首页> 外文会议>Marcel Grossmann Meeting on General Relativity >ABSORPTION CROSS SECTIONS OF LOW ENERGY PHOTONS FOR THE SCHWARZSCHILD AND EXTREME REISSNER-NORDSTR?M BLACK HOLES IN ARBITRARY DIMENSIONS HIGHER THAN THREE
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ABSORPTION CROSS SECTIONS OF LOW ENERGY PHOTONS FOR THE SCHWARZSCHILD AND EXTREME REISSNER-NORDSTR?M BLACK HOLES IN ARBITRARY DIMENSIONS HIGHER THAN THREE

机译:对于施瓦茨德和极端重新销料-NORDSTR的低能量光子的吸收横截面,任意尺寸高于三个

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We examine the electromagnetic field quantization in static spherically symmetric spacetimes of arbitrary n dimensions in a modified Feynman gauge. This gauge is closely related to the A0= 0 gauge and reduces to the Feynman gauge in Minkowski spacetime. The electromagnetic field equations in a black hole spacetime are not decoupled and are difficult to analyze in the Lorenz gauge. However, if we require the field to be divergence free on a (n - 2)-sphere (the spherical Coulomb gauge), the equations for the physical modes reduce to decoupled scalar field equations. Furthermore, solutions in terms of familiar special functions can be found in the low-energy regime. By using the electromagnetic field modes obtained in this modified Feynman gauge we calculate the low energy absorption cross sections of photons for the Schwarzschild and extreme Reissner-Nordstrom black holes in arbitrary dimensions higher than three.
机译:在改进的Feynman仪表中,研究了任意N尺寸的静态球对称时空的电磁场量化。该仪表与A0 = 0仪表密切相关,并减少了Minkowski Spacetime的Feynman Cauge。黑洞时空中的电磁场方程没有解耦并且难以在Lorenz测量处分析。但是,如果我们要求在(n - 2) - 舍尔(球形库仑计)上无分歧,则物理模式的方程减少到分离的标量场方程。此外,可以在低能量方案中找到熟悉的特殊功能方面的解决方案。通过使用该改进的Feynman表中获得的电磁场模式,我们计算施瓦茨德和极端重新销料 - Nordstrom黑洞的低能量吸收横截面,以高于三个。

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