The standard picture of dark matter is one of individual particles: annihilating with each other, bumping into nuclei or electrons in direct detection experiments, or being produced from particle collisions. This is a good description if the dark matter mass is larger than a few electron-volts (eV). But if the dark matter is much lighter, and is a boson rather than a fermion, quantum mechanics tells us that the dark matter particles lose their individual identities and start behaving collectively, as a field. In fact, there is so much dark matter that the quantum nature of this field is not apparent, and it can behave like a classical field. Photons do exactly the same thing: the light from your computer screen that allows you to read this text is best described by an electromagnetic field which satisfies Maxwell’s equations, rather than by individual photons. As a consequence, the intuition for experiments to look for coherent-field dark matter requires thinking about charges and currents, rather than individual scattering events.
The axion is a dark matter candidate which can satisfy all the required properties to behave as a coherent field. There are lots of reasons to expect ultralight axions, both experimental and theoretical. The observation that an electric dipole moment for the neutron has not yet been detected, despite the fact that it is easy to write down a term which would generate one, is known as the “strong CP problem.” An ultralight axion could solve this problem by essentially cancelling off this extra term. Highbrow theoretical arguments from string theory also suggest the existence of axions, maybe even hundreds or thousands of them, which arise from the extra dimensions required by string theory.
Generically, axions will interact very weakly with electromagnetism, which suggests a detection strategy: in a strong magnetic field, the axion field will source a very weak response magnetic field. Along with colleagues at MIT, I proposed a design for an experiment, “ABRACADABRA,” to detect axion dark matter, which exploits advances from totally different fields (MRI research in medical physics, and ultra-sensitive current measurement in metrology) to search for axions over a wide range of masses. The first results from this experiment were posted to the arXiv in December 2018, and our second-run analysis was completed in 2021. The ABRACADBRA collaboration is currently merging with the DM Radio collaboration to build a larger, more sensitive version of the experiment.
I have also proposed an experiment to look for axions which might not make up dark matter, by looking for photon-photon scattering (equivalently, nonlinearities in Maxwell’s equations) mediated by axions in superconducting cavities. This is simultaneously more general (one can look for axions of many masses simultaneously, rather than just the species which make up dark matter) and more limited (if we find a signal, it doesn’t necessarily tell us anything about dark matter) than the ABRACADABRA program, which makes it nicely complementary. This work is being pursued with SQMS at Fermilab, which makes the best superconducting cavities in the world.
Axion dark matter also leads to some pretty interesting astrophysical signals. Since the axion field can convert to electromagnetic radiation in the presence of strong magnetic fields, the best place to look for axion conversion is near the strongest magnetic fields in the universe: the region surrounding magnetars, neutron stars with absurdly large magnetic fields. So large, in fact, that everyday physics changes: hydrogen atoms are cylindrical rather than spherical, and photons of different polarizations travel at different speeds even in vacuum. My collaborators and I calculated the axion-photon conversion probability in the highly-magnetized plasma surrounding magnetars and other high-field neutron stars, and found that radio telescopes might be able to detect axion signals from a magnetar very close to the black hole at the center of the Milky Way. Recently, we analyzed the first batch of data: unfortunately, no axions yet, but we showed how more observation time could lead to the strongest limits yet on the axion-photon coupling.
- J. Foster, Y. Kahn, R. Nguyen, N. Rodd, B. Safdi. Dark Matter Interferometry. Phys. Rev. D103 (2021) 076018. arXiv:2009.14201.
- J. Foster, Y. Kahn et al. Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres. Phys. Rev. Lett. 125 (2020) 171301. arXiv:2004.00011.
- Z. Bogorad, A. Hook, Y. Kahn, and Y. Soreq. Probing ALPs and the Axiverse with Superconducting Radiofrequency Cavities. Phys. Rev. Lett. 123 (2019) 021801. arXiv:1902.01418.
- J. Ouellet et al. First Results from ABRACADABRA-10cm: A Search for Sub-Micro-eV Axion Dark Matter. Phys. Rev. Lett. 122 (2019) 121802. arXiv:1810.12257.
- Ars Technica: Pulsars could convert dark matter into something we could see.
- A. Hook, Y. Kahn, B. Safdi, and Z. Sun. Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres. Phys. Rev. Lett. 121 (2018) no.24, 241102. arXiv:1804.03145.
- Y. Kahn, B. Safdi, and J. Thaler. Broadband and Resonant Approach to Axion Dark Matter Detection. Phys. Rev. Lett. 117, 141801. arXiv:1602.01086.