scholarly journals Impact of the inelastic proton–nucleus cross section on the prompt neutrino flux

2019 ◽  
Vol 79 (2) ◽  
Author(s):  
A. V. Giannini ◽  
V. P. Gonçalves
Keyword(s):  
Particles ◽  
2020 ◽  
Vol 3 (1) ◽  
pp. 164-168
Author(s):  
Mădălina Mihaela Miloi ◽  

For clarifying the validity of the Lepton Universality hypothesis, one of the fundamental statements of the Standard Model, the interaction cross section for all three flavors of leptons have to be known with high precision. In neutrino sector, for electron and muon neutrinos, the interaction cross section is known fairly well, but for tau neutrino only poor estimations exist. In particular, the most direct measurement by the DONuT experiment was performed with rather poor accuracy due to low statistics and an uncertainty of the tau neutrino flux. The DsTau experiment proposes to study tau-neutrino production process and thus to improve significantly the accuracy of calculations of tau neutrino flux for neutrino accelerator experiments. To study reactions providing most of tau neutrinos, the experiment uses a setup based on high resolution nuclear emulsions, capable to register short lived particle decays created in proton-nucleus interactions. The present report is an overview of the DsTau experiment together with some of the preliminary results from the pilot run.


2008 ◽  
Vol 77 (4) ◽  
Author(s):  
E. Borriello ◽  
A. Cuoco ◽  
G. Mangano ◽  
G. Miele ◽  
S. Pastor ◽  
...  

2021 ◽  
Vol 81 (6) ◽  
Author(s):  
Victor P. Gonçalves ◽  
Diego R. Gratieri ◽  
Alex S. C. Quadros

AbstractThe number of ultra-high energy neutrinos arriving at IceCube depends on the energy dependence of the astrophysical neutrino flux and neutrino cross-section. In this paper, we investigate the impact of different assumptions for the description of the QCD dynamics at high energies on the determination of the normalization $$\Phi _{Astro}$$ Φ Astro and spectral index $$\gamma $$ γ of the astrophysical neutrino flux. The distribution of neutrino events at the IceCube is estimated considering the DGLAP, BFKL, CGC and BBMT approaches and the best estimates for $$\Phi _{Astro}$$ Φ Astro and $$\gamma $$ γ are determined using a maximum likelihood fit comparing the predictions with the distribution of observed events at IceCube. Moreover, we also investigate if the increase in the effective exposure time expected in IceCube-Gen2 will to allow us to disentangle the QCD dynamical effects from the description of the astrophysical neutrino flux.


2020 ◽  
Vol 35 (13) ◽  
pp. 2050101
Author(s):  
I. Alikhanov

The Glashow resonance is a rapid enhancement of the cross-section for scattering of electron antineutrinos on electrons at the [Formula: see text] boson production threshold due to the [Formula: see text]-channel contribution. This resonance is being searched for at large volume neutrino detectors in which the reaction [Formula: see text] to be initiated by cosmic ray antineutrinos of energies about 6.3 PeV. The relatively small neutrino flux reaching the Earth together with the necessity of analyzing ultra-high-energy final states make such searches challenging. We argue here that the Glashow resonance may contribute to the process [Formula: see text]. By extending the method of the effective (equivalent) particles to the neutral leptons, we relate the distribution of the effective neutrinos in the electron to the total cross-section for [Formula: see text]. Our approach gives a good fit to the existing experimental data measured at the collider LEP at CERN and allows one to interpret these measurements as an observation of the Glashow resonance. We also discuss an advantage of future electron–positron colliders for probing the resonance.


2011 ◽  
Vol 26 (03n04) ◽  
pp. 754-756
Author(s):  
◽  
TOMASZ JAN PALCZEWSKI

This paper presents one of the physics goals of the NA61/SHINE experiment: measurements of hadron production needed for neutrino (T2K) and cosmic-ray (Pierre Auger and KASKADE) experiments. Preliminary results from the proton-Carbon interactions at 31 GeV/c for the T2K experiment at J-PARC are presented. Knowledge of pion and kaon production is important for improving the accuracy of neutrino flux simulations. Three different methods of the pion spectra extractions are presented. Finally, preliminary differential cross section dsigma/ dp in several intervals of emission angles of charged pion in p + C interactions at 31 GeV/c.


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