In the strong magnetic field of a neutron star’s magnetosphere, axions coupled to electromagnetism develop a nonzero probability to convert into photons. Past studies have revealed that the axion-photon conversion can be resonantly enhanced. We recognize that the axion-photon resonance admits two parametrically distinct resonant solutions, which we call the mass-matched resonance and the Euler-Heisenberg assisted resonance. The mass-matched resonance occurs at a point in the magnetosphere where the radially-varying plasma frequency crosses the axion mass . The Euler-Heisenberg assisted resonance occurs where the axion energy satisfies . This second resonance is made possible though the strong background magnetic field , as well as the nonzero Euler-Heisenberg four-photon self-interaction, which has the coupling . We study the resonant conversion of relativistic axion dark radiation into photons via the Euler-Heisenberg assisted resonance, and we calculate the expected electromagnetic radiation assuming different values for the axion-photon coupling and different amplitudes for the axion flux onto the neutron star . We briefly discuss several possible sources of axion dark radiation. Achieving a sufficiently strong axion flux to induce a detectable electromagnetic signal seems unlikely. Published by the American Physical Society2024 
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                    This content will become publicly available on April 1, 2026
                            
                            Dark Matter Axion Search with HAYSTAC Phase II
                        
                    
    
            This Letter reports new results from the HAYSTAC experiment’s search for dark matter axions in our galactic halo. It represents the widest search to date that utilizes squeezing to realize subquantum limited noise. The new results cover of newly scanned parameter space in the mass ranges and . No statistically significant evidence of an axion signal was observed, excluding couplings and at the 90% confidence level over the respective region. By combining this data with previously published results using HAYSTAC’s squeezed state receiver, a total of of parameter space has now been scanned between  , excluding at the 90% confidence level. These results demonstrate the squeezed state receiver’s ability to probe axion models over a significant mass range while achieving a scan rate enhancement relative to a quantum-limited experiment. Published by the American Physical Society2025 
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                            - PAR ID:
- 10596000
- Author(s) / Creator(s):
- ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »
- Publisher / Repository:
- American Institute of Physics, ArXiv.org
- Date Published:
- Journal Name:
- Physical Review Letters
- Volume:
- 134
- Issue:
- 15
- ISSN:
- 0031-9007
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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