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Experimental limits on the free parameters of higher-derivative gravity

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arxiv 1612.01823 v1 pith:672XWWX5 submitted 2016-12-06 gr-qc

classification gr-qc
keywords gravitybetaexperimentalfreehigher-derivativelimitsparametersalpha
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abstract

Fourth-derivative gravity has two free parameters, $\alpha$ and $\beta$, which couple the curvature-squared terms $R^2$ and $R_{\mu\nu}^2$. Relativistic effects and short-range laboratory experiments can be used to provide upper limits to these constants. In this work we briefly review both types of experimental results in the context of higher-derivative gravity. The strictest limit follows from the second kind of test. Interestingly enough, the bound on $\beta$ due to semiclassical light deflection at the solar limb is only one order of magnitude larger.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Rotating near-horizon extreme geometries in quadratic gravity

    gr-qc 2026-08 conditional novelty 6.0 of 10

    New regular Bachian near-horizon extreme geometries are found in Einstein-Weyl gravity, and their horizon area is bounded above, suggesting microscopic extremal rotating black holes.

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