AI Article Synopsis

  • Axions are theoretical particles that might explain dark matter and a specific physics problem (strong CP problem), and this study investigates their interactions using ^{129}Xe gas and Rb vapor.
  • The method used enhances the detection sensitivity for these axion interactions by 145 times compared to traditional approaches through magnetic amplification and effective field exploitation.
  • The research led to significant improvements in constraints on interactions related to axions, expanding the search for these particles and their potential links to dark matter, with implications for future investigations in this field.

Article Abstract

Axions are highly motivated hypothetical particles beyond the standard model that can be dark matter candidates and address the strong CP problem. Here we search for axion-mediated interactions generated between two separated ^{129}Xe gas ensembles, monitoring and polarizing the ^{129}Xe nuclear spins through spin-exchange interactions with Rb vapor. Our method exploits the magnetic amplification through effective fields from Rb-Xe collisions, increasing the sensitivity for axion-mediated interactions by up to 145-fold relative to conventional methods. Moreover, we employ template filtering to extract exotic interactions with a maximum signal-to-noise ratio. By combining two techniques, axion-mediated interactions are constrained to be less than 10^{-5} of normal magnetic interactions on a length scale of 60 mm. We establish new constraints on the neutron-neutron pseudoscalar couplings for a mass range that expands into the well-motivated "axion window" (10  μeV-1  meV), improving previous constraints by up to 50-fold within it and 118-fold outside it. We further discuss promising applications in searches for other axion-nucleon interactions, including axion dark matter and black hole axion bursts with sensitivity well beyond astrophysical limits by several orders of magnitude.

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Source
http://dx.doi.org/10.1103/PhysRevLett.133.191801DOI Listing

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