We begin a systematic study of quantum energy inequalities (QEIs) in relation to local covariance. We define notions of locally covariant QEIs of both “absolute” and “difference” types and show that existing QEIs satisfy these conditions. Local covariance permits us to place constraints on the renormalized stress-energy tensor in one spacetime using QEIs derived in another, in subregions where the two spacetimes are isometric. This is of particular utility where one of the two spacetimes exhibits a high degree of symmetry and the QEIs are available in simple closed form. Various general applications are presented, including a priori constraints (depending only on geometric quantities) on the ground-state energy density in a static spacetime containing locally Minkowskian regions. In addition, we present a number of concrete calculations in both two and four dimensions that demonstrate the consistency of our bounds with various known ground- and thermal-state energy densities. Examples considered include the Rindler and Misner spacetimes, and spacetimes with toroidal spatial sections. In this paper we confine the discussion to globally hyperbolic spacetimes; subsequent papers will also discuss spacetimes with boundary and other related issues.

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5.

By a stationary state, we mean one whose n-point functions are invariant under translations along the Killing flow: wn(ψt(x1),,ψt(xn))=wn(x1,,xn), where ψt is the group of isometries associated with the Killing field.

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The proof employed in Refs. 18 and 16 proceeds by defining a function V:suppgR with V(v)=1g(v)2, and therefore only applies in the first instance to the case where g has connected support and no zeros in the interior thereof. We extend the result to more general gC0(I;R) by choosing a nonnegative χC0(I) with no zeros in the interior of its support, assumed to be connected, and which is equal to unity on the support of g. Applying Flanagan’s result to gε(τ)=g(τ)2+ε2χ(τ)2, we may take the limit ε0 to obtain Eq. (25) (cf. Cor. A.2 in Ref. 20, where the notation G=g2 is used).

51.

We have g̃(τ)2=g(τ+τ0)2, and want to show that g̃(τ)2=g(τ+τ0)2 for all τ. Differentiating and squaring yields 4g̃(τ)2g̃(τ)2=4g(τ+τ0)2g(τ+τ0)2 from which it follows that g̃(τ)2=g(τ+τ0)2 except perhaps at zeros of g̃(τ). If g̃ vanishes in a neighborhood of τ then so must g̃ and the result holds trivially. For the remaining case, choose a sequence τnτ with g̃(τn)0; since g̃(τn)2=g(τn+τ0)2, we conclude the required result by continuity as n.

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,
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,
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54.

To see this, we note that Q2(coshα)=tanhα+α(1tanh2α) and that the maximum of this expression on R+ occurs at the (unique) solution to αtanhα=1, which is numerically α0=1.199679. Now Q2(coshα0)=α0, so we find that Q2(x)α0<1.2 on [1,) as claimed.

55.

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The Friedrichs extension has a domain contained in the closure of C0(I) in the norm g+12=gg+gLg, which is equivalent to the norm of the Sobolev space W02(I) since τ4 is bounded and bounded away from zero on I. Accordingly, the closure of C0(I) is precisely W02(I) and the desired domain lies in this Sobolev space, all elements of which obey g=g=0 on I.

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65.

For a scalar field with arbitrary curvature coupling constant ε, replaced the numerical coefficient K(a) in the stress tensor with Kε(a)=n=1[cosech4(na2)+4εcosech2(na2)].

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67.

To generalize the result to a scalar field with arbitrary curvature coupling constant ζ, replace the 11 in the numerator with (1160ζ).

68.

Note that the weight function in Ref. 21 was parametrized in terms of η, rather than proper time τ: our g(τ) is related to the f(η) of Ref. 21 by g(τ)=f(τξo)ξo.

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