The split property for quantum field theories in flat and curved spacetimes
Christopher J. Fewster
TL;DR
The paper addresses how spacelike-separated regions in quantum field theory can be treated as essentially independent by detailing the split property, which is stronger than Einstein causality and ties to the thermodynamic notion of locality via nuclearity. It surveys the original Minkowski-space results, elucidates the nuclearity criteria and their connection to quantum energy inequalities, and then extends the discussion to curved spacetimes using the locally covariant QFT framework, yielding a robust reduction to the ultrastatic case. A key contribution is a streamlined curved-spacetime strategy that preserves splitness along chains of Cauchy morphisms, enabling a general proof strategy for standard split inclusions and Reeh–Schlieder-type properties. The work highlights deep structural aspects of local algebras (e.g., type ${\rm III}_1$ factors), links between thermodynamic stability and QEIs, and a rigorous backbone for understanding locality in QFT across flat and curved spacetimes.
Abstract
The split property expresses a strong form of independence of spacelike separated regions in algebraic quantum field theory. In Minkowski spacetime, it can be proved under hypotheses of nuclearity. An expository account is given of nuclearity and the split property, and connections are drawn to the theory of quantum energy inequalities. In addition, a recent proof of the split property for quantum field theory in curved spacetimes is outlined, emphasising the essential ideas.
