论膨胀时空中有效作用虚部的不同计算方法的一致性

IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
E.T. Akhmedov , I.A. Belkovich , D.V. Diakonov , K.A. Kazarnovskii
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引用次数: 0

摘要

我们考虑了两种计算膨胀时空中有效作用虚部的方法。第一种方法使用Bogolyubov系数,第二种方法使用泛函积分或费曼传播算子。在永恒膨胀的时空中,这两种方法对虚部给出了不同的答案。这种差异的根源可以追溯到泛函积分中初始状态和最终状态的波泛函的存在。我们在德西特时空的膨胀庞加莱补丁的例子中明确地说明了这一点。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On (dis)agreement between different methods of calculation of the imaginary part of the effective action in expanding space-times
We consider two approaches to calculate imaginary parts of effective actions in expanding space-times. While the first approach uses Bogolyubov coefficients, the second one uses the functional integral or the Feynman propagator. In eternally expanding space-times these two approaches give different answers for the imaginary parts. The origin of the difference can be traced to the presence if the wave-functionals for the initial and final states in the functional integral. We show this explicitly on the example of the expanding Poincare patch of the de Sitter space-time.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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