1979
DOI: 10.1098/rspa.1979.0130
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Casimir effect for a self-interacting scalar field

Abstract: The effect of a Ao 4 self-interaction upon the vacuum energy of a scalar field in flat space-times with boundaries and in the Einstein universe is investigated.

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Cited by 67 publications
(13 citation statements)
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“…Moreover the two-loop radiative corrections for some effective field theories have been investigated in [6,7,8]. Next, in the case of a real massive scalar field NLO correction to the energy has been computed in [9,10,11,12,13,14,15,16]. This correction is a two loop correction in this case but is O(λ).…”
Section: Introductionmentioning
confidence: 99%
“…Moreover the two-loop radiative corrections for some effective field theories have been investigated in [6,7,8]. Next, in the case of a real massive scalar field NLO correction to the energy has been computed in [9,10,11,12,13,14,15,16]. This correction is a two loop correction in this case but is O(λ).…”
Section: Introductionmentioning
confidence: 99%
“…In the paper by Kong and Ravndal [2] the same boundary conditions as here are studied with the help of a different method, namely some effective field theory and the Euler-Heisenberg Lagrangian. Their result, E 4 , is of one order α smaller than (9). The renormalization has also been discussed in the paper [4].…”
Section: Introductionmentioning
confidence: 86%
“…Their result, E 4 , is of one order α smaller than (9). The renormalization has also been discussed in the paper [4].…”
Section: Introductionmentioning
confidence: 86%
“…The first attempt to calculate the radiative correction to the Casimir energy of electromagnetic field was conducted by Bordag et al [8,9]. Later, several attempts were made in a radiative correction to the Casimir energy for other quantum fields with multiple boundary conditions [10,11,12,13,14]. In this category of problems, a renormalization program is typically used to renormalize the bare parameters.…”
Section: Introductionmentioning
confidence: 99%