Constraints on Scalar Field Dark Matter from Colocated Michelson Interferometers.

Constraints on Scalar Field Dark Matter from Colocated Michelson Interferometers.
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来自同位迈克尔逊干涉仪的标量场暗物质的约束。

DOI:
10.1103/physrevlett.128.121101
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发表时间:
2022
影响因子:
8.6
通讯作者:
Aiello L
Aiello L
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
Aiello L

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低质量(亚eV)标量场暗物质会引起基本常数的明显振荡,导致固体的尺寸和折射率相应的振荡。激光干涉仪对主分束器的尺寸和折射率的变化高度敏感。利用费米实验室全息计仪器的交叉关联数据,我们研究了在和之间的质量范围内可能存在的标量场暗物质候选者。我们为标量场暗物质的耦合参数设置了新的上限,比以前直接搜索的上限提高了3个数量级。
Low-mass (sub-eV) scalar field dark matter may induce apparent oscillations of fundamental constants, resulting in corresponding oscillations of the size and the index of refraction of solids. Laser interferometers are highly sensitive to changes in the size and index of refraction of the main beam splitter. Using cross-correlated data of the Fermilab Holometer instrument, which consists of twin colocated 40-m arm length power-recycled interferometers, we investigate the possible existence of scalar field dark matter candidates in the mass range betweenand. We set new upper limits for the coupling parameters of scalar field dark matter, improving on limits from previous direct searches by up to 3 orders of magnitude.
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