The precise measurement of neutrino properties is among the highest priorities in
fundamental particle physics, involving many experiments worldwide. Since the experiments …

Amplitudes derived from scattering data on elementary targets are basic inputs to neutrino-
nucleus cross section predictions. A prominent example is the isovector axial nucleon form …

A bstract We present a new analysis method that allows one to understand and model
excited state contributions in observables that are dominated by a pion pole. We apply this …

We report a calculation of the nucleon axial form factors GA q (Q 2) and GP q (Q 2) for all
three light quark flavors q∈{u, d, s} in the range 0≤ Q 2≲ 1.2 GeV 2 using lattice QCD. This …

The detectability of light dark matter in direct detection experiments is limited by the small
kinetic energy of the recoiling targets. Thus, scenarios where dark matter is boosted to …

We develop a model of relativistic, charged meson-exchange currents (MEC) for neutrino–
nucleus interactions. The two-body current is the sum of seagull, pion-in-flight, pion-pole and …

A bstract We discuss as accurately as possible the cross section of quasi-elastic scattering of
electron (anti-) neutrinos on nucleons, also known as inverse beta decay in the case of …

We present results for the isovector nucleon form factors measured on a 9 6 4 lattice at
almost the physical pion mass with a lattice spacing of 0.085 fm in 2+ 1 flavor QCD. The …

We report a lattice QCD determination of the π γ→ π π transition amplitude for the P-wave, I=
1 two-pion final state, as a function of the photon virtuality and π π invariant mass. The …

We study direct detection bounds on cosmic ray-upscattered dark matter in simplified
models including light mediators. We find that the energy dependence in the scattering cross …