Related papers: Rigidly Rotating Strange Quark Star
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This paper has been withdrawn by the author due to a crucial sign error in equation 1
This paper has been withdrawn by the author due to extremely unscientific errors.
This paper has been withdrawn by the author due to the presented idea is wrong.
This paper has been withdrawn temporarily.
The paper has been withdrawn by change of content and some errors in the examples.
Recently there is a suggestion about the star RXJ1856.5$-$3754, being a possible candidate for quark star. While from the estimates of the radiation radius, given by the authors, it does not seem to fit with any of the known models for such…
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0010068. This paper has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0607109, gr-qc/0607126,…
This paper has been withdrawn by the authors. Significantly revised versions of the results of this paper are now available in arXiv:0707.0487v2 and arXiv:0808.3169v1.
This paper has been withdrawn by the author.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This paper has been withdrawn because of serious errors.
This paper has been withdrawn by the authors due to overlap with other papers.
This version withdrawn by arXiv administrators because the submitter did not have the right to agree to our license at the time of submission.
This paper has been withdrawn because it overlaps with arXiv:1203.6583
This paper was withdrawn by arXiv admin due to authors' misrepresentation of identity/affiliation.
This paper has been withdrawn by the author, due to the insecurity against attacks received in quant-ph/0605027v5.
This paper has been removed by arXiv administrators because of overlap with gr-qc/0303034. This paper also has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0601133, gr-qc/0602012,…
This paper has been withdrawn by the authors due to the paper is far from complishment.
This paper has been withdrawn owing a re-arrangement of two previously submitted papers. The new version of the theoretical work on the triaxial shape of dark matter haloes can be found at the ArXiv astro-ph list (CO) as article 1104.2905
This paper has been withdrawn.