2018
DOI: 10.1103/physrevd.98.045015
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Role of gravity in the pair creation induced by electric fields

Abstract: We analyze the pair production induced by homogenous, time-dependent electric fields in an expanding space-time background. We point out that, in obtaining the semiclassical Maxwell equations, two distinct notions of adiabatic renormalization are possible. In Minkowski space the two recipes turn out to be equivalent. However, in the presence of gravity only the recipe requiring an adiabatic hierarchy between the gravitational and the gauge field is consistent with the conservation of the energy-momentum tensor. Show more

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Cited by 25 publications
(43 citation statements)
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“…In our analysis we make no assumptions about the background space-time geometry or the fixed, classical, electromagnetic field with which the charged scalar field interacts. Therefore our results are applicable, not only to black hole space-times, but also to scalar QED on cosmological space-times, for which the RSET has recently been computed using adiabatic regularization in two [42] and four [43] space-time dimensions.…”
Section: Introductionmentioning
confidence: 84%
“…In our analysis we make no assumptions about the background space-time geometry or the fixed, classical, electromagnetic field with which the charged scalar field interacts. Therefore our results are applicable, not only to black hole space-times, but also to scalar QED on cosmological space-times, for which the RSET has recently been computed using adiabatic regularization in two [42] and four [43] space-time dimensions.…”
Section: Introductionmentioning
confidence: 84%
“…The vacuum expectation of this observable is UV-divergent and has to be renormalized. In the context of an homogeneous and time dependent background it is very convenient to use the adiabatic regularization/renormalization method described in [18,19]. After performing the appropriated subtractions, one obtains…”
Section: A Electric Currentmentioning
confidence: 99%
“…where h k (t) are again the mode functions of the scalar field and the three last terms account for the adiabatic subtractions required by renormalization [18]. As for the electric current, we will we focus on the late time behavior.…”
Section: B Energy Densitymentioning
confidence: 99%
“…The method of adiabatic subtraction for regularization of both cases scalar and spinor QED in an expanding universe has been extensively studied in Refs. [99][100][101][102]. In this paper our main goals are investigation of the induced energy-momentum tensor of the Dirac field in de Sitter QED and further exploring validity of the adiabatic subtraction regularization.…”
Section: Introductionmentioning
confidence: 99%