Earth-Catalyzed Detection of Magnetic Inelastic Dark Matter with Photons in Large Underground Detectors

Abstract

Inelastic dark matter with moderate splittings, $\mathcal{O}(\mathrm{few}\mathrm{to}150)$ keV, can upscatter to an excited state in the Earth, with the excited state subsequently decaying, leaving a distinctive monoenergetic photon signal in large underground detectors. The photon signal can exhibit sidereal-daily modulation, providing excellent separation from backgrounds. Using a detailed numerical simulation, we examine this process as a search strategy for magnetic inelastic dark matter with the dark matter mass near the weak scale, where the upscatter to the excited state and decay proceed through the same magnetic dipole transition operator. At lower inelastic splittings, the scattering is dominated by moderate mass elements in the Earth with high spin, especially ${}^{27}$Al, while at larger splittings, ${}^{56}$Fe becomes the dominant target. We show that the proposed large volume gaseous detector CYGNUS will have excellent sensitivity to this signal. Xenon detectors also provide excellent sensitivity through the inelastic nuclear recoil signal, and if a future signal is seen, we show that the synergy among both types of detection can provide strong evidence for magnetic inelastic dark matter. In the course we have calculated nuclear response functions for elements relevant for scattering in the Earth, which are publicly available on GitHub.

38 pages, 8 figures, 2 appendices. Ancillary data available at https://github.com/joshaeby/IsotopeResponses. v2: Version accepted by JHEP, minor changes, typo fixed in modulation rate calculation resulting in slightly altering the reach at SUPL (little change to Gran Sasso results)

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