Energy spectrum of gravitational waves

Abstract

The energy spectrum of gravitational waves (GWs), which depicts the energy of GWs per unit volume of space per logarithmic frequency interval normalized to the critical density of the Universe, is a widely used way for quantifying the sensitivity of GW detectors and the strength of GWs, since it has the advantage of having a clear physical meaning. It was found that the energy spectrum of GWs depends on the gauge when the GWs beyond the linear order perturbations are considered. We show that this gauge dependence issue originates from the inappropriate description for the energy of GWs. With the proper description for the energy of GWs, we give a well-defined energy spectrum of GWs, in which the gauge issue disappears naturally.