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Exact Spherically Symmetric Solutions in Massive Gravity

Z. Berezhiani, D. Comelli, F. Nesti, L. Pilo

TL;DR

The paper addresses how to construct a viable infrared modification of gravity by coupling our metric to an extra spin-2 field, yielding a Lorentz-breaking bigravity theory. It develops exact non-linear, static, spherically symmetric solutions that generalize Schwarzschild and reveal a novel power-law correction $S\,r^{\gamma}$ and a source-size dependent mass shift, signaling a dynamical violation of the Strong Equivalence Principle. The analysis shows that linearized results fail to capture the full IR behavior, and it explores decoupling and Lorentz-invariant limits, finding a well-behaved LI phase with massless gravitons but distinct non-perturbative structure. The findings have implications for the phenomenology of massive gravity, including potential astrophysical effects, local Lorentz violation near sources, and cosmological considerations, while leaving stability and Vainshtein-type issues as avenues for further study.

Abstract

A phase of massive gravity free from pathologies can be obtained by coupling the metric to an additional spin-two field. We study the gravitational field produced by a static spherically symmetric body, by finding the exact solution that generalizes the Schwarzschild metric to the case of massive gravity. Besides the usual 1/r term, the main effects of the new spin-two field are a shift of the total mass of the body and the presence of a new power-like term, with sizes determined by the mass and the shape (the radius) of the source. These modifications, being source dependent, give rise to a dynamical violation of the Strong Equivalence Principle. Depending on the details of the coupling of the new field, the power-like term may dominate at large distances or even in the ultraviolet. The effect persists also when the dynamics of the extra field is decoupled.

Exact Spherically Symmetric Solutions in Massive Gravity

TL;DR

The paper addresses how to construct a viable infrared modification of gravity by coupling our metric to an extra spin-2 field, yielding a Lorentz-breaking bigravity theory. It develops exact non-linear, static, spherically symmetric solutions that generalize Schwarzschild and reveal a novel power-law correction and a source-size dependent mass shift, signaling a dynamical violation of the Strong Equivalence Principle. The analysis shows that linearized results fail to capture the full IR behavior, and it explores decoupling and Lorentz-invariant limits, finding a well-behaved LI phase with massless gravitons but distinct non-perturbative structure. The findings have implications for the phenomenology of massive gravity, including potential astrophysical effects, local Lorentz violation near sources, and cosmological considerations, while leaving stability and Vainshtein-type issues as avenues for further study.

Abstract

A phase of massive gravity free from pathologies can be obtained by coupling the metric to an additional spin-two field. We study the gravitational field produced by a static spherically symmetric body, by finding the exact solution that generalizes the Schwarzschild metric to the case of massive gravity. Besides the usual 1/r term, the main effects of the new spin-two field are a shift of the total mass of the body and the presence of a new power-like term, with sizes determined by the mass and the shape (the radius) of the source. These modifications, being source dependent, give rise to a dynamical violation of the Strong Equivalence Principle. Depending on the details of the coupling of the new field, the power-like term may dominate at large distances or even in the ultraviolet. The effect persists also when the dynamics of the extra field is decoupled.

Paper Structure

This paper contains 20 sections, 62 equations.