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This paper is withdrawn because its results have been previously reported in arxiv hep-th/0507200.
This paper has been withdrawn by the author since it has been accepted for publishing in J. Geophys. Res. Please contact the American Geophysical Union for the refereed article.
This paper has been withdrawn by the author to comply with the journal policy to which it has been submitted.
This paper has been withdrawn because of the requirement from the journal where the modified version of the paper is to be published.
This paper has been withdrawn by the author. This draft is withdrawn for its poor quality in english, unfortunately produced by the author when he was just starting his science route. Look at the ICML version instead:…
This paper has been withdrawn by the author: it was a too preliminary version.
This paper has been withdrawn by the author.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This paper has been withdrawn by the author, due to a significant error in section 4.3.1.
This paper has been withdrawn by the author.
This paper has been withdrawn by the author, due an error in the proof of Proposion 2.13.
This paper has been withdrawn.
This paper has been withdrawn by the authors, due to issues concerning the use of unpublished experimental data.
This paper has been withdrawn by the author because the conclusions reached in it are incorrect.
This paper has been withdrawn.
This paper has been withdrawn due to a crucial theoretical and experimental error.
The paper has been withdrawn because a new, substantially revised version of the theory of neutron star radiation is completed by the author.
This paper has been withdrawn.
This paper has been withdrawn due to non-clearness of some technical points, as well as lack of a reasonable statement of quantization conjecture.
This paper has been withdrawn by the author.
This paper has been withdrawn by the author.