Related papers: Pulsar dynamics: magnetic dipole model revisited
This paper has been withdrawn by the author because of copyright reasons.
This paper has been withdrawn.
This paper has been withdrawn by the authors for adding some results.
%auto-ignore Paper has been withdrawn by the author.
This paper has been withdrawn.
This paper has been withdrawn by the authors as they feel it inappropriate to publish this paper for the time being.
This paper has been withdrawn
This paper has been withdrawn by the authors in order to replace it with a more correct treatment. The basic results remain the same but the treatment is more rigorously correct.
This paper has been withdrawn by the author because overcame by arXiv:0910.4694
This paper has been withdrawn because the models on which it was based have undergone significant changes and improvements. A new paper with the same title, based on the improved models, is accepted for publication in MNRAS and is available…
This paper has been withdrawn by the author.
This submission has been withdrawn by arXiv administrators because it is a duplicate of 0705.0667.
Major mistake. The paper has been withdrawn.
The paper has been withdrawn.
The paper has been withdrawn.
This paper has been withdrawn by the authors.
This paper has been withdrawn by the authors.
This paper has been withdrawn by the authors, due a oversimplified decoherence model. It will be substituted by a new work.
This paper has been withdrawn by the author.
This paper has been withdrawn by the author.