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??? |
|---|---|
| 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 |
指紋
深入研究「Quasilocal energy-momentum and energy flux at null infinity」主題。共同形成了獨特的指紋。引用此
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