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Energy Density-Flux Correlations in an Unusual Quantum State and in the Vacuum

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arxiv 0706.1970 v2 pith:YBQSRW3E submitted 2007-06-13 quant-ph gr-qchep-th

classification quant-phgr-qchep-th
keywords energystatenegativehelferquantumregiondensityvacuum
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In this paper we consider the question of the degree to which negative and positive energy are intertwined. We examine in more detail a previously studied quantum state of the massless minimally coupled scalar field, which we call a ``Helfer state''. This is a state in which the energy density can be made arbitrarily negative over an arbitrarily large region of space, but only at one instant in time. In the Helfer state, the negative energy density is accompanied by rapidly time-varying energy fluxes. It is the latter feature which allows the quantum inequalities, bounds which restrict the magnitude and duration of negative energy, to hold for this class of states. An observer who initially passes through the negative energy region will quickly encounter fluxes of positive energy which subsequently enter the region. We examine in detail the correlation between the energy density and flux in the Helfer state in terms of their expectation values. We then study the correlation function between energy density and flux in the Minkowski vacuum state, for a massless minimally coupled scalar field in both two and four dimensions. In this latter analysis we examine correlation functions rather than expectation values. Remarkably, we see qualitatively similar behavior to that in the Helfer state. More specifically, an initial negative energy vacuum fluctuation in some region of space is correlated with a subsequent flux fluctuation of positive energy into the region. We speculate that the mechanism which ensures that the quantum inequalities hold in the Helfer state, as well as in other quantum states associated with negative energy, is, at least in some sense, already ``encoded'' in the fluctuations of the vacuum.

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  1. Probability Distribution for Vacuum Energy Flux Fluctuations in Two Spacetime Dimensions

    hep-th 2024-12 conditional novelty 6.0 of 10

    Time-averaged vacuum energy flux in 2D CFT follows a symmetric variance-gamma distribution, and the joint flux-energy density distribution is explicitly constructed.

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