Interior Matter Estimates of Rapidly Rotating Compact Stars
High Energy Astrophysical Phenomena
2010-05-12 v1 Solar and Stellar Astrophysics
Abstract
The authors try to probe the inner components of rapidly rotating compact stars such as the millisecond pulsar SAX J1808.4-3658 and the possible sub-millisecond pulsar XTE J1739-285 in their own way by comparing the genuine rotation frequencies under different theoretical models with the observational data, which may exert more stringent constraint on matter composition of compact stars. According to their treatment, the SAX J1808.4-3658 is a star with exotic matter and XTE J1739-285 a hybrid star.
Cite
@article{arxiv.1005.1864,
title = {Interior Matter Estimates of Rapidly Rotating Compact Stars},
author = {Na-na Pan and Xiao-ping Zheng},
journal= {arXiv preprint arXiv:1005.1864},
year = {2010}
}
Comments
4 pages, 2 figures. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at Peking University, Beijing - P. R. China [http://vega.bac.pku.edu.cn/rxxu/csqcd.htm]