摘要
Early energy-momentum investigations for gravitating systems gave reference-frame-dependent pseudotensors; later the quasilocal idea was developed. Quasilocal energy-momentum can be determined by the Hamiltonian boundary term, which also identifies the variables to be held fixed on the boundary. We show that a pseudotensor corresponds to a Hamiltonian boundary term. Hence, they are quasilocal and acceptable; each is the energy-momentum density for a definite physical situation with certain boundary conditions. These conditions are identified for well-known pseudotensors.
原文 | ???core.languages.en_GB??? |
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頁(從 - 到) | 1897-1901 |
頁數 | 5 |
期刊 | Physical Review Letters |
卷 | 83 |
發行號 | 10 |
DOIs | |
出版狀態 | 已出版 - 1999 |