2002
DOI: 10.1007/s002200100584
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A Quantum Weak Energy Inequality¶for Dirac Fields in Curved Spacetime

Abstract: Quantum fields are well known to violate the weak energy condition of general relativity: the renormalised energy density at any given point is unbounded from below as a function of the quantum state. By contrast, for the scalar and electromagnetic fields it has been shown that weighted averages of the energy density along timelike curves satisfy 'quantum weak energy inequalities' (QWEIs) which constitute lower bounds on these quantities. Previously, Dirac QWEIs have been obtained only for massless fields in t… Show more

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Cited by 73 publications
(157 citation statements)
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References 83 publications
(205 reference statements)
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“…They have since been established for the free Klein-Gordon [22,24,26,38,10,16,8,19,47,20], Dirac [47,17,12], Maxwell [26,37,14] and Proca [14] quantum fields in both flat and curved spacetimes, the RaritaSchwinger field in Minkowski space [49], and also for general unitary positiveenergy conformal field theories in two-dimensional Minkowski space [11]. We will not give a full history of the development of the subject, referring the reader to the recent reviews [9,42].…”
Section: Quantum Energy Inequalitiesmentioning
confidence: 99%
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“…They have since been established for the free Klein-Gordon [22,24,26,38,10,16,8,19,47,20], Dirac [47,17,12], Maxwell [26,37,14] and Proca [14] quantum fields in both flat and curved spacetimes, the RaritaSchwinger field in Minkowski space [49], and also for general unitary positiveenergy conformal field theories in two-dimensional Minkowski space [11]. We will not give a full history of the development of the subject, referring the reader to the recent reviews [9,42].…”
Section: Quantum Energy Inequalitiesmentioning
confidence: 99%
“…Moreover, the same is true if f is replaced by a partial differential operator with smooth coefficients compactly supported in the coordinate patch. Microlocal formulations of the Hadamard condition are also known for the Dirac [34,30,44], Maxwell and Proca fields [14]. They may be regarded as local remnants of the spectrum condition, i.e., the Minkowski space requirement that the joint spectrum of the generators P µ of spacetime translations should lie in the future causal cone.…”
Section: Microscopic Stability: the Hadamard Conditionmentioning
confidence: 99%
“…In the particular case A = W (h) for h ∈ D(M; R), this gives 15) and, noting that each term in (A.15) is a product of smooth Klein-Gordon solutions, we use the following lemma.…”
Section: A21 Weyl Operatorsmentioning
confidence: 99%
“…The important point is that the constant c g,γ bounding the weighted integral of the energy density along γ from below may depend on the weight-function g and the curve γ, but is state-independent. To comment on this constraint, we note first that an inequality of the form (1.1) has been shown to hold for the class of Hadamard states ω of the free Klein-Gordon field and the Dirac field on arbitrary, globally hyperbolic spacetimes [12,15]. Moreover, in more special situations, the inequality (1.1) was obtained in a more specific form.…”
Section: Introductionmentioning
confidence: 99%
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