Neutrino cross-section in ultrahigh energy regime using double asymptotic limit of QCD

被引:0
|
作者
Kalpana Bora
Neelakshi Sarma
Jaydip Singh
机构
[1] Gauhati University,Department of Physics
[2] Lucknow University,Department of Physics
来源
Pramana | 2017年 / 89卷
关键词
Neutrino cross-section; ultrahigh energy; quantum chromodynamics; double asymptotic limit; dynamic pomeron; Reggeon; 13.15.+g; 13.85.Lg; 12.40.Nn;
D O I
暂无
中图分类号
学科分类号
摘要
Studies on neutrino–nucleon (νN\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\nu }N$$\end{document}) cross-sections have regained interest due to increasing importance of precision measurements, as they are needed as an ingredient in all neutrino experiments. In this work, we use the QCD-inspired double asymptotic limit fit of electron–proton structure function F2ep\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$F_{2}^{ep}$$\end{document} to low-x\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ x $$\end{document} HERA data, to calculate ν\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\nu $$\end{document}N cross-section for charged current (CC) and neutral current (NC) neutrino interactions in ultrahigh energy (UHE) neutrino energy (Eν\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_{\nu }$$\end{document}) regime (109GeV≤Eν≤1012GeV\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10^{9}\, \mathrm {GeV} \le E_{\nu } \le 10^{12}\, \mathrm {GeV} $$\end{document}). The form F2ep∼x-λ(Q2)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$F_{2}^{ep} \sim x^{-\lambda (Q^{2})}$$\end{document}, used in our analysis, can be conjectured like a dynamic pomeron (DP)-type behaviour. We also find an analytic form of the total cross-sections, σCCνN\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\sigma _{\mathrm {CC}}^{\nu N}$$\end{document} and σNCνN\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\sigma _{\mathrm {NC}}^{\nu N}$$\end{document}, which appear to be of Reggeon exchange type. We also do a comparative analysis of our results with those available in literature. Future measurements will support / confront our predictions.
引用
收藏
相关论文
共 50 条
  • [1] Neutrino cross-section in ultrahigh energy regime using double asymptotic limit of QCD
    Bora, Kalpana
    Sarma, Neelakshi
    Singh, Jaydip
    PRAMANA-JOURNAL OF PHYSICS, 2017, 89 (04):
  • [2] A LIMIT ON THE NEUTRINO NEUTRINO SCATTERING CROSS-SECTION FROM THE SUPERNOVA
    MANOHAR, A
    PHYSICS LETTERS B, 1987, 192 (1-2) : 217 - 218
  • [3] Dynamical QCD predictions for ultrahigh energy neutrino cross sections
    Glück, M
    Kretzer, S
    Reye, E
    ASTROPARTICLE PHYSICS, 1999, 11 (03) : 327 - 334
  • [4] SMALL-CHI-QCD AND THE ULTRAHIGH ENERGY NU-N TOTAL CROSS-SECTION
    MCKAY, DW
    RALSTON, JP
    PHYSICS LETTERS B, 1986, 167 (01) : 103 - 107
  • [5] Quantifying uncertainties in the high-energy neutrino cross-section
    A COOPER-SARKAR
    P MERTSCH
    S SARKAR
    Pramana, 2012, 79 : 1301 - 1308
  • [6] Low-energy neutrino cross-section measurements at SNS
    Stancu, I
    NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2006, 155 : 251 - 253
  • [7] ENERGY DEPENDENCE OF INELASTIC NEUTRINO CROSS-SECTION IN RESONANCE MODEL
    KAWAKAMI, A
    FUKAWA, M
    NUOVO CIMENTO, 1965, 38 (04): : 1875 - +
  • [8] Quantifying uncertainties in the high-energy neutrino cross-section
    Cooper-Sarkar, A.
    Mertsch, P.
    Sarkar, S.
    PRAMANA-JOURNAL OF PHYSICS, 2012, 79 (05): : 1301 - 1308
  • [9] High-energy limit of neutrino quasielastic cross section
    Ankowski, AM
    ACTA PHYSICA POLONICA B, 2006, 37 (02): : 377 - 387
  • [10] ASYMPTOTIC CONDITION TO CROSS-SECTION
    MARTIN, PA
    HELVETICA PHYSICA ACTA, 1972, 45 (05): : 794 - 801