black hole spacetimes | vanishing angular momentum | positive angular momentum |
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vanishing charge | Schwarzschild spacetime | Kerr spacetime |
positive charge | Reissner-Nordstrom spacetime | Kerr-Newman spacetime |
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Types of quantum field thories
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.
See also:
Discussion of the averaged null energy condition? for conformal field theory on de Sitter spacetime and anti de Sitter spacetime:
See also:
Taha A Malik, Rafael Lopez-Mobilia, Proof of the quantum null energy condition for free fermionic field theories (arXiv:1910.07594)
Philipp Stanzer, Numerical Relativity, Holography and the Quantum Null Energy Condition (arXiv:2009.07040)
Last revised on July 14, 2022 at 12:18:59. See the history of this page for a list of all contributions to it.