实验室和太阳系中的筛选标量场

IF 2.5 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Universe Pub Date : 2024-07-15 DOI:10.3390/universe10070297
Hauke Fischer, Christian Käding, Mario Pitschmann
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引用次数: 0

摘要

在过去的几十年里,有大量证据表明物理学超越了粒子物理学和宇宙学这两个标准模型。众所周知,宇宙物质/能量的最大部分是 "暗 "的,由暗能量和暗物质组成。尽管在实验和理论方面都做出了大量努力,但这两种物质的起源仍然完全未知。经过筛选的标量场被假设为暗能量或暗物质的潜在候选者。其中最著名的模型有变色龙、对称子和依赖环境的稀拉顿。在这篇文章中,我们总结了对这三种模型参数的最新实验约束。为此,我们采用了来自 qBounce 合作、中子干涉测量和月球激光测距(LLR)等的实验结果。此外,还预测了卡西米尔和非牛顿力实验(Cannex)的约束条件。将这些结果与之前的结果结合起来,本文收集了对所考虑的三种屏蔽标量场模型的最新约束。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Screened Scalar Fields in the Laboratory and the Solar System
The last few decades have provided abundant evidence for physics beyond the two standard models of particle physics and cosmology. As is now known, the by far largest part of our universe’s matter/energy content lies in the ‘dark’, and consists of dark energy and dark matter. Despite intensive efforts on the experimental as well as the theoretical side, the origins of both are still completely unknown. Screened scalar fields have been hypothesized as potential candidates for dark energy or dark matter. Among these, some of the most prominent models are the chameleon, symmetron, and environment-dependent dilaton. In this article, we present a summary containing the most recent experimental constraints on the parameters of these three models. For this, experimental results have been employed from the qBounce collaboration, neutron interferometry, and Lunar Laser Ranging (LLR), among others. In addition, constraints are forecast for the Casimir and Non-Newtonian force Experiment (Cannex). Combining these results with previous ones, this article collects the most up-to-date constraints on the three considered screened scalar field models.
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来源期刊
Universe
Universe Physics and Astronomy-General Physics and Astronomy
CiteScore
4.30
自引率
17.20%
发文量
562
审稿时长
24.38 days
期刊介绍: Universe (ISSN 2218-1997) is an international peer-reviewed open access journal focused on fundamental principles in physics. It publishes reviews, research papers, communications, conference reports and short notes. Our aim is to encourage scientists to publish their research results in as much detail as possible. There is no restriction on the length of the papers.
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