Theoretical expectations and experimental prospects for solar axions searches with crystal detectors
S. Scopel, I. G. Irastorza, S. Cebrian, E. Garcia, D. Gonzalez, A. Morales, J. Morales, A. Ortiz de Solorzano, J. Puimedon, A. Salinas, M. L. Sarsa, J. A. Villar
Abstract
A calculation of the expected signal due to Primakov coherent conversion of solar axions into photons via Bragg scattering in several solid--state detectors is presented and compared with present and future experimental sensitivities. The axion window ma>~0.03 eV (not accessible at present by other techniques) could be explored in the foreseeable future with crystal detectors to constrain the axion--photon coupling constant below the latest bounds coming from helioseismology. On the contrary a positive signal in the sensitivity region of such devices would imply revisiting other more stringent astrophysical limits derived for the same range of the axion mass.
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