Related papers: Rigidly Rotating Strange Quark Star

This paper has been removed by arXiv administrators because it overlaps hep-th/0308070, and others. This paper also has excessive overlap with the following paper also written by the authors or their collaborators: gr-qc/0506061.

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This article has been withdrawn; see astro-ph/0611542

This paper has been withdrawn by the authors due to some technical problems in the paper.

This paper has been withdrawn due to an error. We plan to replace it with a corrected version.

This paper has been removed by arXiv administrators because it overlaps gr-qc/0303009, hep-th/0405047, gr-qc/0412120, and others. This paper also has excessive overlap with the following papers also written by the authors or their…

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This paper has been withdrawn by the author(s), due to technical copyright problems with the Royal Society of Chemistry.

This paper has been withdrawn by the authors, since it had been the excessive repetition of the part of hep-ph/0310190.

This paper has been withdrawn by the authors because it has been merged with paper arXiv:0903.3501v1 [math.DG]

This paper has been withdrawn by the author, due to an error in the proof of Theorem 3.8.

This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0011027, "Viscous cosmologies in scalar-tensor theories for Kasner type metrics," by M. Cataldo, S. del Campo and P. Salgado; Phys. Rev. D 41, 1086 (1990),…

This paper has been withdrawn by the author because eq.(4) and those subsequent are incorrect.

This paper has been withdrawn.

This paper has been withdrawn.

The reason, we need three terms of `strange', `bare', and `solid' before quark stars, is presented concisely though some fundamental issues are not certain. Observations favoring these stars are introduced.

This submission has been withdrawn by arXiv administrators because of inappropriate authorship claims.

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This paper has been withdrawn at the request of one of the authors.

This paper was withdrawn by the authors.