Published October 28, 2024 | Version v1
Journal article Open

Discovering neutrino tridents at the Large Hadron Collider

  • 1. University of California Santa Cruz
  • 2. National Centre for Nuclear Research
  • 3. University of Oxford
  • 4. Michigan State University
  • 5. University of Chicago

Description

Neutrino trident production of dilepton pairs is well recognized as a sensitive probe of both electroweak physics and physics beyond the Standard Model. Although a rare process, it could be significantly boosted by such new physics, and it also allows the electroweak theory to be tested in a new regime. We demonstrate that the forward neutrino physics program at the Large Hadron Collider offers a promising opportunity to measure for the first time, dimuon neutrino tridents with a statistical significance exceeding 5⁢𝜎, improving on the previous claims at the ∼3⁢𝜎 level by the CHARM-II and CCFR collaborations while accounting for additional backgrounds later identified by the NuTeV collaboration. We present predictions for various proposed experiments and outline a specific experimental strategy to identify the signal and mitigate backgrounds, based on "reverse tracking" dimuon pairs in the FASER⁢𝜈⁢2 detector. We also discuss prospects for constraining beyond Standard Model contributions to neutrino trident rates at high energies.

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PhysRevD.110.072018.pdf

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Additional details

Identifiers

DOI
10.1103/PhysRevD.110.072018
Other
oai:uchicago.tind.io:13826

Funding

National Science Centre, Poland
2021/42/E/ST2/00031
National Science Foundation
PHY-2111427
National Science Foundation
PHY-2210283
Heising-Simons Foundation
2020-1840
European Union
AstroCeNT: Particle Astrophysics Science and Technology Centre
European Union
Horizon 2020 research and innovation program
National Science Foundation
PHY-2013791
National Science Foundation
PHY-2310497
U.S. Department of Energy
DE-SC0010107
U.S. Department of Energy
DE-AC02-07CH11359

UChicago Information

Division(s)
Institutes & Centers
Center(s) or Institute(s)
Kavli Institute for Cosmological Physics