Quasilocal energy conditions

Details Quasilocal energy conditions Quasilocal energy conditions

1994-03-18

arxiv.org/abs/gr-qc/9403039v1

Phys.Rev. D52 (1995) 2001-2006

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

19 pages LaTeX, report number Alberta Thy 11-94

Scientific paper

10.1103/PhysRevD.52.2001

The classical value of the Hamiltonian for a system with timelike boundary has been interpreted as a quasilocal energy. This quasilocal energy is not positive definite. However, we derive a `quasilocal dominant energy condition' which is the natural consequence of the local dominant energy condition. We discuss some implications of this quasilocal energy condition. In particular, we find that it implies a `quasilocal weak energy condition'.

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