Related papers: Rigidly Rotating Strange Quark Star

This paper has been withdrawn by the author because the conclusions reached in it are incorrect.

Withdrawn by arXiv administration because authors have forged affiliations and acknowledgements, and have not adequately responded to charges [hep-th/9912039] of unattributed use of verbatim material.

Withdrawn; paper superceded by astro-ph/0105392

The paper was removed.

This paper has been withdrawn by the authors.

This paper has been administratively withdrawn by arXiv, duplicate of arXiv:1008.2691.

The paper has been withdrawn by the authors for modification.

This paper has been withdrawn by the author because there are some typos in proofs.

This paper has been withdrawn by the author because similar published work on the topic was overlooked. See S. Deser and A. Waldron, Nucl. Phys. B 631, 369-387 (2002).

This paper has been withdrawn by the authors.

This paper has been withdrawn by the authors, because of serious experimental problems.

Withdrawn; originally put in incomplete form without permission

This paper has been withdrawn by the authors due to an unlikely results.

This paper was withdrawn by the author.

This paper has been withdrawn by the author due to inconsistency of the considered working hypothesis.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This paper has been withdrawn by the authors due to a crucial error in equation 12.

This paper has been retracted.

This paper has been withdrawn by the author due to a new work in [arXiv:0901.0456v4] which can contain the results in this paper.

This paper is withdrawn due to some errors, which are corrected in arXiv:0912.0071v4 [cs.LG].

This paper has been withdrawn by the author(s),