de Sitter时空中量子化实Klein-Gordon场的一般协变理论

Q2 Physics and Astronomy
S. feng
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引用次数: 2

摘要

本文提出了德西特时空中实克莱因-戈登场的量子化方案。在维尔拜因的帮助下,我们的方案通常是协变的,这对于弯曲时空中的旋量场通常是必要的。我们首先给出一个哈密顿结构,然后按照标准方法对场进行量子化。对于自由场,将随时间变化的量子化哈密顿量用Bogliubov变换对角化,并将每一时刻的本征态解释为该时刻的观测粒子态。这一解释得到了已知的宇宙学红移公式和自由场4动量的壳上条件的支持。虽然为了方便起见,数学是在保形坐标下进行的,但整个理论可以根据一般协方差转换成任何其他坐标。结果表明,粒子状态,特别是真空状态,具有时变特性,在某一时刻的真空状态在以后的时间演化为非真空状态。给出了微扰的广义狄拉克图的形式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Generally Covariant Theory of Quantized Real Klein-Gordon Field in de Sitter Spacetime
We propose in this paper a quantization scheme for real Klein-Gordon field in de Sitter spacetime. Our scheme is generally covariant with the help of vierbein, which is necessary usually for spinor field in curved spacetime. We first present a Hamiltonian structure, then quantize the field following the standard approach. For the free field, the time-dependent quantized Hamiltonian is diagonalized by Bogliubov transformation and the eigen-states at each instant are interpreted as the observed particle states at that instant. The interpretation is supported by the known cosmological red-shift formula and the on-shell condition of 4-momentum for a free field. Though the mathematics is carried out in term of conformal coordinates for the sake of convenience, the whole theory can be transformed into any other coordinates based on general covariance. It is concluded that particle states, such as vacuum states in particular are time-dependent and vacuum states at one time evolves into non-vacuum states at later times. Formalism of perturbational is provided with en extended Dirac picture.
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
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