New limit on the mass of 14.4-keV solar axions emitted in an M1 transition in Fe-57 nuclei - INSPIRE

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New limit on the mass of 14.4-keV solar axions emitted in an M1 transition in Fe-57 nuclei

A.V. Derbin
(
- St. Petersburg, INP
)
,
V.N. Muratova
(
- St. Petersburg, INP
)
,
D.A. Semenov
(
- St. Petersburg, INP
)
,
E.V. Unzhakov
(
- St. Petersburg, INP
)

2011

7 pages

Published in:

Phys.Atom.Nucl. 74 (2011) 596-602,
Yad.Fiz. 74 (2011) 620-626

DOI:

10.1134/S1063778811040041

{{\mathit A}^{0}}

(Axion) Limits from Nucleon Coupling

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Abstract: (Springer)

Axions of energy 14.4 keV that originated from the M1 transition in (57)Fe nuclei in the Sun were sought by using the resonance-absorption reaction A+(57)Fe -> (57)Fe* -> (57)Fe+ l (14.4 keV). Asectioned Si(Li) detector arranged in a low-backgr ound facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, |-'1.19g ( )AN( ) (0) + g ( )AN( ) (3) | 3.0Oe10(-'6). Within the hadronic-axion model, the respective constraint on t he axion mass is m (A) 145 eV (at a 95% C.L.).

axion: mass: upper limit
coupling: (nucleon axion)
axion: energy
axion: solar
axion: absorption
iron: excited nucleus
transition: magnetic
photon: energy spectrum
experimental results
semiconductor detector

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