Ultrahigh-energy neutrino-nucleon deep-inelastic scattering and the Froissart bound.

نویسندگان

  • Alexey Yu Illarionov
  • Bernd A Kniehl
  • Anatoly V Kotikov
چکیده

We present a simple formula for the total cross section σ(νN) of neutral- and charged-current deep-inelastic scattering of ultrahigh-energy neutrinos on isoscalar nuclear targets, which is proportional to the structure function F(2)(νN)(M(V)(2)/s,M(V)(2)), where M(V) is the intermediate-boson mass and s is the square of the center-of-mass energy. The coefficient in front of F(2)(νN)(x,Q(2)) depends on the asymptotic low-x behavior of F(2)(νN). It contains an additional lns term if F(2)(νN) scales with a power of ln(1/x). Hence, an asymptotic low-x behavior F(2)(νN)∝ln(2)(1/x), which is frequently assumed in the literature, already leads to a violation of the Froissart bound on σ(νN).

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

Ultrahigh-Energy Neutrino-Nucleon Cross Sections and Perturbative Unitarity

Unitarity relates the total cross section for neutrino-nucleon scattering to the neutrino-nucleon forward scattering amplitude. Assuming the validity of the perturbative expansion of the forward amplitude in the weak coupling constant, we derive a unitarity bound on the inelastic cross section. The inelastic cross section saturates this bound at a typical neutrino energy Eν ≃ 108 GeV. This impl...

متن کامل

Ultrahigh energy neutrino scattering: an update

We update our estimates of charged and neutral current neutrino total cross sections on isoscalar nucleons at ultrahigh energies using a global (x, Q) fit, motivated by the Froissart bound [1], to the F2 (electron-proton) structure function utilizing the most recent analysis [2] of the complete ZEUS and H1 data sets from HERA I. Using the large Q, small Bjorken-x limits of the “wee” parton mode...

متن کامل

Flux Independent Measurements of Deep Inelastic Neutrino Processes

2 BP The scaling variable v = xy = 2(Ep/M) sin 2 is useful for the description of deep inelastic neutrino-nucleon scattering processes. This variable is determined solely by the momentum and angle of the outgoing lepton. The normalized scattering distribution in this variable is independent of incident lepton energy and flux, provided scale-invariance is valid. The sensitivity to various hypoth...

متن کامل

Radiative Corrections to Deep-Inelastic Neutrino–Nucleon Scattering in the MSSM

In the Standard Model (SM), neutral (NC) and charged current (CC) neutrino–nucleon scattering are described in leading order by t-channel W and Z exchange, respectively (see Fig. 1). At the NuTeV experiment, νμ and ν̄μ beams of a mean energy of 125 GeV were scattered off a target detector and the ratios R = σ NC/σ ν CC and R ν̄ = σ NC/σ ν̄ CC were measured. The NuTeV collaboration also provided a ...

متن کامل

Neutrino 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 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:
  • Physical review letters

دوره 106 23  شماره 

صفحات  -

تاریخ انتشار 2011