A search for bremsstrahlung solar axions using the Majorana low-background BEGe detector at Kimballton (MALBEK)
N. Abgrall, E. Aguayo, F.T. Avignone III, A.S. Barabash, F.E., Bertrand, M. Boswell, V. Brudanin, M. Busch, A.S. Caldwell, Y-D. Chan, C.D., Christofferson, D.C. Combs, R.J. Cooper, R.J. Creswick, J.A. Detwiler, P.J., Doe, Yu. Efremenko, V. Egorov, S.R. Elliott, J.E. Fast

TL;DR
This study uses a specialized germanium detector to search for solar axions produced via bremsstrahlung, setting new limits on axion-electron coupling and exploring detection prospects through annual modulation signals.
Contribution
It provides the first experimental upper bound on DFSZ axion-electron coupling using low-background germanium detectors and discusses future sensitivity improvements.
Findings
Upper bound of $1.36\times 10^{-11}$ on axion-electron coupling
Detection prospects via seasonal modulation signals
Potential for improved sensitivity with future detectors
Abstract
A low-background, high-purity germanium detector has been used to search for evidence of low-energy, bremsstrahlung-generated solar axions. An upper bound of is placed on the direct coupling of DFSZ model axions to electrons. The prospects for the sensitivity of the Majorana Demonstrator array of point-contact germanium detectors to solar axions are discussed in the context of the model-independent annual modulation due to the seasonal variation of the earth-sun distance.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena · Cosmology and Gravitation Theories
