Search for resonant absorption of solar axions emitted in an M1 transition in 57Fe nuclei View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2007-03

AUTHORS

A. V. Derbin, A. I. Egorov, I. A. Mitropol’sky, V. N. Muratova, N. V. Bazlov, S. V. Bakhlanov, D. A. Semenov, E. V. Unzhakov

ABSTRACT

The resonant absorption of solar axions by 57Fe nuclei, which is accompanied by the excitation of the first excited nuclear level: A + 57Fe → 57Fe* → 57Fe + γ(14.4 keV), is sought. To seek 14.4-keV photons, a Si(Li) detector and an enriched 57Fe target are used. The detector and target are placed in a low-background setup equipped with passive and active shieldings. As a result, a new upper limit mA ≤ 360 eV (at 90% C.L.) has been determined for the axion mass. More... »

PAGES

12-16

References to SciGraph publications

  • 2005-10-14. Vus determination from hyperon semileptonic decays in JOURNAL OF HIGH ENERGY PHYSICS
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1134/s0021364007010031

    DOI

    http://dx.doi.org/10.1134/s0021364007010031

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