Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-29T17:53:07.803Z Has data issue: false hasContentIssue false
  • English
  • Français

Gravitational Radiation by a Collapsing Rotating Stellar Core

Published online by Cambridge University Press:  30 March 2016

Yu Yunqiang
Yu Yunqiang*
Affiliation:
Department of Physics, Peking University, Peking China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The reduction of the ratio between specific angular momentum and mass (a/m) due to gravitational radiation has been investigated for a model of collapsing rotating stellar core in a post-newtonian scheme. Results show that if the initial value of the ratio is significantly greater than one, it tends towards one and if the initial ratio is nearly one, no sharp reduction happens as the core collapses to the neutron star or black hole size.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 641 - 643
Copyright
Copyright © Reidel 1986

References

REFERENCES

1) Felice, F. de and Yunqiang, Yu, J. Phys. A15 3341 (1982).Google Scholar
2) Yunqiang, Yu, Ph.D Thesis in SISSA (Trieste) (1982) unpublished.Google Scholar
3) Yunqiang, Yu, Journal of Peking Observatory, 5 45 (1983).Google Scholar
4) Felice, F. de, Miller, J. and Yunqiang, Yu, SISSA preprint 39/84/A (1984); soon be published in Ap. J. (1985).Google Scholar
5) Thome, K., Rev. Mod. Phys. 52 299 (1980).Google Scholar