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Gravity resonance spectroscopy and dark energy symmetron fields
The European Physical Journal Special Topics ( IF 2.6 ) Pub Date : 2021-06-08 , DOI: 10.1140/epjs/s11734-021-00088-y
Tobias Jenke , Joachim Bosina , Jakob Micko , Mario Pitschmann , René Sedmik , Hartmut Abele

Spectroscopic methods allow to measure energy differences with unrivaled precision. In the case of gravity resonance spectroscopy, energy differences of different gravitational states are measured without recourse to the electromagnetic interaction. This provides a very pure and background-free look at gravitation and topics related to the central problem of dark energy and dark matter at short distances. In this article, we analyse the effect of dark energy scalar symmetron fields, a leading candidate for a screened dark energy field, and place limits in a large volume of parameter space.



中文翻译:

重力共振光谱和暗能量对称子场

光谱方法允许以无与伦比的精度测量能量差异。在重力共振光谱的情况下,测量不同重力状态的能量差异而不依赖于电磁相互作用。这提供了对引力和与短距离暗能量和暗物质中心问题相关的主题的非常纯粹和无背景的观察。在本文中,我们分析了暗能量标量对称子场(筛选暗能量场的主要候选者)的影响,并在大量参数空间中设置限制。

更新日期:2021-06-08
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