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Search for Dark Matter Ionization on the Night Side of Jupiter with Cassini

Carlos Blanco1,2,* and Rebecca K. Leane3,4,†

  • *carlosblanco2718@princeton.edu
  • †rleane@slac.stanford.edu
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Phys. Rev. Lett. 132, 261002 – Published 27 June, 2024

DOI: https://doi.org/10.1103/PhysRevLett.132.261002

Abstract

We present a new search for dark matter (DM) using planetary atmospheres. We point out that annihilating DM in planets can produce ionizing radiation, which can lead to excess production of ionospheric H3+. We apply this search strategy to the night side of Jupiter near the equator. The night side has zero solar irradiation, and low latitudes are sufficiently far from ionizing auroras, leading to a low-background search. We use Cassini data on ionospheric H3+ emission collected three hours either side of Jovian midnight, during its flyby in 2000, and set novel constraints on the DM-nucleon scattering cross section down to about 10−38  cm2. We also highlight that DM atmospheric ionization may be detected in Jovian exoplanets using future high-precision measurements of planetary spectra.

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Phys. Rev. Lett. 132, 261002– Published 27 June, 2024
  • Received 22 December 2023
  • Revised 9 April 2024
  • Accepted 16 May 2024
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Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

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