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2003-10-20
On the angular momentum of the neutron star
Zakir F. Seidov
文献摘要
It is shown that the mass loss due to rotation-driven hydrodynamical instability during the catastrophic collapse of the star is small. Neutron star is formed with a large rotational kinetic energy and the spin-down takes place in the following life of neutron star as a pulsar.
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