Quantum energy density inside a Schwarzschild black hole
Isotropy near the singularity, the trace anomaly, and conservation of energy-momentum
lead to a complete description of the quantum energy-momentum inside a Schwarzschild black hole.
Near the singularity,
it consists of Hawking radiation and negative vacuum energy in the ratio \(3:-2\),
diverging as \(\rho \propto r^{-6}\)
(Hamilton 2018).
The diverging quantum energy-momentum serves merely to exacerbate the singularity.
A full theory of quantum gravity is still needed.
The Schwarzschild singularity
