Theoretical expectations and experimental prospects for solar axions searches with crystal detectors

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dc.creatorScopel, S.
dc.creatorIrastorza, I. G.
dc.creatorCebrian, S.
dc.creatorGarcia, E.
dc.creatorGonzalez, D.
dc.creatorMorales, A.
dc.creatorMorales, J.
dc.creatorde Solorzano, A. Ortiz
dc.creatorPuimedon, J.
dc.creatorSalinas, A.
dc.creatorSarsa, M. L.
dc.creatorVillar, J. A.
dc.date1998-10-20
dc.date.accessioned2026-07-07T02:28:29Z
dc.date.available2026-07-07T02:28:29Z
dc.descriptionA 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 m_a>~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.
dc.description8 pages, 1 figure, To be published in the proceedings of the 2nd International Workshop on the Identification of Dark Matter (IDM98), Buxton, England, 7-11 September 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9810308
dc.identifierhttp://arxiv.org/abs/astro-ph/9810308
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13143
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTheoretical expectations and experimental prospects for solar axions searches with crystal detectors
dc.typetext

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