Maxwell and Scalar Fields in Nonstandard Cosmology

G. Scharf
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Abstract

: We study the scalar field equation and Maxwell equations in the nonstandard back-ground previously investigated. We separate the angular dependence by expanding in sphericalharmonics and solve the radial wave equations exactly by separating the variablestandr. Weobtain electric and magnetic multipole radiation as in vacuum without gravitation, but the fre-quencies get redshifted. The exact results are essential for understanding the Planckian characterof CMB properly. Abstract We study the scalar field equation and Maxwell equations in the nonstandard background previously investigated. We separate the angular dependence by expanding in spherical harmonics and solve the radial wave equations exactly by separating the variables t and r . We obtain electric and magnetic multipole radiation as in vacuum without gravitation, but the frequencies get redshifted. The exact results are essential for understanding the Planckian character of CMB properly.
非标准宇宙学中的麦克斯韦和标量场
我们研究了先前研究的非标准背景下的标量场方程和麦克斯韦方程。我们通过在球谐域中展开分离角依赖,并通过分离变量标准精确地求解径向波动方程。我们得到了在没有重力的真空中一样的电和磁多极辐射,但频率发生了红移。精确的结果对于正确理解宇宙微波背景的普朗克特性至关重要。摘要研究了非标准背景下的标量场方程和麦克斯韦方程。我们通过在球面谐波中展开来分离角依赖性通过分离变量t和r来精确地解径向波方程。在没有重力的真空中,我们得到了电和磁的多极辐射,但频率发生了红移。准确的结果对于正确理解宇宙微波背景的普朗克特性至关重要。
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