Search for solar axions by Primakoff effect in NaI crystals

By R. Bernabei, P. Belli, R. Cerulli, F. Montecchia, F. Nozzoli, A. Incicchitti, D. Prosperi, C. Dai, H. L. He, H. Kuang and 2 more. 2001

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Towards a new generation axion helioscope (2011, background): “Crystal detectors may provide such fields [47–49], giving rise to characteristic Bragg patterns that have been searched for as byproducts of dark matter searches [50–53].”
Axions and the Strong CP Problem (2008, methodology): “, as well as the DAMA experiment [40, 42, Bernabei et al. (2001, 2003)] which utilized NaI crystals.”
New experimental approaches in the search for axion-like particles (2018, methodology): “The best result so far is that of DAMA, that sets gaγ 1.7 × 10−9GeV−1 (90% C.L.).”
Astrophysical axion bounds (2006, background): “Solar axions could also transform in electric crystal fields, but the limits obtained by SOLAX [43], COSME [44], and DAMA [45] are less restrictive and require a solar axion luminosity exceeding (15) and (16), i.”
An improved limit on the axion–photon coupling from the CAST experiment (2007, background): “[21], SOLAX [26], COSME [27], DAMA [28], Tokyo helioscope [22, 23] and HB stars [7, 52]) discussed in the introduction.”