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Simultaneous detection of boosted dark matter and neutrinos from the semi-annihilation at DUNE

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arxiv 2309.00395 v2 pith:O3R27GWA submitted 2023-09-01 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords matterdarkboosteddunedetectioncrossdependentexperiments
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Dark matter direct detection experiments impose the strong bounds on thermal dark matter scenarios. The bound can naturally be evaded if the cross section is momentum transfer or velocity dependent. One can test such thermal dark matter scenarios if dark matter particles are boosted by some mechanism. In this work, we consider a specific semi-annihilation $\chi\chi\to \nu\overline{\chi}$ where $\chi$ ($\overline{\chi}$) is dark matter (anti-dark matter), and search for simultaneous detection of the neutrino and the boosted dark matter in the final state at DUNE. We find that the energies of the neutrino and boosted dark matter are reconstructed by kinematics. In addition, we find that both signals can be testable at DUNE if the dark matter mass is below $8~\mathrm{GeV}$, and the scattering cross section is momentum transfer dependent. Even for larger dark matter masses, the two signals can be tested by combination of DUNE and the other experiments such as IceCube/DeepCore and Hyper-Kamiokande.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams

    hep-ph 2026-02 conditional novelty 6.0 of 10

    A new relativistic formalism computes capture and energy deposition of directed particle beams in compact stars, applied to blazar-boosted dark matter heating of white dwarfs and neutron stars.

  2. Dark matter spikes with strongly self-interacting particles

    hep-ph 2025-06 conditional novelty 5.0 of 10

    Number-changing dark matter self-interactions can significantly deplete dark matter spikes around supermassive black holes, while the 2 to 1 semi-annihilation generally preserves the spike structure.

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