2016
DOI: 10.1002/9781119148739.ch2
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Long‐Range Interparticle Interactions

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Cited by 2 publications
(2 citation statements)
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“…are the distances between the atoms [22]. Equation (36) coincides with the known expression of the three-body component of the dispersion interaction as obtained by a standard sixth-order perturbative approach [11,[44][45][46], or also by field energy density considerations [47,48] or using effective Hamiltonians [12,49]. Our approach, however, gives a clear physical insight on the origin of the nonadditive nature of such interactions, stressing the fundamental role played by dressed spatial correlations of vacuum fluctuations.…”
Section: Three-body Dispersion Interactionssupporting
confidence: 67%
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“…are the distances between the atoms [22]. Equation (36) coincides with the known expression of the three-body component of the dispersion interaction as obtained by a standard sixth-order perturbative approach [11,[44][45][46], or also by field energy density considerations [47,48] or using effective Hamiltonians [12,49]. Our approach, however, gives a clear physical insight on the origin of the nonadditive nature of such interactions, stressing the fundamental role played by dressed spatial correlations of vacuum fluctuations.…”
Section: Three-body Dispersion Interactionssupporting
confidence: 67%
“…Secondly, although (46) vanishes if each atom is outside the causality sphere of the other two, i.e., α, β, γ > ct, it nevertheless shows relevant nonlocal aspects: for example, for times such that one atom (A, for example) is not causally connected with the other two atoms (B and C), while B and C are causally connected to each other, situation represented by the conditions β > ct, γ > ct, α < ct, the dynamical three-body interaction (45) is not vanishing. In other word, this observable interaction energy manifests a nonlocal behavior, ultimately related to the nonlocal features of the dynamical spatial correlations of the electric field, since it is not vanishing even if one atom is outside the causality sphere of the other two [13,51].…”
Section: Dynamical Three-body Casimir-polder Interactionsmentioning
confidence: 99%