Introduction to Cosmology Ryden · Problem 9.5

Nucleosynthesis and the Early Universe

Physics — Astrophysics · cosmic-neutrino-background-interaction

Problem

The typical energy of a neutrino in the cosmic neutrino background, as pointed out in Chapter 5, is Eν∼kTν∼5×10−4 eVE_\nu \sim kT_\nu \sim 5 \times 10^{-4}\,\text{eV}. What is the approximate interaction cross-section σw\sigma_w for one of these cosmic neutrinos? Suppose you had a large lump of 56^{56}Fe (with density ρ=7900 kg m−3\rho = 7900\,\text{kg}\,\text{m}^{-3}). What is the number density of protons, neutrons, and electrons within the lump of iron? How far, on average, would a cosmic neutrino travel through the iron before interacting with a proton, neutron, or electron? (Assume that the cross-section for interaction is simply σw\sigma_w, regardless of the type of particle the neutrino interacts with.)

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