Neutrino cross sections and nuclear structure
نویسندگان
چکیده
منابع مشابه
Total neutrino and antineutrino nuclear cross sections around 1 GeV
We investigate neutrino-nucleus interactions at energies around 1 GeV. In this regime, the main contributions to the cross sections come from quasi-elastic and ∆ production processes. Our formalism, based on the Impulse Approximation is well suited to describe both types of interactions. We focus on a series of important nuclear effects in the interaction of electron neutrinos with 16O, also re...
متن کاملNeutrino nucleus cross sections
We present the results of our calculation which has been performed to study the nuclear effects in the quasielastic, inelastic and deep inelastic scattering of neutrinos(antineutrinos) from nuclear targets. These calculations are done in the local density approximation. We take into account the effect of Pauli blocking, Fermi motion, Coulomb effect, renormalization of weak transition strengths ...
متن کاملSuperscaling and Charge-changing Neutrino Cross Sections
Dip. di Fisica Teorica, Univ. di Torino and INFN, Via P. Giuria 1, I10125 Turin, Italy, Dep. de F́ısica Moderna, Univ. de Granada, 18071 Granada, Spain, Dep. de F́ısica Atómica, Molecular y Nuclear, Univ. de Sevilla, Apdo. 1065, 41080 Sevilla, Spain, CTP, LNS and Dep. of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA, Dep. für Physik und Astronomie, Univ. Basel, CH-4056 ...
متن کاملNeutrino Cross Sections and Scattering Physics
Large flux uncertainties and small cross sections have made neutrino scattering physics a challenge. However, a worthwhile challenge, as these tiny particle interactions can teach us a lot about neutrinos themselves, the weak interaction, and nucleon structure. As well, knowledge of these cross sections is crucial input to the growing field of neutrino oscillation physics. New, intense, well un...
متن کاملNeutrino Cross Sections at HERA and Beyond
The sources of very high energy cosmic rays should also be sources of neutrinos. While the complete scheme of ultrahigh energy cosmic ray production is not yet understood [1], ancillary to cosmic ray production are neutrino fluxes, both at the source of the cosmic rays and through cosmic ray propagation and scattering with the microwave background. Given that neutrinos are unabsorbed and undefl...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Nuclear Physics B - Proceedings Supplements
سال: 2009
ISSN: 0920-5632
DOI: 10.1016/j.nuclphysbps.2009.02.033