Neutrino-nucleus cross sections for W-boson and trident production
arXiv:1910.08090 · doi:10.1103/PhysRevD.101.036011
Abstract
The physics of neutrino-nucleus cross sections is a critical probe of the Standard Model and beyond. A precise understanding is also needed to accurately deduce astrophysical neutrino spectra. At energies above GeV, the cross section is dominated by deep inelastic scattering, mediated by weak bosons. In addition, there are subdominant processes where the hadronic coupling is through virtual photons, : (on-shell) -boson production (e.g., where the underlying interaction is ) and trident production (e.g., where it is ). These processes become increasingly relevant at TeV--PeV energies. We undertake the first systematic approach to these processes (and those with hadronic couplings through virtual and bosons), treating them together, avoiding common approximations, considering all neutrino flavors and final states, and covering the energy range -- GeV. In particular, we present the first complete calculation of -boson production and the first calculation of trident production at TeV--PeV energies. When we use the same assumptions as in prior work, we recover all of their major results. In a companion paper, we show that these processes should be taken into account for IceCube-Gen2.
arXiv commentMain text 14 pages and 13 figures; minor changes; results and conclusions unchanged; matches published version
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