Vacuum local and global electromagnetic self-energies for a point-like and an extended field source
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We consider the electric and magnetic energy densities (or equivalently field fluctuations) in the space around a point-like field source in its ground state, after having subtracted the spatially uniform zero-point energy terms, and discuss the problem of their singular behavior at the source’s position. We show that the assumption of a point-like source leads, for a simple Hamiltonian model of the interaction of the source with the electromagnetic radiation field, to a divergence of the renormalized electric and magnetic energy density at the position of the source. We analyze in detail the mathematical structure of such a singularity in terms of a delta function and its derivatives. We also show that an appropriate consideration of these singular terms solves an apparent inconsistency between the total field energy and the space integral of its density. Thus the finite field energy stored in these singular terms gives an important contribution to the self-energy of the source. We then consider the case of an extended source, smeared out over a finite volume and described by an appropriate form factor. We show that in this case all divergences in local quantities such as the electric and the magnetic energy density, as well as any inconsistency between global and space-integrated local self-energies, disappear.
KeywordsEnergy Density Polarizable Body Singular Term Field Energy Singular Behavior
The authors wish to thank F. Persico, R. Messina and N. Bartolo for interesting discussions on the subject of this paper. Financial support by the Julian Schwinger Foundation, by Ministero dell’Istruzione, dell’Università e della Ricerca and by Comitato Regionale di Ricerche Nucleari e di Struttura della Materia is gratefully acknowledged. The authors acknowledge support from the ESF Research Networking Program CASIMIR.
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