Search for solar axions using 57Fe

We have made a search for 57Fe gamma rays of energy 14.4 keV induced by resonant absorption of monochromatic solar axions, as proposed by Moriyama. The proposed axions are suggested to be emitted from the Sun, in M1 transitions between the first, thermally excited state and the ground state of 57Fe....

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Main Authors: Krčmar, M., Krečak, Z., Stipčević, M., Ljubičić, A., Bradley, David Andrew
Format: Article
Published: Elsevier 1998
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Online Access:http://eprints.um.edu.my/25674/
https://doi.org/10.1016/S0370-2693(98)01231-3
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spelling my.um.eprints.256742020-12-18T04:11:48Z http://eprints.um.edu.my/25674/ Search for solar axions using 57Fe Krčmar, M. Krečak, Z. Stipčević, M. Ljubičić, A. Bradley, David Andrew Q Science (General) QC Physics We have made a search for 57Fe gamma rays of energy 14.4 keV induced by resonant absorption of monochromatic solar axions, as proposed by Moriyama. The proposed axions are suggested to be emitted from the Sun, in M1 transitions between the first, thermally excited state and the ground state of 57Fe. An upper limit on hadronic axion mass of 745 eV is obtained at the 95% confidence level, it being assumed that z = 0.56 and S = 0.5. © 1998 Elsevier Science B.V. All rights reserved. Elsevier 1998 Article PeerReviewed Krčmar, M. and Krečak, Z. and Stipčević, M. and Ljubičić, A. and Bradley, David Andrew (1998) Search for solar axions using 57Fe. Physics Letters B, 442 (1-4). pp. 38-42. ISSN 0370-2693 https://doi.org/10.1016/S0370-2693(98)01231-3 doi:10.1016/S0370-2693(98)01231-3
institution Universiti Malaya
building UM Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Malaya
content_source UM Research Repository
url_provider http://eprints.um.edu.my/
topic Q Science (General)
QC Physics
spellingShingle Q Science (General)
QC Physics
Krčmar, M.
Krečak, Z.
Stipčević, M.
Ljubičić, A.
Bradley, David Andrew
Search for solar axions using 57Fe
description We have made a search for 57Fe gamma rays of energy 14.4 keV induced by resonant absorption of monochromatic solar axions, as proposed by Moriyama. The proposed axions are suggested to be emitted from the Sun, in M1 transitions between the first, thermally excited state and the ground state of 57Fe. An upper limit on hadronic axion mass of 745 eV is obtained at the 95% confidence level, it being assumed that z = 0.56 and S = 0.5. © 1998 Elsevier Science B.V. All rights reserved.
format Article
author Krčmar, M.
Krečak, Z.
Stipčević, M.
Ljubičić, A.
Bradley, David Andrew
author_facet Krčmar, M.
Krečak, Z.
Stipčević, M.
Ljubičić, A.
Bradley, David Andrew
author_sort Krčmar, M.
title Search for solar axions using 57Fe
title_short Search for solar axions using 57Fe
title_full Search for solar axions using 57Fe
title_fullStr Search for solar axions using 57Fe
title_full_unstemmed Search for solar axions using 57Fe
title_sort search for solar axions using 57fe
publisher Elsevier
publishDate 1998
url http://eprints.um.edu.my/25674/
https://doi.org/10.1016/S0370-2693(98)01231-3
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score 13.211869