up to 0.02 eV. In 2005, Helium-4 was added to the magnet, extending sensitivity to masses up to 0.39 eV, then Helium-3 was used during 2008–2011 for masses up to 1.15 eV. CAST then ran with vacuum again searching for axions below 0.02 eV.

As of 2014, CAST has not turned up definitive evidence for solar axions. It has considerably narrowed down the range of parameters where these elusive particles may exist. CAST has set significant limits on axion coupling to electrons[1] and photons.[2]

References

  1. ↑ Barth, K.; Belov, A.; Beltran, B.; Bräuninger, H.; Carmona, J.M.; Collar, J.I.; Dafni, T.; Davenport, M.; Di Lella, L.; Eleftheriadis, C.; Englhauser, J.; Fanourakis, G.; Ferrer-Ribas, E.; Fischer, H.; Franz, J.; Friedrich, P.; Galán, J.; García, J.A.; Geralis, T.; Giomataris, I.; Gninenko, S.; Gómez, H.; Hasinoff, M.D.; Heinsius, F.H.; Hoffmann, D.H.H.; Irastorza, I.G.; Jacoby, J.; Jakovčić, K.; Kang, D.; Königsmann, K.; Kotthaus, R.; Kousouris, K.; Krčmar, M.; Kuster, M.; Lakić, B.; Liolios, A.; Ljubičić, A.; Lutz, G.; Luzón, G.; Miller, D.W.; Papaevangelou, T.; Pivovaroff, M.J.; Raffelt, G.; Redondo, J.; Riege, H.; Rodríguez, A.; Ruz, J.; Savvidis, I.; Semertzidis, Y.; Stewart, L.; Van Bibber, K.; Vieira, J.D.; Villar, J.A.; Vogel, J.K.; Walckiers, L.; Zioutas, K. (9 May 2013). "CAST constraints on the axion-electron coupling". Journal of Cosmology and Astroparticle Physics. 2013 (05): 010–010. arXiv:1302.6283Freely accessible. Bibcode:2013JCAP...05..010B. doi:10.1088/1475-7516/2013/05/010.
  2. ↑ Arik, M.; Aune, S.; Barth, K.; Belov, A.; Borghi, S.; Bräuninger, H.; Cantatore, G.; Carmona, J.M.; Cetin, S.A.; Collar, J.I.; Dafni, T.; Davenport, M.; Eleftheriadis, C.; Elias, N.; Ezer, C.; Fanourakis, G.; Ferrer-Ribas, E.; Friedrich, P.; Galán, J.; García, J.A.; Gardikiotis, A.; Gazis, E.N.; Geralis, T.; Giomataris, I.; Gninenko, S.; Gómez, H.; Gruber, E.; Guthörl, T.; Hartmann, R.; Haug, F.; Hasinoff, M.D.; Hoffmann, D.H.H.; Iguaz, F.J.; Irastorza, I.G.; Jacoby, J.; Jakovčić, K.; Karuza, M.; Königsmann, K.; Kotthaus, R.; Krčmar, M.; Kuster, M.; Lakić, B.; Laurent, J.M.; Liolios, A.; Ljubičić, A.; Lozza, V.; Lutz, G.; Luzón, G.; Morales, J.; Niinikoski, T.; Nordt, A.; Papaevangelou, T.; Pivovaroff, M.J.; Raffelt, G.; Rashba, T.; Riege, H.; Rodríguez, A.; Rosu, M.; Ruz, J.; Savvidis, I.; Silva, P.S.; Solanki, S.K.; Stewart, L.; Tomás, A.; Tsagri, M.; van Bibber, K.; Vafeiadis, T.; Villar, J.A.; Vogel, J.K.; Yildiz, S.C.; Zioutas, K. (23 December 2011). "Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope with 3He Buffer Gas" (PDF). Physical Review Letters. 107 (26): 261302–1–261302–4. arXiv:1106.3919Freely accessible. Bibcode:2011PhRvL.107z1302A. doi:10.1103/PhysRevLett.107.261302.

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