Spring · project 10 of 18

Neutrino radiation hazard

Every second an enormous number of neutrinos passes through the Earth and its inhabitants. Estimate the effect of these fluxes on a human being in terms of radiation dose.

  • Compute the cross section of neutrino scattering on an electron and the deep inelastic cross section on a nucleon (use the parton distributions of LHAPDF).

  • Use the fluxes of solar, atmospheric and relic neutrinos from the literature.

  • Compute the number of interactions per year in a human body of mass 70 kg and the energy deposited.

  • Convert this number of interactions into an equivalent dose (Sv/year) using the approximation \[D \approx N_{\text{events}} \cdot \langle E_{\text{dep}} \rangle \cdot \frac{Q}{m},\] where \(Q = 1\) is the weighting factor for secondary electrons and muons, \(m = 70\) kg and \(\langle E_{\text{dep}} \rangle\) is the mean energy deposited in the body in one interaction.

  • Compare this dose with the natural background and the permitted limits. Draw a conclusion: are neutrinos dangerous?

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