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Null energy conditions in quantum field theory

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arxiv gr-qc/0209036 v2 pith:MRCU665Y submitted 2002-09-11 gr-qc

classification gr-qc
keywords quantumenergynullspacetimestatesalongaveragedfield
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For the quantised, massless, minimally coupled real scalar field in four-dimensional Minkowski space, we show (by an explicit construction) that weighted averages of the null-contracted stress-energy tensor along null geodesics are unbounded from below on the class of Hadamard states. Thus there are no quantum inequalities along null geodesics in four-dimensional Minkowski spacetime. This is in contrast to the case for two-dimensional flat spacetime, where such inequalities do exist. We discuss in detail the properties of the quantum states used in our analysis, and also show that the renormalized expectation value of the stress energy tensor evaluated in these states satisfies the averaged null energy condition (as expected), despite the nonexistence of a null-averaged quantum inequality. However, we also show that in any globally hyperbolic spacetime the null-contracted stress energy averaged over a timelike worldline does satisfy a quantum inequality bound (for both massive and massless fields). We comment briefly on the implications of our results for singularity theorems.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Curious QNEIs from QNEC: New Bounds on Null Energy in Quantum Field Theory

    hep-th 2025-10 unverdicted novelty 6.0 of 10

    Derives new state-independent lower bounds on semi-local integrals of null energy flux in QFTs of two and higher dimensions using QNEC, strong subadditivity, and modular Hamiltonians.

  2. How negative can null energy be in large N CFTs?

    hep-th 2024-12 conditional novelty 6.0 of 10

    In large N conformal field theories, states built from light scalar operators or stress tensors can have negative smeared null energy, but the negative amount is bounded by a scale set by the central charge.

  3. Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply

    astro-ph.CO 2026-05 unverdicted novelty 3.0 of 10

    Effective phantom dark energy is a background-level reconstruction that does not imply fundamental pathologies such as ghost instabilities or null energy condition violation by the underlying stress tensor.

  4. Modave lectures on energy conditions in quantum field theory and semi-classical gravity

    hep-th 2026-05 accept novelty 2.0 of 10

    Review of classical energy conditions, their quantum violations, and information-theoretic bounds for semi-classical gravity, based on Modave lectures.

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