کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
5495794 1529828 2017 42 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
In medium dispersion relation effects in nuclear inclusive reactions at intermediate and low energies
ترجمه فارسی عنوان
در اثرات ارتباط پراکندگی متوسط ​​در واکنش های اتمی فراگیر در انرژی های متوسط ​​و کم
موضوعات مرتبط
مهندسی و علوم پایه فیزیک و نجوم فیزیک و نجوم (عمومی)
چکیده انگلیسی


- The role of the spectral functions (SFs) in neutrino nucleus reactions is studied.
- Accurate SFs are used to predict intermediate energy CCQE (anti-)neutrino scattering for various targets.
- We compare our SF and RPA results to predictions obtained within other representative approaches.
- We show that uncertainties on the σμ∕σe ratio are much smaller than 5%.

In a well-established many-body framework, successful in modeling a great variety of nuclear processes, we analyze the role of the spectral functions (SFs) accounting for the modifications of the dispersion relation of nucleons embedded in a nuclear medium. We concentrate in processes mostly governed by one-body mechanisms, and study possible approximations to evaluate the particle-hole propagator using SFs. We also investigate how to include together SFs and long-range RPA-correlation corrections in the evaluation of nuclear response functions, discussing the existing interplay between both type of nuclear effects. At low energy transfers (≤50MeV), we compare our predictions for inclusive muon and radiative pion captures in nuclei, and charge-current (CC) neutrino-nucleus cross sections with experimental results. We also present an analysis of intermediate energy quasi-elastic neutrino scattering for various targets and both neutrino and antineutrino CC driven processes. In all cases, we pay special attention to estimate the uncertainties affecting the theoretical predictions. In particular, we show that errors on the σμ∕σe ratio are much smaller than 5%, and also much smaller than the size of the SF+RPA nuclear corrections, which produce significant effects, not only in the individual cross sections, but also in their ratio for neutrino energies below 400 MeV. These latter nuclear corrections, beyond Pauli blocking, turn out to be thus essential to achieve a correct theoretical understanding of this ratio of cross sections of interest for appearance neutrino oscillation experiments. We also briefly compare our SF and RPA results to predictions obtained within other representative approaches.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Annals of Physics - Volume 383, August 2017, Pages 455-496
نویسندگان
, ,