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Revisiting the detection rate for axion haloscopes
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abstract
The cavity haloscope has been employed to detect microwave photons resonantly converted from invisible cosmic axions under a strong magnetic field. In this scheme, the axion-photon conversion power has been formulated to be valid for certain conditions, either $Q_{cavity}\ll Q_{\rm axion}$ or $Q_{cavity} \gg Q_{axion}$. This remedy, however, fails when these two quantities are comparable to each other. Furthermore, the noise power flow has been treated independently of the impedance mismatch of the system, which could give rise to misleading estimates of the experimental sensitivity. We revisit the analytical approaches to derive a general description of the signal and noise power. We also optimize the coupling strength of a receiver to yield the maximal sensitivity for axion search experiments.
Forward citations
Cited by 3 Pith papers
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The VORTEX cavity for the RADES axion haloscope
A split-cylinder axion haloscope tunes continuously from 9 to 8.2 GHz with modest Q loss, operates at millikelvin temperatures, and its TM010 field profile passes bead-pull verification.
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Classical Analysis of Non-Coherent Dark Matter to Photon Conversion in a Resonant Cavity
Random-phase (non-coherent) axion or dark photon dark matter produces the same average resonant-cavity signal power as coherent dark matter, given by the standard formula with the quality factor replaced by min(Q_cavi...
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Experiments to test the hypothesis for solar and dark matter axions
This is a pedagogical review of haloscope and helioscope experiments searching for dark matter and solar axions, with an overview of near-future technological developments.
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