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This paper has been withdrawn by the author due to inconsistency of the considered working hypothesis. The consistent treatment is presented in the last publications of the author.

This paper has been withdrawn by the author because of publication in the journal Earth and Planetary Science Letters (Elsevier), which does not permit preprints at arxiv.org

This paper has been withdrawn by the author due to the appearence of enlarged version with one new author name more (hep-ph/0012293).

This paper has been withdrawn by the author. It will be posted on astro-ph once the proceedings of the 363rd Heraeus Seminar on Neutron Stars and Pulsars are ready.

This paper has been withdrawn by the author.

This paper has been withdrawn due to copyright reasons.

This paper has been withdrawn by the author(s),

This paper has been withdrawn by the author.

This paper has been withdrawn by the author.

This paper has been withdrawn by the author due to similarity to the author's other paper

This paper has been withdrawn by the author(s), due to double submission. You can find it under: physics/0208019

This paper has been withdrawn by the author due to inconsistency of the considered working hypothesis. The consistent treatment is presented in the last publications of the author.

This paper has been withdrawn by the author.

This paper has been withdrawn by the author due to new results to be added.

This paper has been withdrawn by the author.

This paper has been withdrawn by the author due to new results to be added.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the author(s), due to a crucial error in eq. 6.

This paper has been withdrawn because the content has been substantially improved in a later paper, arXiv:0806.1165.

This paper has been withdrawn by the author.