REVIEW 2 cited by
New $\mu$ Forces From $\nu_\mu$ Sources
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
abstract
Accelerator-based experiments reliant on charged pion and kaon decays to produce muon-neutrino beams also deliver an associated powerful flux of muons. Therefore, these experiments can additionally be sensitive to light new particles that preferentially couple to muons and decay to visible final states on macroscopic length scales. Such particles are produced through rare 3-body meson decays in the decay pipe or via muon scattering in the beam dump, and decay in a downstream detector. To demonstrate the potential of this search strategy, we recast existing MiniBooNE and MicroBooNE studies of neutral pion production in neutrino-induced neutral-current scattering ($\nu_\mu N \to \nu_\mu N \pi^0,~\pi^0\rightarrow \gamma\gamma$) to place new leading limits on light ($< 2m_\mu$) muon-philic scalar particles that decay to diphotons through loops of virtual muons. Our results exclude scalars of mass between 10 and 60 MeV in which this scenario resolves the muon $g-2$ anomaly. We also make projections for the sensitivity of SBND to these models and provide a road map for future neutrino experiments to perform dedicated searches for muon-philic forces.
Forward citations
Cited by 2 Pith papers
-
The LHC as a TeV Muon Beam Dump: Muonphilic Scalars at FASER
FASER and FASER2 could probe unconstrained muonphilic scalar masses below the dimuon threshold, including the (g-2)_mu favored region, using diphoton and muon-plus-diphoton signals.
-
Constraining self-interacting ultrahigh-energy muon neutrinos by cosmic microwave background spectral distortion
Scalar-mediated scattering of PeV muon neutrinos on the cosmic neutrino background injects photon energy that distorts the CMB, giving coupling bounds g_nu_mu of about 10^-4 to 10^-5 with projected PIXIE sensitivities...
Discussion (0). Continue with ORCID to comment.