Generator of neutrino-nucleon interactions for the FLUKA based simulation code (original) (raw)

Simulations from a new neutrino event generator

Nuclear Physics B - Proceedings Supplements, 2006

We construct a new Monte Carlo generator of events for neutrino interactions. The dynamical models for quasielastic reactions, ∆ excitation and more inelastic events described by the DIS formalism with the PDFs modified according to recent JLab data are used. We describe in detail single pion production channels, which combine the ∆ excitation and DIS contribution. Many comparisons of the outcome of simulations with experimental data are presented.

PRELIMINARY RESULTS OF NEUTRINO INTERACTIONS STUDY USING GENIE EVENT GENERATOR *

With the advent of intense accelerator-based sources of neutrinos and the demand of neutrino oscillation experiments to more precisely determine signal and background rates in their detectors has precipitated a resurged interest for neutrino interactions in the few-GeV energy range. Such measurements have not been updated for decades, having first been measured in bubble and spark chamber experiments. New measurements are sorely needed and yield important constraints for present and future neutrino oscillation experiments operating in this energy range. In the present contribution, we studied neutrino interactions in the few-GeV energy range. We used GENIE, a new neutrino Monte Carlo generator, to generate events and compute the cross sections for neutrino-nucleus interactions. Events are generated for particular user-defined situation: neutrinos scattered off a fix nuclear target (40 Ar nucleus). We present the obtained results, after we analyzed the event samples, on relevant dist...

Nuclear Models in FLUKA: Present Capabilities, Open Problems and Future Improvements

2004

The nuclear reaction models embedded in the FLUKA code cover hadron, ion, photon and neutrino induced nuclear interactions from energies as low as few tens of MeV up to several tens of TeV. A short description of the main physics ingredients in the FLUKA nuclear models is given, with emphasis on the intermediate energy range and on "exotic" reactions. The treatment of electromagnetic dissociation as recently implemented in FLUKA is described. Examples of performances are presented for illustrative situations covering some of the most typical FLUKA applications.

Simulation of nuclear effects in quasi elastic and resonant neutrino interactions

1998

The effects of nuclear re-interactions in quasi elastic and resonant neutrino interactions have been considered in the framework of the nuclear models of the DPMJET code. A preliminary investigation on the modifications induced on the final state has been performed. Some consequences affecting the experimental identification are discussed.

Numerical implementation of lepton-nucleus interactions and its effect on neutrino oscillation analysis

We discuss the implementation of the nuclear model based on realistic nuclear spectral functions in the GENIE neutrino interaction generator. Besides improving on the Fermi gas description of the nuclear ground state, our scheme involves a new prescription for Q 2 selection, meant to efficiently enforce energy momentum conservation. The results of our simulations, validated through comparison to electron scattering data, have been obtained for a variety of target nuclei, ranging from carbon to argon, and cover the kinematical region in which quasi elastic scattering is the dominant reaction mechanism. We also analyse the influence of the adopted nuclear model on the determination of neutrino oscillation parameters.

Neutrino Interactions Importance to Nuclear Physics

AIP Conference Proceedings, 2009

We review the general interplay between Nuclear Physics and neutrino-nucleus cross sections at intermediate and high energies. The effects of different reaction mechanisms over the neutrino observables are illustrated with examples in calculations using several nuclear models and ingredients.

A hadronization model for few-GeV neutrino interactions

The European Physical Journal C, 2009

We present a detailed description of a new hadronic multiparticle production model for use in neutrino interaction simulations. Its validity spans a wide invariant mass range starting from pion production threshold. This model focuses on the low invariant mass region which is probed in few-GeV neutrino interactions and is of particular importance to neutrino oscillation experiments using accelerator and atmospheric fluxes. It exhibits reasonable agreement with a wide variety of experimental data. We also describe measurements that can be made in upcoming experiments that can improve modeling in areas where uncertainties are currently large.

GENEVE: a Montecarlo generator for neutrino interactions in the intermediate energy range

Nuclear Physics B - Proceedings Supplements, 2002

GENEVE is a MonteCarlo code developed during the last few years inside the ICARUS Collaboration. It describes neutrino interactions on nuclear target in the "intermediate energy range" and therefore is well suited for simulation of atmospheric neutrino scattering. We provide here few indications about the models adopted for the simulation of quasi-eiastic interactions and of scattering processes proceeding via nucleon resonances excitation and decay. The code has been tested with comparisons with available data and an overall agreement turns out to be achieved. A gradual upgrade of the code is indeed necessary, according to many indications, reviewed during this Workshop, from more recent theoretical developments and experimental hints. More in general, the definitive assessment of a canonical MonteCarlo code for neutrino physics (in the intermediate energy range) has been identified as one of the most urgent task for a fully comprehensive understanding of the neutrino oscillation phenomenon. We believe that the only way to proceed relies on the forthcoming results of present and future generations of experiments, performed with best suited, available technologies, aiming to precise neutrino cross section measurements.

Study of neutrino-nucleus reactions with CRISP Program (0<$E_\nu$<3 GeV)

2021

The neutrino-nucleus reactions are studied at energies from 0 to 3 GeV, using the CRISP program. To simulate these reactions, CRISP uses the Monte Carlo method through an intranuclear cascade model. Quase-elastic and baryonic resonance formation channels for the neutrino-nucleon interaction are considered. The total and differential particle emission cross sections were obtained, obtaining a good agreement with the values reported by the MiniBooNE experiment. The influence of nuclear effects on the studied reactions, such as fermionic motion, the Pauli blocking mechanism, and the nucleonic separation energy, was shown. It was not possible to simultaneously reproduce the νμ+D and νμ + 12 C reactions using the same axial mass value. For the charged current quasi-elastic channel, MA = 0.95 GeV for the νμ + D reaction, and MA = 1.35 GeV for the νμ + 12 C reaction. This can be solved if one considers, in addition to the neutrino-nucleon interaction, the neutrino interaction with a pair o...

Neutrino-nucleus interactions

2012

Interactions of neutrinos with nuclei in the energy ranges relevant for the MiniBooNE, T2K, NOνA, MINERνA and MINOS experiments are discussed. It is stressed that any theoretical treatment must involve all the relevant reaction mechanisms: quasielastic scattering, pion production and DIS. In addition, also many-body interactions play a role. In this talk we show how a misidentification of the reaction mechanism can affect the energy reconstruction. We also discuss how the newly measured pion production cross sections, as reported recently by the MiniBooNE collaboration, can be related to the old cross sections obtained on elementary targets. The MiniBooNE data seem to be compatible only with the old BNL data. Even then crucial features of the nucleon-pion-Delta interaction are missing in the experimental pion kinetic energy spectra. We also discuss the meson production processes at the higher energies of the NOνA, MINERνA and MINOS experiments. Here final state interactions make it impossible to gain knowledge about the elementary reaction amplitudes. Finally, we briefly explore the problems due to inaccuracies in the energy reconstruction that LBL experiments face in their extraction of oscillation parameters.