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Possible resonance effect of axionic dark matter in Josephson junctions
1Isaac Newton Institute for Mathematical Sciences, University of Cambridge, 20 Clarkson Road, Cambridge CB3 0EH, United Kingdom and School of Mathematical Sciences, Queen Mary University of London, Mile End Road, London E1 4NS, United Kingdom.
Theoretical arguments suggest dark-matter axions may create an observable signal in Josephson junctions. This signal, a Shapiro steplike feature, could confirm axion properties and galactic dark matter density.
Area of Science:
- Theoretical physics
- Astrophysics
- Condensed matter physics
Background:
- Axions are hypothetical elementary particles proposed as a dark matter candidate.
- Josephson junctions are sensitive superconducting devices exhibiting quantum mechanical phenomena.
Purpose of the Study:
- To propose a theoretical framework for detecting dark-matter axions using resonant S/N/S Josephson junctions.
- To interpret a previously observed resonance signal as evidence for axionic dark matter.
Main Methods:
- Developing theoretical arguments based on gauge-invariant axion Josephson phase angles.
- Analyzing the interaction process between galactic axions and Josephson junctions.
- Comparing theoretical predictions with experimental observations of resonance signals.
Main Results:
- Theoretical prediction of a Shapiro steplike feature in Josephson junctions due to axion interaction.
- Consistency of the theory with a previously observed resonance signal (Hoffmann et al., 2004).
- Estimation of axion mass (m(a)c²=0.11 meV) and galactic axionic dark matter density (0.05 GeV/cm³).
Conclusions:
- The observed resonance signal can be interpreted as a signature of dark-matter axions.
- Future experiments are needed to experimentally verify the dark-matter nature of this signal.
- This work provides a novel avenue for detecting axionic dark matter.
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