Complete interior RSET of a massless scalar in Unruh and Hartle–Hawking states approaches a universal conserved r^{-6} focusing tensor near the Schwarzschild singularity.
A mode-sum prescription for the renormalized stress energy tensor on black hole spacetimes
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abstract
In this paper, we describe an extremely efficient method for computing the renormalized stress-energy tensor of a quantum scalar field in spherically-symmetric black hole spacetimes. The method applies to a scalar field with arbitrary field parameters. We demonstrate the utility of the method by computing the renormalized stress-energy tensor for a scalar field in the Schwarzschild black hole spacetime, applying our results to discuss the null energy condition and the semi-classical backreaction.
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gr-qc 1years
2026 1verdicts
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Complete Quantum Stress Tensor Inside a Four Dimensional Schwarzschild Black Hole: A Divergent Focusing Source
Complete interior RSET of a massless scalar in Unruh and Hartle–Hawking states approaches a universal conserved r^{-6} focusing tensor near the Schwarzschild singularity.