Observables in quantum field theory on a collapsing black hole background

Abstract

We study the quantum radiation from a curved background using scalar observables constructed from the (1+1) dimensional renormalized stress-energy tensor (RSET). We compute energy density U, flux F and pressure P for an arbitrary collapse scenario and an arbitrary observer. The results show a clear structure: F−U represents the collapse-independent ingoing modes, F+U represents the collapse-dependent outgoing modes and P−U represents the trace anomaly. We also compute the observables constructed from the perception renormalized stress-energy tensor (PeRSET). We find they have the same collapse-dependent contribution comparing to their RSET-related counterparts. For free-falling observers, in particular, the PeRSET-related observables are the same as the corresponding RSET-related ones, except the energy densities differ by the trace anomaly.