International audienceIn order to measure neutrino oscillation parameters, long-baseline accelerator neutrino experiments are using MC simulations to determine initial neutrino flux. Uncertainties of the hadron production models limit the knowledge of the neutrino flux. Additional hadron production measurements are needed to reduce this uncertainty. The only experiment currently capable of providing such measurements is the NA61/SHINE experiment. I present recently published NA61/SHINE hadron production measurements for the T2K experiment which include spectra of hadrons $(π^{±}, K^{±}, p, K^0_s and Λ)$ in the proton-carbon interaction at 31 GeV/c and $π^{±}$ spectra exiting the surface of the T2K replica target
Les étapes nécessaires à une prédiction précise du flux de neutrinos de T2K pour la mesure de l'osci...
The T2K neutrino beam predictions require precise knowledge of the hadron production in proton-carbo...
From hypothetical particles in the 30s, neutrinos have turned into the first hint for new physics be...
In order to measure neutrino oscillation parameters, long-baseline accelerator neutrino experiments ...
The largest source of uncertainty on the initial neutrino flux in modern accelerator neutrino ex- pe...
New measurements of hadron production with a proton beam on a 2 cm carbon target at 31 GeV/c perform...
The neutrino programme of the NA61/ SHINE experiment at the CERN SPS is aiming to deliver precise ha...
AbstractNew measurements of hadron production with a proton beam on a 2 cm carbon target at 31 GeV/c...
New results from the NA61/SHINE experiment on the determination of charged hadron yields in proton-c...
A precise prediction of the neutrino flux is a key ingredient for achieving the physics goals of lon...
We report on measurements of hadron yields in proton-carbon interactions at 31 GeV/ c recorded by th...
An overview of the recent NA61/SHINE results on determination of charged hadron yields in proton-car...
T2K replica target hadron production measurements in NA61/SHINE and T2K neutrino flux predictions HA...
In this article the NA61/SHINE detector will be presented which is a large acceptance hadron spectro...
Les étapes nécessaires à une prédiction précise du flux de neutrinos de T2K pour la mesure de l'osci...
Les étapes nécessaires à une prédiction précise du flux de neutrinos de T2K pour la mesure de l'osci...
The T2K neutrino beam predictions require precise knowledge of the hadron production in proton-carbo...
From hypothetical particles in the 30s, neutrinos have turned into the first hint for new physics be...
In order to measure neutrino oscillation parameters, long-baseline accelerator neutrino experiments ...
The largest source of uncertainty on the initial neutrino flux in modern accelerator neutrino ex- pe...
New measurements of hadron production with a proton beam on a 2 cm carbon target at 31 GeV/c perform...
The neutrino programme of the NA61/ SHINE experiment at the CERN SPS is aiming to deliver precise ha...
AbstractNew measurements of hadron production with a proton beam on a 2 cm carbon target at 31 GeV/c...
New results from the NA61/SHINE experiment on the determination of charged hadron yields in proton-c...
A precise prediction of the neutrino flux is a key ingredient for achieving the physics goals of lon...
We report on measurements of hadron yields in proton-carbon interactions at 31 GeV/ c recorded by th...
An overview of the recent NA61/SHINE results on determination of charged hadron yields in proton-car...
T2K replica target hadron production measurements in NA61/SHINE and T2K neutrino flux predictions HA...
In this article the NA61/SHINE detector will be presented which is a large acceptance hadron spectro...
Les étapes nécessaires à une prédiction précise du flux de neutrinos de T2K pour la mesure de l'osci...
Les étapes nécessaires à une prédiction précise du flux de neutrinos de T2K pour la mesure de l'osci...
The T2K neutrino beam predictions require precise knowledge of the hadron production in proton-carbo...
From hypothetical particles in the 30s, neutrinos have turned into the first hint for new physics be...