The renormalization-group running of neutrino mixing is undetectable
hep-ph, astro-ph.HE
Submitted: 2026-10-20
Updated: 2026-10-20
Comments: 26 pages, 7 figures
License: http://creativecommons.org/licenses/by/4.0/
The gist: Quantum corrections make the parameters of a theory depend on an arbitrary renormalization scale, μ.
Abstract
Quantum corrections make the parameters of a theory depend on an arbitrary renormalization scale, μ. The renormalization-group (RG) running of neutrino masses and mixing is a standard tool to relate models defined at a high mass scale to measured values. A growing body of work holds that the running is also directly observable: a neutrino produced or detected at momentum transfer Q would carry the mixing matrix evaluated at μ= Q. Proposed signatures include flavor change at zero distance from the source, shifts in the measured CP-violation phase, and an anomalous flavor composition of high-energy astrophysical neutrinos. We show that this premise is incorrect. The mixing is a property of the neutrino itself, fixed by its self-energy on the mass shell, not by the process that produces or detects it. Setting μ= Q is legitimate, but then large logarithms in the self-energy undo the running; the premise incorrectly drops them. Hence, apart from small vertex and box corrections, every experiment measures the same mixing: the running is undetectable. We illustrate this in the Minimal Supersymmetric Standard Model, two seesaw models, and the Standard Model effective field theory. Independently, short-baseline data already limit the change of any one mixing angle between pion decay and detection at Q of a few GeV to below 0.7 -- 2.4.
Related papers
- Classification of g-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
- New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating
- Probing Memory-Burdened Primordial Black Holes with High-Energy Neutrinos
- From Axion Detection to Dark Matter Astronomy