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arXiv 1602.04047math-phmath.APmath.MPquant-ph
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磁 Euler-Heisenberg 能量的推导

Derivation of the magnetic Euler-Heisenberg energy

Philippe Gravejat, Mathieu Lewin, Éric Séré

AI总结:

本文从与量子化 Dirac 场耦合的慢变强磁场出发,在半经典极限下严格证明极化真空能量收敛于 Euler-Heisenberg 泛函,并以 Pauli-Villars 正则化与电荷重整化处理紫外发散。

摘要:

在量子场论中,真空是一种涨落介质,其行为类似于非线性可极化材料。本文中,我们首次严格推导了磁 Euler-Heisenberg 有效能量,这是一个描述经典磁场中量子真空有效涨落的非线性泛函。我们从与处于基态的量子化 Dirac 场相互作用的经典磁场出发,研究经典磁场缓慢变化的极限。经过尺度变换后,这等价于半经典极限 $\hbar\to0$,其中磁场强度为 $1/\hbar$ 阶。在此机制下,我们证明 Dirac 极化真空的能量收敛于 Euler-Heisenberg 泛函。该模型存在紫外发散,我们采用 Pauli-Villars 方法对其进行正则化。我们还讨论了如何利用电荷重整化,在耦合常数的任意阶上以微扰方式去除 Euler-Heisenberg 有效 Lagrangian 的正则化。

英文摘要:

In quantum field theory, the vacuum is a fluctuating medium which behaves as a nonlinear polarizable material. In this article, we perform the first rigorous derivation of the magnetic Euler-Heisenberg effective energy, a nonlinear functional that describes the effective fluctuations of the quantum vacuum in a classical magnetic field. We start from a classical magnetic field in interaction with a quan-tized Dirac field in its ground state, and we study a limit in which the classical magnetic field is slowly varying. After a change of scales, this is equivalent to a semi-classical limit $\hbar\to0$, with a strong magnetic field of order $1/\hbar$. In this regime, we prove that the energy of Dirac's polarized vacuum converges to the Euler-Heisenberg functional. The model has ultraviolet divergences, which we regularize using the Pauli-Villars method. We also discuss how to remove the regularization of the Euler-Heisenberg effective Lagrangian, using charge renormaliza-tion, perturbatively to any order of the coupling constant.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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