摘要
The null infinity limit of the gravitational energy-momentum and energy flux determined by the covariant Hamiltonian quasilocal expressions is evaluated using the Newman-Penrose spin coefficients. The reference contribution is considered by three different embedding approaches. All of them give the expected Bondi energy and energy flux.
原文 | ???core.languages.en_GB??? |
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文章編號 | 124010 |
頁(從 - 到) | 1-11 |
頁數 | 11 |
期刊 | Physical Review D - Particles, Fields, Gravitation and Cosmology |
卷 | 71 |
發行號 | 12 |
DOIs | |
出版狀態 | 已出版 - 15 6月 2005 |