English

Proof of the Quantum Null Energy Condition

High Energy Physics - Theory 2016-01-20 v2 General Relativity and Quantum Cosmology

Abstract

We prove the Quantum Null Energy Condition (QNEC), a lower bound on the stress tensor in terms of the second variation in a null direction of the entropy of a region. The QNEC arose previously as a consequence of the Quantum Focussing Conjecture, a proposal about quantum gravity. The QNEC itself does not involve gravity, so a proof within quantum field theory is possible. Our proof is somewhat nontrivial, suggesting that there may be alternative formulations of quantum field theory that make the QNEC more manifest. Our proof applies to free and superrenormalizable bosonic field theories, and to any points that lie on stationary null surfaces. An example is Minkowski space, where any point pp and null vector kak^a define a null plane NN (a Rindler horizon). Given any codimension-2 surface Σ\Sigma that contains pp and lies on NN, one can consider the von Neumann entropy SoutS_\text{out} of the quantum state restricted to one side of Σ\Sigma. A second variation SoutS_\text{out}^{\prime\prime} can be defined by deforming Σ\Sigma along NN, in a small neighborhood of pp with area A\cal A. The QNEC states that Tkk(p)2πlimA0Sout/A\langle T_{kk}(p) \rangle \ge \frac{\hbar}{2\pi} \lim_{{\cal A}\to 0}S_\text{out}^{ \prime\prime}/{\cal A}.

Keywords

Cite

@article{arxiv.1509.02542,
  title  = {Proof of the Quantum Null Energy Condition},
  author = {Raphael Bousso and Zachary Fisher and Jason Koeller and Stefan Leichenauer and Aron C. Wall},
  journal= {arXiv preprint arXiv:1509.02542},
  year   = {2016}
}

Comments

32 pages, 3 figures. v2: references and minor typos

R2 v1 2026-06-22T10:52:15.326Z