An improved limit on the axion–photon coupling from the CAST experiment

By S. Andriamonje, S. Aune, D. Autiero, K. Barth, A. Belov, B. Beltrán, H. Bräuninger, J. Carmona, S. Cebrián, J. Collar and 51 more. 2007

376 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/73c645ca242d3b5b18af9af5dab5b1ae8f5f9033

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Citations in the corpus

Microwave Background Constraints on Mixing of Photons with Hidden Photons (2008, methodology): “from tests of the Coulomb 1/r2 law [36,37], magnetic ﬁelds of Jupiter and earth [38], photon-regeneration-experiments [39–44], arguments of the lifetime of the Sun and the CAST search of solar axions [7,45]. The solid black line indicates the best possible bound Eq. (32) that can be obtained from as”
Axions as dark matter particles (2009, background): “88 × 10 GeV, valid for ma < 10 eV [75], slightly more stringent than those derived from horizontal branch stars.”
Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles (2014, methodology): “ SN core after the bounce, thereby obtaining for the rst time a detailed evolution of the ALP production with time. An excellent t to the total production rate is provided by the following expression [32], also widely used in SN neutrino studies, dN_ a dE = C E E 0 e (+1)E=E 0 : (2.11) Here Cis a ”
The type IIB string axiverse and its low-energy phenomenology (2012, methodology): “ither the non-observation of an anomalous energy loss of Horizontal Branch (HB) stars due to axion emission [57] or (slightly stronger) from the non-observation of solar axions in the CAST experiment [58]: L ⊃ − 1 4 gaγaFµνF˜µν, with gaγ≡ α 2π Ciγ fai <10−10 GeV−1. (B.1) This translates into a bo”
New experimental approaches in the search for axion-like particles (2018, methodology): “A reference formula for helioscopes is [30,396,481]:”