Semi-local Bounds on Null Energy in QFT
Jackson R. Fliss, Ben Freivogel

TL;DR
This paper proves a lower bound on the smeared null energy in quantum field theory using light-sheet quantization, introduces a double-smeared bound that is UV cutoff independent, and discusses its behavior with respect to smearing scales.
Contribution
It establishes the Smeared Null Energy Condition (SNEC) for free and super-renormalizable QFTs and proposes the Double-Smeared Null Energy Condition (dSNEC) as a UV-independent lower bound.
Findings
Proves SNEC for free and super-renormalizable QFTs with a UV cutoff.
Shows that smearing on a light-sheet alone cannot improve the bound.
Introduces dSNEC, a bound involving smearing over two null directions, independent of UV cutoff.
Abstract
We investigate whether the null energy, averaged over some region of spacetime, is bounded below in QFT. First, we use light-sheet quantization to prove a version of the "Smeared Null Energy Condition" (SNEC) proposed in [1], applicable for free and super-renormalizable QFT's equipped with a UV cutoff. Through an explicit construction of squeezed states, we show that the SNEC bound cannot be improved by smearing on a light-sheet alone. We propose that smearing the null energy over two null directions defines an operator that is bounded below and independent of the UV cutoff, in what we call the "Double-Smeared Null Energy Condition," or dSNEC. We indicate schematically how this bound behaves with respect to the smearing lengths and argue that the dSNEC displays a transition when the smearing lengths are comparable to the correlation length.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Algebraic structures and combinatorial models
