In this work we investigate an interesting connection between the absence of Newtonian singularities in the classical non-relativistic potential and renormalizability properties in Higher-Derivative models of Quantum Gravity. In the framework of a large class of Ddimensional Higher-Derivative models of Quantum Gravity, we compute the non-relativistic potential energy associated with two point-like masses. Investigating its behavior for small distances, we find an algebraic condition which is sufficient for the cancellation of the Newtonian singularity. We verify that the same condition is necessary to ensure power-counting renormalizability and, as a consequence, we conclude that renormalizable Higher-Derivative models do not exhibit the so-called newtonian singularity. Finally, we discuss the role of ghosts in the mechanism for the cancellation of Newtonian singularities.
I. INTRODUCTIONThe quest for a quantum gravity theory is still one of the most important problems of theoretical physics. As is well known, the biggest challenge in the construction of a quantum theory for the gravitational interaction is the lack of experimental evidences concerning gravity at the microscopic level. Despite that, however, there exist several approaches to quantum gravity which were proposed in the last few decades. For instance: string theory, loop quantum gravity, causal dynamical triangulations, causal sets and induced quantum gravity [1,2]. Nevertheless, none of the aforementioned theories can be considered a complete quantum gravity theory up to now.At the classical level, the gravitational interaction is very well described in terms of Einstein's general relativity (GR), which is confirmed for the excellent concordance between its theoretical predictions and the available experimental tests (e.g.