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One loop field strengths of charges and dipoles on a locally de Sitter background

机译:局部de Sitter背景下电荷和偶极子的一圈磁场强度

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We use the one loop vacuum polarization induced by scalar quantum electrodynamics to compute the electric and magnetic fields of point charges and magnetic dipoles on a locally de Sitter background. Our results are consistent with the physical picture of an inflating universe filling with a vast sea of charged particles as more and more virtual infrared scalar are ripped out of the vacuum. One consequence is that vacuum polarization quickly becomes nonperturbatively strong. Our computation employs the Schwinger–Keldysh effective field equations and is done in flat, conformal coordinates. Results are also obtained for static coordinates.
机译:我们使用由标量量子电动力学引起的单环真空极化来计算局部de Sitter背景上的点电荷和磁偶极子的电场和磁场。随着越来越多的虚拟红外标量被抽离真空,我们的结果与膨胀的宇宙充满大量带电粒子的物理图像是一致的。结果是真空极化迅速变得非干扰性强。我们的计算采用了Schwinger-Keldysh有效场方程,并在平坦的保形坐标中完成。还可以获得静态坐标的结果。

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