Related papers: Electromagnetic Pulsar Spindown

This paper has been withdrawn by the authors. It has been superseded by hep-th/0309154

The paper has been withdrawn by the author.

This paper has been withdrawn by the author due to new results to be added.

This paper has been withdrawn by the authors.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 is due to the fact that it has been substantially revised. As a consequence title and aim of the contents

This paper has been withdrawn by the authors due to overlap with other papers.

This paper has been withdrawn

This paper has been withdrawn by the author due to an error

This paper has been withdrawn by the authors.

This paper has been withdrawn due to a copyright restrictions.

This paper has been withdrawn by the author due to some problems.

This paper has been withdrawn by the author, due to the fact that a similar paper (quant-ph/9904075) has been published.

This paper has been withdrawn

This paper has been withdrawn by the author. An assumption made in the analysis is not valid under the experimental conditions.

This paper has been withdrawn.

This paper has been withdrawn by the author.

This paper has been withdrawn. An extended version of this work can be found in E. Cappelluti, C. Grimaldi, L. Pietronero, S. Straessler: Phys. Rev. Lett. 85, 4771 (2000) [cond-mat/0105560] and E. Cappelluti, C. Grimaldi, L. Pietronero, S.…

This paper has been withdrawn.

This paper was withdrawn as it may have appeared elsewhere, although in a different form.

This paper has been withdrawn.

This paper has been withdrawn by the author. The spinor matrix element was incorrect, and orders of magnitude too big.