Shocks in the Early Universe

Understand

We point out a surprising consequence of the usually assumed initial conditions for cosmological perturbations.

• Namely, a spectrum of Gaussian, linear, adiabatic, scalar, growing mode perturbations not only creates acoustic oscillations of the kind observed on very large scales today, it also leads to the production of shocks in the radiation fluid of the very early universe.
• Shocks cause departures from local thermal equilibrium as well as creating vorticity and gravitational waves.
• For a scale-invariant spectrum and standard model physics, shocks form for temperatures $1$ GeV$<T<10^{7}$ GeV.