Related papers: Mitigating radiation loads in Nb3Sn quadrupoles fo…

This paper has been withdrawn by the author.

This paper has been withdrawn by the author due to new results to be added.

This paper has been withdrawn by the author.

This paper has been withdrawn by the authors due to some technical problems in the paper.

This paper has been withdrawn by the authors due to substantial changes.

This paper has been withdrawn.

This paper has been withdrawn by the author.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This paper has been withdrawn.

This paper has been withdrawn due to disagreement of suggested results and methods between authors.

This paper has been withdrawn by the author(s).

This paper has been withdrawn by the authors as they feel it inappropriate to publish this paper for the time being.

This paper has been withdrawn by the author, due to errors in the figures.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the authors due to overlap with other papers.

This paper has been withdrawn by the authors because the authors excluded the paper from electronic proceedings of the conference.

This paper has been withdrawn.

This paper has been temprally withdrawn by the author

This paper has been withdrawn by the authors, since it had been the excessive repetition of the part of hep-ph/0310190.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the author(s), due a crucial error in the data.