Related papers: Pentaquark masses: another look

This paper has been withdrawn by the author due to a crucial error in the submission action.

This paper has been withdrawn.

This paper has been withdrawn by the authors due to an error.

This paper has been withdrawn by the authors, and instead we have replaced hep-ph/9807214 by this new version.

The paper has been withdrawn by authors.

This paper has been withdrawn by the authors.

This paper has been withdrawn by the author because the conclusions reached in it are incorrect.

This paper has been withdrawn by the author due to imprecisions which must conduce to wrong results.

This paper has been withdrawn by the author [arXiv admin].

This paper has been withdrawn by the author. A revised and expanded version is gr-qc/9907028 (Phys.Rev. D60 (1999) 104043).

The paper has been withdrawn by the author.

This paper has been withdrawn.

This paper has been withdrawn by the author due to a new work in [arXiv:0901.0456v4] which can contain the results in this paper.

This paper has been withdrawn by the author due to an error in the proof.

This paper has been withdrawn by the author.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This paper was withdrawn as it may have appeared elsewhere, although in a different form.

This paper has been withdrawn by the authors. A substantially altered paper will be submitted incorporating major corrections, additions and improvements.

This paper has been withdrawn by the author due to a crucial errors.

This paper has been withdrawn: it has been merged with the preprint to which it refers.

This paper has been withdrawn by the authors. Because of a misunderstanding, the paper was submitted prematurely to the arXiv. A replacement will follow.