Related papers: Electromagnetic Pulsar Spindown

The article has been withdrawn by the author.

This paper has been withdrawn by the author due to imprecisions which must conduce to wrong results.

This paper has been withdrawn to allow publication elsewhere.

This paper has been withdrawn by the author due to the need for further revision.

This paper has been withdrawn by the author, due to necessity of revision.

The paper has been withdrawn by the author.

This paper has been withdrawn by the author.

This paper has been withdrawn by the authors as they feel it inappropriate to publish this paper for the time being.

This paper has been withdrawn by the author. The most updated version can be accessed by arXiv:1806.07290.

This paper has been withdrawn pending revision.

This paper has been withdraw by the author due to adding more modeling results.

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This paper has been withdrawn.

This paper has been withdrawn by the author due to a crucial sign error in some equations

This paper has been withdrawn by the authors.

This paper has been withdrawn.

This paper is withdrawn.

This paper has been withdrawn by the authors. Significantly revised versions of the results of this paper are now available in arXiv:0707.0487v2 and arXiv:0808.3169v1.

This paper has been withdrawn by the author.

The paper is withdrawn by the author, due to the fact that in Larsson's Phys.Lett. A256 (1999) 245-252 (quant-ph/9901074) a similar model was published with even higher efficiency.