New limit on the mass of 14.4-keV solar axions emitted in an M1 Transition in [sup.57]Fe nuclei
Axions of energy 14.4 keV that originated from the Ml transition in [sup.57]Fe nuclei in the Sun were sought by using the resonance-absorption reaction A + [sup.57]Fe → [sup.57]Fe * → [sup.57]Fe + γ (14.4 keV). A sectioned Si(Li) detector arranged in a low-background facility was used to record phot...
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| Veröffentlicht in: | Physics of atomic nuclei 2011-04, Vol.74 (4), p.596 |
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| creator | Derbin, A.V Muratova, V.N Semenov, D.A Unzhakov, E.V |
| description | Axions of energy 14.4 keV that originated from the Ml transition in [sup.57]Fe nuclei in the Sun were sought by using the resonance-absorption reaction A + [sup.57]Fe → [sup.57]Fe * → [sup.57]Fe + γ (14.4 keV). A sectioned Si(Li) detector arranged in a low-background facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, [absolute value of -l.19[g.sup.0.sub.AN] + [g.sup.3.sub.AN]] ≤ 3.0 x [10.sup.-6]. Within the hadronic-axion model, the respective constraint on the axion mass is [m.sub.A] ≤ 145 eV (at a 95% C.L.). |
| doi_str_mv | 10.1134/S1063778811040041 |
| format | Article |
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A sectioned Si(Li) detector arranged in a low-background facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, [absolute value of -l.19[g.sup.0.sub.AN] + [g.sup.3.sub.AN]] ≤ 3.0 x [10.sup.-6]. 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A sectioned Si(Li) detector arranged in a low-background facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, [absolute value of -l.19[g.sup.0.sub.AN] + [g.sup.3.sub.AN]] ≤ 3.0 x [10.sup.-6]. 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A sectioned Si(Li) detector arranged in a low-background facility was used to record photons from this reaction. This resulted in setting a new limit on the axion couplings to nucleons, [absolute value of -l.19[g.sup.0.sub.AN] + [g.sup.3.sub.AN]] ≤ 3.0 x [10.sup.-6]. Within the hadronic-axion model, the respective constraint on the axion mass is [m.sub.A] ≤ 145 eV (at a 95% C.L.).</abstract><cop>United States</cop><pub>Springer</pub><doi>10.1134/S1063778811040041</doi><tpages>7</tpages></addata></record> |
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| ispartof | Physics of atomic nuclei, 2011-04, Vol.74 (4), p.596 |
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| subjects | AXIONS COUPLING EV RANGE IRON 57 KEV RANGE LI-DRIFTED SI DETECTORS M1-TRANSITIONS NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEONS PHOTONS RESONANCE ABSORPTION REST MASS SUN |
| title | New limit on the mass of 14.4-keV solar axions emitted in an M1 Transition in [sup.57]Fe nuclei |
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