Boundary sources in the Doran - Lobo - Crawford spacetime

Details Boundary sources in the Doran - Lobo - Crawford spacetime Boundary sources in the Doran - Lobo - Crawford spacetime

2007-03-19

arxiv.org/abs/hep-th/0703168v2

Cent. Eur. J. Phys. 6(1), 317 - 320 (2008)

Physics

High Energy Physics

High Energy Physics - Theory

4 pages, title changed, no figures, minor text changes

Scientific paper

10.2478/s11534-008-0010-8

We take a null hypersurface (the causal horizon) generated by a congruence of null geodesics as the boundary of the Doran-Lobo-Crawford spacetime, to be the place where the Brown-York quasilocal energy is located. The components of the outer and inner stress tensors are computed and shown to depend on time and on the impact parameter $b$ of the test particle trajectory. The surface energy density $\sigma$ on the boundary is given by the same expression as that obtained previously for the energy stored on a Rindler horizon.

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