Exciting the Vacuum: Non-Thermal Particle Bursts and Multi-Messenger Signals from Binary Black Holes
We investigate particle production in the dynamical curved spacetime of a binary black hole system. Particle production is a well-known feature of quantum field theory in curved spacetime, underlying the Hawking and Unruh effects. Here we extend it to the time-varying gravitational perturbation sourced by a binary black hole. Treating a massless scalar field coupled to the binary metric, we compute the particle flux and radiated energy to leading order in the metric perturbation $h_{\mu\nu}$, using both the Bogoliubov transformation method and the S-matrix formalism. The perturbation is modeled with the standard quadrupole formalism, retaining the time-domain quadrupolar ($\ell=2$) contribution that dominates gravitational-wave emission. Our calculation is valid in the weak-field, large-separation inspiral regime and is not expected to capture the strong-field, nonlinear merger phase. In this regime we find a characteristic non-thermal, power-law emission with $dE/dt \propto M^{10/3}\omega^{16/3}$, in contrast to a thermal Hawking spectrum. Extending the analysis through merger that uses the numerically-relativistic metric is left to future work.