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European Spallation Source as a searching tool for an ultralight scalar field

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arxiv 2207.11308 v2 pith:YWCVTX4P submitted 2022-07-22 hep-ph astro-ph.HEgr-qchep-ex

European Spallation Source as a searching tool for an ultralight scalar field

classification hep-ph astro-ph.HEgr-qchep-ex
keywords ulsfeuropeanfieldfutureinteractionneutrinoneutrinosphysics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Dark matter (DM) nature is one of the major issues in physics. The search for a DM candidate has motivated the known proposal of an ultralight scalar field (ULSF). We explore the possibility to search for this ULSF at the upcoming European Spallation Source neutrino Super-Beam experiment. We have considered the recent study case in which there could be an interaction between the ULSF and active neutrinos. We have found that in this future experimental setup, the sensitivity is competitive with other neutrino physics experiments. We show the expected future sensitivity for the main parameter modeling the interaction between ULSF and neutrinos.

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Cited by 2 Pith papers

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

  1. Ultralight dark matter in long-baseline accelerator neutrino oscillations

    hep-ph 2023-12 unverdicted novelty 5.0

    Systematic study of scalar and vector ULDM interactions on long-baseline neutrino oscillations finds order-of-magnitude weaker constraints for m_φ ≲ 10^{-17} eV due to stochastic effects, with combined T2K+NOvA data s...

  2. Searching non-standard interactions with atmospheric neutrinos at ESSnuSB

    hep-ex 2025-08 unverdicted novelty 4.0

    With 5.4 Mt·year atmospheric neutrino exposure, ESSnuSB could constrain |ε_eμ^m| < 0.053, |ε_eτ^m| < 0.057, |ε_μτ^m| < 0.021 and related diagonal differences at 90% CL, while NSI would alter mass ordering and θ23 octa...