(非)阿基米德空间上的速子膨胀

M. Milošević, G. Djordjevic
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引用次数: 1

摘要

评述了量子滚转速子及其在标准宇宙学、p进宇宙学和阿得利宇宙学框架下的暴胀情景。Sen在零维版本中提出的速子物质场论导致了粒子在不同势下运动的许多模型。我们考虑了模型的量子传播子,以及真空状态和构造线性泛化所必需的条件。此外,我们提出了一些基于解析和数值计算的有趣模型的暴胀情景。简要概述了该领域的技术现状,并提出了进一步考虑的建议。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
TACHYONIC INFLATION ON (NON-)ARCHIMEDEAN SPACES
The relevance of quantum rolling tachyons and corresponding inflation scenario in the frame of the standard, p-adic and adelic cosmology are reviewed. The field theory of tachyon matter proposed by Sen in a zero-dimensional version leads to a number of models with a particle moving under different potentials. We consider quantum propagators of the models, as well as, the vacuum states and conditions necessary to construct an adelic generalization. In addition we present inflationary scenarios for some interesting models based on analytic and numeric calculations. A brief overview of the state of art in the field and suggestions for further consideration close the paper.
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