Theoretical expectations and experimental prospects for solar axions searches with crystal detectors
Scopel, S. · Irastorza, I. G. · Cebrian, S. · Garcia, E. · Gonzalez, D. · Morales, A. · Morales, J. · de Solorzano, A. Ortiz · Puimedon, J. · Salinas, A. · Sarsa, M. L. · Villar, J. A.
Original · EN
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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