论文标题
量子场理论中的可观察到崩溃的黑洞背景
Observables in quantum field theory on a collapsing black hole background
论文作者
论文摘要
我们使用（1+1）尺寸重新归一化的应激能量张量（RSET）构建的标量可观察到的标量可观察到的量子辐射。我们计算能量密度$ \ cal U $，Flux $ \ cal f $和压力$ \ cal p $，用于任意崩溃方案和任意观察者。结果显示出清晰的结构：$ \ cal f - \ cal u $代表独立于崩溃的ingoing模式，$ \ cal f + \ cal u $代表倒塌的向外发出模式，$ \ cal p - \ cal u $代表痕量异常。我们还计算了根据感知重新归一化的应力能量张量（Perset）构建的可观察物。我们发现它们与与RSET相关的对应物相比，它们具有相同的崩溃依赖性贡献。特别是对于自由观察者而言，与相应的RSET相关的观察者相同，除了能量密度因痕量异常而异。
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 $\cal U$, flux $\cal F$ and pressure $\cal P$ for an arbitrary collapse scenario and an arbitrary observer. The results show a clear structure: $\cal F - \cal U$ represents the collapse-independent ingoing modes, $\cal F + \cal U$ represents the collapse-dependent outgoing modes and $\cal P - \cal U$ 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.
