General Relativistic Collapse of Accreting Neutron Stars with Rotation
- 1 October 1983
- journal article
- Published by Oxford University Press (OUP) in Progress of Theoretical Physics
- Vol. 70 (4) , 1144-1147
- https://doi.org/10.1143/ptp.70.1144
Abstract
Numerical calculations have been performed for the collapse of an axially-symmetric rotating protoneutron star of mass 1.09 M⊙ with a rotating envelope of mass 0.81 M⊙. For q(≡total angular momentum / (M(GM/C2)C))≃1, it is found that depending on the rotation law a rapidly rotating spheroid, disk or ring-like shape neutron star is formed.Keywords
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