QED Corrections to Neutrino Electron Scattering
arXiv:hep-ph/0011190 · doi:10.1103/PhysRevD.64.113002
Abstract
We evaluate the O(alpha) QED corrections to the recoil electron energy spectrum in the process nu_l + e --> nu_l + e (+gamma), where (+gamma) indicates the possible emission of a photon and l=e, mu or tau. The soft and hard bremsstrahlung differential cross sections are computed for an arbitrary value of the photon energy threshold. We also study the O(alpha) QED corrections to the differential cross section with respect to the total combined energy of the recoil electron and a possible accompanying photon. Their difference from the corrections to the electron spectrum is investigated. We discuss the relevance and applicability of both radiative corrections, emphasizing their role in the analysis of precise solar neutrino electron scattering experiments.
14 pages + 10 figures. Minimal changes, published version
References in corpus (1)
Cited by in corpus (24)
- Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
- Neutrino-Electron Scattering Theory
- s in neutrino scattering at DUNE
- The neutrino charge radius is a physical observable
- Radiative Corrections in Precision Electroweak Physics: a Historical Perspective
- Theory of elastic neutrino-electron scattering
- The Monte Carlo simulation of the Borexino detector
- What can we learn from neutrino electron scattering?
- On the effective theory of neutrino-electron and neutrino-quark interactions
- Neutrino energy loss rate in a stellar plasma
- Which solar neutrino experiment after KamLAND and Borexino?
- Constraints on Flavor-Diagonal Non-Standard Neutrino Interactions from Borexino Phase-II
- Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino
- Elastic Scattering of Neutrinos off Polarized Electrons
- Dynamical Zero in Antineutrino_e -- Electron Scattering and the Neutrino Magnetic Moment
- Radiative corrections to neutrino energy loss rate in stellar interiors
- Radiative tritium beta-decay and the neutrino mass
- Radiative (anti)neutrino energy spectra from muon, pion, and kaon decays
- Elastic Neutrino-electron Scattering at the One-loop Level in the Standard Model
- Sensitivity of accelerator-based neutrino experiments to neutrino-electron scattering radiative corrections
- QED Corrections to the Scattering of Solar Neutrinos and Electrons
- Essential Solar Neutrinos
- Radiative corrections to inverse muon decay for accelerator neutrinos
- Reducing Hadronic Uncertainty in Low-Energy Neutral-Current Processes