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Casimir effect for a perfectly conducting wedge in terms of local zeta function

机译:卡西米尔效应,根据局部zeta函数可实现理想导电的楔形

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The vacuum energy density of electromagnetic field inside a perfectly conducting wedge is calculated by making use of the local zeta function technique. This regularization completely eliminates divergent expressions in the course of calculations and gives rise to a finite expression for the energy density in question without any subtractions. Employment of the Hertz potentials for constructing the general solution to the Maxwell equations results in a considerable simplification of the calculations. Transition to the global zeta function is carried out by introducing a cutoff nearby the cusp at the origin. Proceeding from this the heat kernel coefficients are calculated and the high temperature asymptotics of the Helmholtz free energy and of the torque of the Casimir forces are found. The wedge singularity gives rise to a specific high temperature behavior similar toT(2) of the quantities under consideration. The obtained results are directly applicable to the free energy of a scalar massless field and electromagnetic field on the background of a cosmic string. (C) 2002 Elsevier Science (USA). [References: 33]
机译:通过使用局部zeta函数技术,可以计算出理想导电楔形内部电磁场的真空能量密度。这种正则化完全消除了计算过程中的发散表达式,并且在没有任何减法的情况下,可以使所讨论的能量密度成为有限的表达式。利用赫兹势来构造麦克斯韦方程组的一般解可大大简化计算。过渡到全局zeta函数是通过在原点附近的尖点处引入截止来实现的。由此计算出热核系数,并找到了亥姆霍兹自由能和卡西米尔力的转矩的高温渐近线。楔形奇异性引起与所考虑量的T(2)相似的特定高温行为。所得结果可直接应用于宇宙弦背景下标量无质量场的自由能和电磁场。 (C)2002 Elsevier Science(美国)。 [参考:33]

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