On the cancellation of Newtonian singularities in higher-derivative gravity
From MaRDI portal
Publication:1796919
DOI10.1016/j.physletb.2017.01.019zbMath1397.83031arXiv1609.05432OpenAlexW2523408059MaRDI QIDQ1796919
Publication date: 17 October 2018
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1609.05432
Related Items
The gravitational field of a star in quadratic gravity ⋮ On the vDVZ discontinuity in massive conformal gravity ⋮ Effective models of quantum gravity induced by Planck scale modifications in the covariant quantum algebra ⋮ Regular multi-horizon Lee-Wick black holes ⋮ Asymptotically nonlocal gravity ⋮ On black holes in higher-derivative gravities ⋮ Stability issues of black hole in non-local gravity ⋮ Relating renormalizability of D-dimensional higher-order electromagnetic and gravitational models to the classical potential at the origin ⋮ Gravitational “seesaw” and light bending in higher-derivative gravity ⋮ Light bending in \(F [g(\square) R\) extended gravity theories] ⋮ Spacetime completeness of non-singular black holes in conformal gravity ⋮ Effective delta sources and regularity in higher-derivative and ghost-free gravity
Cites Work
- Superrenormalizable quantum gravity with complex ghosts
- Super-renormalizable or finite Lee-Wick quantum gravity
- Counting ghosts in the ``ghost-free non-local gravity
- On Newtonian singularities in higher derivative gravity models
- Black holes in D = 4 higher-derivative gravity
- Renormalization of a Classical Gravitational Field Interacting with Quantized Matter Fields
- The Newtonian limit of fourth and higher order gravity
- Some Remarks on High Derivative Quantum Gravity
- Gravitational “seesaw” and light bending in higher-derivative gravity
- Simple prescription for computing the interparticle potential energy for D -dimensional gravity systems
