General Relativistic Collapse of Accreting Neutron Stars with Rotation

Details General Relativistic Collapse of Accreting Neutron Stars with Rotation General Relativistic Collapse of Accreting Neutron Stars with Rotation

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pthph..70.1144n&link_type=abstract

Progress of Theoretical Physics, Vol. 70, No. 4, pp. 1144-1147

Physics

20

Scientific paper

Numerical calculations have been performed for the collapse of anaxially-symmetric rotating protoneutron star of mass 1.09 M&sun;with a rotating envelope of mass 0.81 M&sun;. 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.

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