Classical and tree-level approaches to gravitational deflection in higher-derivative gravity

Abstract

Among the so-called classical tests of general relativity (GR), light bending has been confirmed with an accuracy that increases as times goes by. Here we study the gravitational deflection of photons within the framework of classical and semiclassical higher-derivative gravity (HDG) -- the only version of GR that is known up to now to be renormalizable along with its matter couplings. Since our computations are restricted to scales much below the Planck cut-off we need not be afraid of the massive spin-2 ghost that haunts HDG. An upper bound on the constant related to the $R_{\mu \nu }^2$-sector of the theory is then found by analyzing -- from a classical and semiclassical viewpoint -- the deflection angle of a photon passing by the Sun. This upper limit greatly improves that available in the literature.

arXiv comment9 pages, 7 figures. Accepted for publication in PRD

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Cited by in corpus (14)

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• Determination of Bending Angle of Light Deflection Subject to Possible Weak and Strong Quantum Gravity Effects
• The gravitational field of a star in quadratic gravity
• Time Evolution of Black Hole Perturbations in Quadratic Gravity
• Light bending by a slowly rotating source in quadratic theories of gravity
• Light Bending in the Infinite Derivative Theories of Gravity
• Light bending in $F\left[g(\square )R\right]$ extended gravity theories
• Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background
• Higher-order theories from the minimal length
• Interparticle potential energy for D-dimensional electromagnetic models from the corresponding scalar ones
• The Energy Dependence of Micro Black Hole Horizon in Quantum Gravity Theory