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Time reparameterization in Bianchi type I spinor cosmology

机译:Bianchi I型旋子宇宙学中的时间重新参数化

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The problem of time reparameterization is addressed at both the classical and quantum levels in a Bianchi-I universe in which the matter source is a massive Dirac spinor field. We take the scale factors of the metric as the intrinsic time and their conjugate momenta as the extrinsic time. A scalar character of the spinor field is identified as a representation of the extrinsic time. The construction of the field equations and quantization of the model is achieved by solving the Hamiltonian constraint after time identification has been dealt with. This procedure leads to a true Hamiltonian whose exact solutions for the above choices of time are presented. (C) 2008 Published by Elsevier Inc.
机译:时间重新参数化的问题在Bianchi-I宇宙的经典和量子水平上都得到了解决,在该宇宙中,物质源是巨大的狄拉克旋子场。我们将度量的比例因子作为内在时间,将其共轭矩作为外在时间。旋转子场的标量特征被标识为外部时间的表示。在解决了时间识别问题后,通过求解哈密顿约束来实现场方程的构建和模型的量化。该过程导致了真正的哈密顿量,给出了上述时间选择的精确解。 (C)2008由Elsevier Inc.发布

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