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Casimir self-stress on a perfectly conducting spherical shell

โœ Scribed by Kimball A. Milton; Lester L. DeRaad Jr.; Julian Schwinger


Publisher
Elsevier Science
Year
1978
Tongue
English
Weight
690 KB
Volume
115
Category
Article
ISSN
0003-4916

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โœฆ Synopsis


The Casimir stress on a perfectly conducting uncharged sphere, due to occurrence of fluctuations in the electromagnetic field, is calculated using a source theory formulation. Two independent methods are employed: we compute (1) the total Casimir energy inside and outside the sphere, and (2) the radial component of the stress tensor on the surface. It is necessary to exercise care in allowing the field points to overlap; a correct limiting procedure supplies a "cutoff" in the frequency integration. In spite of numerous technical improvements, the result of Boyer, that the self-stress is repulsive (and not attractive as Casimir hoped), is confirmed unambiguously. The magnitude of the Casimir energy of a sphere of radius a is found, by numerical and analytic techniques, to be E = (fic/2a)(0.09235), also in agreement with the very recent result of Balian and Duplantier.


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