The Necessity of the Hadamard Condition
Christopher J Fewster, Rainer Verch

TL;DR
This paper demonstrates that Hadamard states are essential for finite fluctuations of Wick squares in curved spacetimes, critiques S-J states for their infinite fluctuations, and shows limitations in extending states beyond double-cone regions.
Contribution
It provides a new motivation for the Hadamard condition based on fluctuation finiteness and analyzes the limitations of S-J states and state extensions in quantum field theory.
Findings
Wick squares have finite fluctuations only with Hadamard states.
S-J states generally produce infinite fluctuations, limiting their usefulness.
States cannot be extended beyond double-cone regions without singularities.
Abstract
Hadamard states are generally considered as the physical states for linear quantized fields on curved spacetimes, for several good reasons. Here, we provide a new motivation for the Hadamard condition: for "ultrastatic slab spacetimes" with compact Cauchy surface, we show that the Wick squares of all time derivatives of the quantized Klein-Gordon field have finite fluctuations only if the Wick-ordering is defined with respect to a Hadamard state. This provides a converse to an important result of Brunetti and Fredenhagen. The recently proposed "S-J (Sorkin-Johnston) states" are shown, generically, to give infinite fluctuations for the Wick square of the time derivative of the field, further limiting their utility as reasonable states. Motivated by the S-J construction, we also study the general question of extending states that are pure (or given by density matrices relative to a pure…
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