C-metric in a (nut)shell
Cameron R D Bunney, Robert B Mann

TL;DR
This paper explores the 2+1 dimensional C-metric by embedding it within shells of stress energy, analyzing their shapes, energy conditions, and resulting solutions for accelerating particles and black holes in AdS space.
Contribution
It introduces a detailed construction of the 2+1 C-metric with shells, classifies solutions based on energy conditions, and finds new Einstein solutions involving finite strings and struts.
Findings
Shell shapes are cuspoidal or teardrop-shaped.
Stress energy respects energy conditions for accelerating particles.
New solutions include black holes pulled or pushed by finite strings or struts.
Abstract
We present a comprehensive study of the C-metric in dimensions, placing it within a shell of stress energy and matching it to an exterior vacuum AdS metric. The C-metric is not circularly symmetric and hence neither are the constructed shells, which instead take on a cuspoidal or teardrop shape. We interpret the stress energy of the shells as a perfect fluid, calculating the energy density and pressure. For accelerating particles (Class I), we find the stress energy is concentrated on the part of shell farthest from the direction of acceleration and always respects the strong and weak energy conditions. For accelerating black holes (Class I, II, and III), the shell stress energy may either respect or violate the energy conditions depending on the parameter of the exterior metric -- between the two regimes lies a critical value of the external parameter for…
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Taxonomy
TopicsAlgebraic and Geometric Analysis
