Casimir forces and non-Newtonian gravitation

被引:91
作者
Onofrio, Roberto [1 ]
机构
[1] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA
[2] Univ Padua, Dipartimento Fis G Galilei, I-35131 Padua, Italy
来源
NEW JOURNAL OF PHYSICS | 2006年 / 8卷
关键词
D O I
10.1088/1367-2630/8/10/237
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The search for non-relativistic deviations from Newtonian gravitation can lead to new phenomena signalling the unification of gravity with the other fundamental interactions. Various recent theoretical frameworks indicate a possible window for non-Newtonian forces with gravitational coupling strength in the micrometre range. The major expected background in the same range is attributable to the Casimir force or variants of it if dielectric materials, rather than conducting ones, are considered. Here we review the measurements of the Casimir force performed so far in the micrometre range and how they determine constraints on non-Newtonian gravitation, also discussing the dominant sources of false signals. We also propose a geometry-independent parameterization of all data in terms of the measurement of the constant (h) over barc. Any Casimir force measurement should lead, once all corrections are taken into account, to a determination of the constant (h) over barc which, in order to assess the accuracy of the measurement, can be compared with its more precise value known through microscopic measurements. Although the last decade of experiments has resulted in solid demonstrations of the Casimir force, the situation is not conclusive with respect to being able to discover new physics. Future experiments and novel phenomenological analysis will be necessary to discover non-Newtonian forces or to push the window for their possible existence into regions of the parameter space which theoretically appear unnatural.
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页数:30
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