Betz J, Manley J, Wright E M, Grin D, Singh S
Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA.
Department of Electrical and Computer Engineering, University of Delaware, Newark, Delaware 19716, USA.
Phys Rev Lett. 2022 Sep 23;129(13):131302. doi: 10.1103/PhysRevLett.129.131302.
A light scalar field framework of dark energy, sometimes referred to as quintessence, introduces a fifth force between normal matter objects. Screening mechanisms, such as the chameleon model, allow the scalar field to be almost massless on cosmological scales while simultaneously evading laboratory constraints. We explore the ability of existing mechanical systems to directly detect the fifth force associated with chameleons in an astrophysically viable regime where it could be dark energy. We provide analytical expressions for the weakest accessible chameleon model parameters in terms of experimentally tunable variables and apply our analysis to two mechanical systems: levitated microspheres and torsion balances, showing that the current generation of these experiments have the sensitivity to rule out a significant portion of the proposed chameleon parameter space. We also indicate regions of theoretically well-motivated chameleon parameter space to guide future experimental work.
暗能量的轻标量场框架,有时被称为第五元素,在正常物质物体之间引入了第五种力。诸如变色龙模型之类的屏蔽机制,使得标量场在宇宙学尺度上几乎无质量,同时又能规避实验室限制。我们探索现有机械系统在天体物理可行的情况下直接探测与变色龙相关的第五种力的能力,在这种情况下它可能是暗能量。我们根据实验可调变量给出了最弱可及变色龙模型参数的解析表达式,并将我们的分析应用于两种机械系统:悬浮微球和扭秤,表明这些实验的当前一代具有排除相当一部分所提出的变色龙参数空间的灵敏度。我们还指出了理论上动机充分的变色龙参数空间区域,以指导未来的实验工作。