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PULSAR DRIFT AND ROTATIONAL COLLAPSE |
| Asghar Qadir*;M. Rafique;A.W. Siddiqui* |
| *Mathematics Department, Quaid-i-Azam University, Islamabad, Pakistan.
Pakistan Military Academy, Kakul, Pakistan.
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| Cite this article: |
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Asghar Qadir, M. Rafique, A.W. Siddiqui 1987 Chin. Phys. Lett. 4 177-180 |
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Abstract The relativistic explanation of pulsar drift is based on an extremely simplistic model. The collapsing star is treated as composed of a collection of particles falling radially inwards. A calculation incorporating a finite angular momentum is found to give reasonable drift velocities provided the initial pulsar frequency is sufficiently high. The values required are not unreasonable.
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Published: 01 April 1987
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