Shocks in the Early Universe

TL;DR

This paper reveals that initial conditions for cosmological perturbations can produce shocks in the early universe's radiation fluid, leading to observable effects like gravitational waves that can constrain early universe models.

Contribution

It demonstrates that Gaussian perturbations can generate shocks in the early universe, linking primordial conditions to observable gravitational wave signals.

Findings

Shocks form in the radiation fluid for temperatures between 1 GeV and 10^7 GeV.

Shock formation leads to vorticity and gravitational waves.

Gravitational wave signals can constrain early universe conditions.

Abstract

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. For more general power spectra, such as have been invoked to form primordial black holes, shock formation and the consequent gravitational wave emission provides a signal detectable by current and planned gravitational wave experiments, allowing them to strongly constrain conditions present in the primordial universe as early as $10^{-30}$ seconds after the big bang.