On the theory of spherically symmetric thin shells in conformal gravity
Victor Berezin, Vyacheslav Dokuchaev, Yury Eroshenko

TL;DR
This paper develops a theory for spherically symmetric thin shells in conformal gravity, comparing it with General Relativity, and finds unique properties and dynamics of shells in different gravitational frameworks.
Contribution
It introduces a comprehensive analysis of thin shells in conformal gravity, extending previous models in General Relativity and revealing novel shell behaviors.
Findings
Massless shells have arbitrary dynamics in conformal gravity.
Weyl+Einstein gravity restores shell trajectories without external solutions.
Shell properties differ significantly between theories.
Abstract
The spherically symmetric thin shells are the nearest generalizations of the point-like particles. Moreover, they serve as the simple sources of the gravitational fields both in General Relativity and much more complex quadratic gravity theories. We are interested in the special and physically important case when all the quadratic in curvature tensor (Riemann tensor) and its contractions (Ricci tensor and scalar curvature) terms are present in the form of the square of Weyl tensor. By definition, the energy-momentum tensor of the thin shell is proportional to Dirac delta-function. We constructed the theory of the spherically symmetric thin shells for three types of gravitational theories with the shell: (1) General Relativity; (2) Pure conformal (Weyl) gravity where the gravitational part of the total Lagrangian is just the square of the Weyl tensor; (3) Weyl+Einstein gravity. The…
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