2020
DOI: 10.21468/scipostphys.8.4.064
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A bound on thermal relativistic correlators at large spacelike momenta

Abstract: We consider thermal Wightman correlators in a relativistic quantum field theory in the limit where the spatial momenta of the insertions become large while their frequencies stay fixed. We show that, in this limit, the size of these correlators is bounded by e −βR , where R is the radius of the smallest sphere that contains the polygon formed by the momenta. We show that perturbative quantum field theories can saturate this bound through suitably highorder loop diagrams. We also consider holographic theories i… Show more

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Cited by 13 publications
(17 citation statements)
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“…Our results suggest that this a general phenomenon associated with composite operators in non-trivial backgrounds, independent of coupling strength. Indeed, similar behaviour has been observed in thermal free field theory [10,11,2] and there are general arguments for a thermal field theory bound on the size of spacelike correlators at large momenta [12], for any coupling. More generally, composite operators are sensitive to non-trivial backgrounds, both thermal and non-thermal, at both weak and strong coupling.…”
Section: Discussionsupporting
confidence: 73%
See 1 more Smart Citation
“…Our results suggest that this a general phenomenon associated with composite operators in non-trivial backgrounds, independent of coupling strength. Indeed, similar behaviour has been observed in thermal free field theory [10,11,2] and there are general arguments for a thermal field theory bound on the size of spacelike correlators at large momenta [12], for any coupling. More generally, composite operators are sensitive to non-trivial backgrounds, both thermal and non-thermal, at both weak and strong coupling.…”
Section: Discussionsupporting
confidence: 73%
“…The presence of spacelike correlations has been seen previously in certain large N thermal field theories, even in the limit of vanishing coupling [10,11,2]. That different momentum modes thermalise independently after the quench however means that recent bounds [12] on correlations at spacelike momenta, obtained from thermal field theory, are not applicable.…”
Section: Introductionmentioning
confidence: 91%
“…A motivation behind the operator thermalisation hypothesis, and one of its strengths, is that it can be used to study surprising similarities between ordinary interacting systems and free or integrable systems [6,10,11,13]. While pure exponential decay occurs in free systems in contrast to naive expectations, it is generally masked by leading power law decay for d > 2, as well as multiplied by inverse powers of time.…”
Section: Jhep09(2020)103mentioning
confidence: 99%
“…Such operators can in fact interact with the thermal bath and as such exhibit a range of phenomena that are usually attributed to their interacting counterparts. For instance, their correlation functions can exhibit exponential decay at late times [10] and JHEP09(2020)103 their spectral densities have support in the deeply off-shell regime [10,11], reminiscent of collision-less Landau damping [12].…”
Section: Introductionmentioning
confidence: 99%
“…The states |n of the CFT are forced to satisfy the condition E n ≥ |P n |, but this does not necessarily force ρ(k, ω) to be zero if |k| > |ω|. An intuitive explanation [7] is that in the thermal background φ can create a particle with some energy E and momentum k and destroy another one with a similar energy but opposite momentum. This excitation will have a small energy but possibly large momentum.…”
Section: Introductionmentioning
confidence: 99%