Hawking's area theorem with a weaker energy condition
Martin Lesourd

TL;DR
This paper explores a strengthened version of Hawking's area theorem that relies on a weaker energy condition, potentially applicable in semi-classical contexts where null energy condition violations occur.
Contribution
It introduces a new formulation of the area theorem based on a less restrictive energy condition, expanding its applicability beyond classical null energy assumptions.
Findings
Theorem holds under weakened energy conditions.
Potential relevance to semi-classical quantum effects.
Discussion on the validity of energy conditions in quantum regimes.
Abstract
Hawking's area theorem is a fundamental result in black hole theory that is universally associated with the null energy condition. That this condition can be weakened is illustrated by the formulation of a strengthened version of the theorem based on an energy condition that allows for violations of the null energy condition. With the semi-classical context in mind, some brief remarks pertaining to the suitability of the area theorem and its energy condition are made.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
