Related papers: Second-order perturbation theory for the parametri…

This paper was withdrawn by arXiv administrators upon request of the Chairperson and Spokesperson of the L3 Collaboration.

This paper has been withdrawn by the author because it has been substantially modified.

This paper has been withdrawn by the author due to a crucial error in the formulation.

This paper has been withdrawn by the author because the conclusions reached in it are incorrect.

This paper has been withdrawn by the author due to similarity to the author's other paper

This paper has been withdrawn by the author. A much more revised version is available as arXiv:0909.4238.

The original version of this paper has been withdrawn by the authors and merged with the revised version of astro-ph/9702014.

This paper has been withdrawn by the author due to time-consuming revision.

Withdrawn by the authors

This paper has been withdrawn by the author because of copyright reasons.

This paper is withdrawn.

This paper has been withdrawn by the author due to a coming paper completely superseding it.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the author due to serious flaws in certain proofs. For instance, the method used to construct certain automorphic representations is flawed.

This paper has been withdrawn by the author.

This paper has been withdrawn by the authors.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This paper has been withdrawn by the authors due to a gap in the proof of the main result (in 5.3).

This paper was withdrawn because subsequent measurements produced results not always consistent with the ones presented in the paper.

This paper has been withdrawn by the author.

The paper has been withdrawn by the author.