nLab energy condition

Context

Gravity

gravity, supergravity

Formalism

Definition

Spacetime configurations

Properties

Spacetimes

Quantum theory

Physics

physics, mathematical physics, philosophy of physics

Surveys, textbooks and lecture notes


theory (physics), model (physics)

experiment, measurement, computable physics

Contents

Idea

The theory of classical gravity (general relativity) a priori and straightforwardly admits the coupling to gravity of (matter-)fields with any covariant local Lagrangian. The resulting Einstein equations will always exist and will equate the Einstein tensor with the given stress-energy tensor of the matter fields.

While that hence gives consistent theories in themselves – a set of differential equations –, not all choices of matter Lagrangians are physically reasonable. One consistency condition for physical reasonable choices is for instance that from far away any non-vanishing matter distribution should behave as a single ball of positive mass. An energy condition is an extra condition imposed on a stress-energy tensor that is meant to reflect physical plausibility conditions of this kind.

There are various conditions of various strengths considered in the literature. One is called the dominant energy condition and that indeed implies the above asymptotic positivity of mass distributions, this is the content of the positive energy theorem.

References

Review with focus on the situation in quantum gravity:

  • Jackson R. Fliss: Modave lectures on energy conditions in quantum field theory and semi-classical gravity [arXiv:2605.18964]

See also:

On the averaged null energy condition:

On the quantum null energy condition:

Last revised on May 20, 2026 at 07:58:11. See the history of this page for a list of all contributions to it.