Pressureless disk cannot be the source for the Kerr metric-Reference-Cited by-同舟云学术

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Pressureless disk cannot be the source for the Kerr metric

Published:1976-03 Issue:13 Volume:15 Page:477-479
ISSN:1827-613X
Container-title:Lettere Al Nuovo Cimento Series 2
language:en
Short-container-title:Lett. Nuovo Cimento

Author:

Abramowicz M. A.,Arkuszewski W.,Muchotrzeb B.

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.1007/BF02725151.pdf

Reference2 articles.

1. B. Carter:Black-hole equilibrium states, inBlack Holes, edited byC. DeWitt andB. S. DeWitt (New York, N. Y., 1973).

2. J. M. Bardeen:Rapidity rotating stars, disks and black holes, inBlack Holes, edited byC. DeWitt andB. S. DeWitt (New York, N. Y., 1973).

Cited by 4 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

1. Gravitating discs around black holes;Classical and Quantum Gravity;2004-03-08

2. A toroidal source for the Kerr black hole geometry;Classical and Quantum Gravity;1991-05-05

3. A family of rotating disks as sources of the Kerr metric;General Relativity and Gravitation;1987-09

4. Ellipsoidal space-times, sources for the Kerr metric;Annals of Physics;1978-05

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