TESTS OF THE GRAVITATIONAL INVERSE-SQUARE LAW
By E. Adelberger, B. Heckel, A. Nelson. 2003
696 citations recorded by the source corpus.
▪ Abstract We review recent experimental tests of the gravitational inverse-square law and the wide variety of theoretical considerations that suggest the law may break down in experimentally accessible regions.
Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/7929eb30c21f07f45acff46900927c0e99c6ea9f
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In Astronomy and Astrophysics
- C. Burgess
- Antonio Padilla
- William M. Folkner
- Pedro G. Ferreira
- T. Clifton
- Maria T. Zuber
- C. Will
- C. Skordis
In Statistical and Nonlinear Physics
Citations in the corpus
- Beyond the Cosmological Standard Model (2014, neutral): “For other searches for deviations from the inverse square law, see [843–850] and for a review of these types of experiments, see [851]”
- Torsion-balance tests of the weak equivalence principle (2012, background): “An anomalous precession of the moon’s orbit around earth [3] 2.”
- The Cosmological Constant Problem: Why it's hard to get Dark Energy from Micro-physics (2013, background): “be. Tests of Newton’s inverse-square law provide the strongest constraints on the existence of extra dimensions in the sub-eV range. In the conventions used here, these presently give an upper limit [47] L<L e’45 m, and so 1=L>1=L e’4 10 3 eV, so L<L e is not inconsistent with (2.31) or (2.”
- The Confrontation between General Relativity and Experiment (2005, background): “For a comprehensive review of both the theory and the experiments, see [3].”
- Dark energy from mass varying neutrinos (2003, background): “g Range Forces Could the acceleron mediate forces between other particles than neutrinos? There are strong limits on new forces for between nucleons and/or electrons at scales longer than 100 microns [51]. For instance, the operators me(A)¯ee , md(A)dd , m¯ u(A)¯uu , 1 g2 s(A) Ga µνG a,µν . (5.1) 3A”
- Spin-dependent macroscopic forces from new particle exchange (2006, background): “9) where the weaker limit applies to 1/m0 of order 1 cm, while the stronger one applies to 1/m0 > 10 8 m, the Earth-Moon distance (see figure 4 of [1]).”
- Mars high resolution gravity fields from MRO, Mars seasonal gravity, and other dynamical parameters (2011, background): “31 also shows estimates of a at other length scales from other experiments as summarized by Adelberger et al. (2003).”
- Search for New Physics with Atoms and Molecules (2017, background): “In the AEgIS expariment, a cold, pulsed beam of antihydrogen will pass through a moiré deflectometer (Aghion et al., 2014), coupled to a position-sensitive detector to measure the strength of the gravitational interaction between matter and antimatter to a precision of 1%. A second goal of the AEgIS”