Introducing DMRadio-GUT, a search for GUT-scale QCD axions
arXiv:2203.11246 · doi:10.1103/PhysRevD.106.112003
Abstract
The QCD axion is a leading dark matter candidate that emerges as part of the solution to the strong CP problem in the Standard Model. The coupling of the axion to photons is the most common experimental probe, but much parameter space remains unexplored. The coupling of the QCD axion to the Standard Model scales linearly with the axion mass; therefore, the highly-motivated region 0.4-120 neV, corresponding to a GUT-scale axion, is particularly difficult to reach. This paper presents the design requirements for a definitive search for GUT-scale axions and reviews the technological advances needed to enable this program.
16 pages, 4 figures
References in corpus (11)
- Amplification and squeezing of quantum noise with a tunable Josephson metamaterial
- Revisiting the bound on axion-photon coupling from Globular Clusters
- Back-action evasion and squeezing of a mechanical resonator using a cavity detector
- The LUX-ZEPLIN (LZ) Experiment
- The dark-matter axion mass
- An M Theory Solution to the Strong CP Problem and Constraints on the Axiverse
- The photo-philic QCD axion
- Projected Sensitivity of DMRadio-m: A Search for the QCD Axion Below eV
- Design and Implementation of the ABRACADABRA-10 cm Axion Dark Matter Search
- Highly-sensitive superconducting circuits at ~700 kHz with tunable quality factors for image-current detection of single trapped antiprotons
- Axion Dark Matter, Proton Decay and Unification
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