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Experimental limits on the free parameters of higher-derivative gravity
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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
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Rotating near-horizon extreme geometries in quadratic gravity
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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