Self-gravitating field configurations: The role of the energy-momentum trace

Abstract

Static spherically-symmetric matter distributions whose energy-momentum tensor is characterized by a non-negative trace are studied analytically within the framework of general relativity. We prove that such field configurations are necessarily highly relativistic objects. In particular, for matter fields with $T\ge \alpha \cdot \rho \ge 0$ (here $T$ and $\rho$ are respectively the trace of the energy-momentum tensor and the energy density of the fields, and $\alpha$ is a non-negative constant), we obtain the lower bound ${\text{max}}_r\{2m(r)/r\}>(2+2\alpha )/(3+2\alpha )$ on the compactness (mass-to-radius ratio) of regular field configurations. In addition, we prove that these compact objects necessarily possess (at least) {\it two} photon-spheres, one of which exhibits {\it stable} trapping of null geodesics. The presence of stable photon-spheres in the corresponding curved spacetimes indicates that these compact objects may be nonlinearly unstable. We therefore conjecture that a negative trace of the energy-momentum tensor is a {\it necessary} condition for the existence of stable, soliton-like (regular) field configurations in general relativity.

11 pages

References in corpus (3)

• Upper bound on the radii of black-hole photonspheres
• Einstein-Yang-Mills Solitons: The Role of Gravity
• Bounds on the mass-to-radius ratio for non-compact field configurations

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