Neutrino Interaction Calculations from MeV to GeV Region

نویسنده

  • J. E. Amaro
چکیده

The Quasi-Elastic (QE) contribution of the nuclear inclusive electron model developed in reference [1] is extended to the study of neutrino/antineutrino Charged Current (CC) and Neutral Current (NC) induced nuclear reactions at intermediate energies. Long range nuclear (RPA) correlations, Final State Interaction (FSI) and Coulomb corrections are included within the model. RPA correlations are shown to play a crucial role in the whole range (100–500 MeV) of studied neutrino energies. Results for inclusive muon capture for different nuclei through the Periodic Table are also discussed. In addition, and by means of a Monte Carlo cascade method to account for the rescattering of the outgoing nucleon, we also study the CC and NC inclusive one nucleon knockout reactions off nuclei.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Early Photon-shock Interaction in a Stellar Wind: a Sub-gev Photon Flash and High Energy Neutrino Emission from Long Grbs

For gamma-ray bursts (GRBs) born in a stellar wind, as the reverse shock crosses the ejecta, usually the shocked regions are still precipitated by the prompt MeV γ−ray emission. Because of the tight overlapping of the MeV photon flow with the shocked regions, the optical depth for the GeV photons produced in the shocks is very large. These high energy photons are absorbed by the MeV photon flow...

متن کامل

Early photon-shock interaction in stellar wind: sub-GeV photon flash and high energy neutrino emission from long GRBs

For gamma-ray bursts (GRBs) born in a stellar wind, as the reverse shock crosses the ejecta, usually the shocked regions are still precipitated by the prompt MeV γ−ray emission. Because of the tight overlapping of the MeV photon flow with the shocked regions, the optical depth for the GeV photons produced in the shocks is very large. These high energy photons are absorbed by the MeV photon flow...

متن کامل

EARLY PHOTON-SHOCK INTERACTION IN A STELLAR WIND: A SUB-GeV PHOTON FLASH AND HIGH-ENERGY NEUTRINO EMISSION FROM LONG GAMMA-RAY BURSTS

For gamma-ray bursts (GRBs) born in a stellar wind, as the reverse shock crosses the ejecta, usually the shocked regions are still precipitated by the prompt MeV -ray emission. Because of the tight overlapping of the MeV photon flow with the shocked regions, the optical depth for the GeV photons produced in the shocks is very large. These high-energy photons are absorbed by the MeV photon flow ...

متن کامل

ICRR-Report-336-95-2 Calculation of the Flux of Atmospheric Neutrinos

Atmospheric neutrino{ uxes are calculated over the wide energy range from 30 MeV to 3,000 GeV for the study of neutrino{physics using the data from underground neutrino{detectors. In this calculation, a full Monte Carlo method is employed for low energy neutrinos (30 MeV { 3 GeV), while a hybrid method is used for high energy neutrinos (1 { 3,000 GeV). At low energies, the ratio ( e + e)=( +  ...

متن کامل

Charged-Current Interaction Measurements in MiniBooNE

Neutrino oscillation is the only known phenomenon for physics beyond the standard model. To investigate this phenomenon, the understanding of low energy neutrino scattering (200 < Eν < 2000 MeV) is the crucial task for high energy physicists. In this energy region, the charged current quasi-elastic (CCQE) neutrino interaction is the dominant process, and experiments require a precise model to p...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008