Search for Solar Axions Produced in the p+d→3He+Ap + d \rightarrow\rm{^3He}+ A Reaction

preprint2010arXivOpen access

Abstract

A search for the axioelectric absorption of 5.5-MeV solar axions produced in the p+d→3He+γ(5.5MeV)p+d\rightarrow \rm{^3He}+γ(5.5 \rm{MeV}) reaction was performed with two BGO detectors placed inside a low-background setup. A model independent limit on axion-photon and axion-nucleon couplings was obtained: ∣gAe×gAN∣≤3.2×10−9(mA=0)|g_{Ae}\times g_{AN}| \leq 3.2\times 10^{-9} (m_A=0). Constraints on the axion-electron coupling constant were obtained for axions with masses in the (0.1−1.0)(0.1-1.0) MeV range: gAe≤(1.8−9.0)×10−7g_{Ae}\leq (1.8-9.0)\times 10^{-7}. The solar positron flux from A→e−+e+A\rightarrow e^-+e^+ decay was determined for axions with masses mA>2mem_A > 2m_e. Using the existing experimental data on the interplanetary positron flux, a new constraint on the axion-electron coupling constant for axions with masses in the (1.2−5.4)(1.2-5.4) MeV range was obtained: gAe≤(1−5)×10−17g_{Ae} \leq (1-5)\times 10^{-17}.

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