Related papers: Electromagnetic Pulsar Spindown
This paper has been withdrawn by the author due to the appearence of enlarged version with one new author name more (hep-ph/0012293).
This paper has been withdrawn by the author.
This paper has been withdrawn by the author due to the paper does not belong to Condensed Matter field.
The paper has been withdrawn because a new, substantially revised version of the theory of neutron star radiation is completed by the author.
This paper has been withdrawn. A significantly revised version will be posted in the near future.
This paper has been withdrawn Abstract: This paper has been withdrawn by the author due to the publication.
This paper has been withdrawn by the author.
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This paper has been withdrawn by the author
This paper is being withdrawn.
A modified version of this paper is under process and with a new title and abstract. Hence, this version of the article is completely withdrawn.
Manuscript withdrawn by the authors.
This paper has been withdrawn by the authors to avoid redundancy with e-print hep-ph0507031.
This paper has been withdrawn by the author.
This paper has been withdrawn because the models on which it was based have undergone significant changes and improvements.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…
Concluding Remarks of the 270.WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants.
This paper has been withdrawn.
This paper has been withdrawn by the author.
This manuscript has been withdrawn by the author. Some of the material has been included in the manuscript 'Embedded Monopoles' at hep-th/0106254.
This paper has been withdrawn.