Abstract
We compute the limiting behaviour of an energy integral proposed by Hawking. In the presence of matter, we find that the leading-order contribution to this integral is just the energy density of the matter. In the absence of matter, the leading-order contribution is the (time component of the) Bel-Robinson tensor.
Reference14 articles.
1. C.r.hebd;Bel L.;Seanc. Acad. Sci. Paris,1958
2. Eardley D. 1979 In Sources of gravitational radiation (ed. L. Smarr). Cambridge U niversity Press.
3. ENERGY EXTRACTION
4. Geroch R. 1977 In Asymptotic structure of space-time (ed. F. P. Esposito and L. W itten). New York London: Plenum .
5. J . math;Hawking S. W.;Phys.,1968
Cited by
56 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献