Is XTE J1739-285 a quark star masquerading as a neutron star TeX Export

@misc{citeulike:2205122, abstract = {The recent discovery of burst oscillation at 1122Hz in the X-ray transient XTE J1739-285 supports the suggestion that it contains a submillisecond pulsar\cite{1}. We here find for the first time the enormous dissipation effect in the transition boundary layer between quark matter core and hadron matter envelope. Just combining the estimation with previous dissipation mechanism together, we show that XTE J1739-285 can be uniquely restricted to a quark star masquerading as a neutron star (hybrid star) that contains a pure quark matter or mixed quark-hadron matter core from synthesizing both gravitational wave radiation (r-mode) instability and Keplerian motion constraints at 1122Hz lever. Such constraints allow the radii in the range \$9{\rm km}\leq R\leq 12{\rm km}\$ and the masses in the range \$1.2M\_\odot\leq M\leq 2.0M\_\odot\$. The normal neutron stars, hyperon stars and strange stars within the mass-radius limits are excluded.}, archivePrefix = {arXiv}, author = {Xiaoping, Zheng and Nana, Pan and Li, Zhang}, citeulike-article-id = {2205122}, citeulike-linkout-0 = {http://arxiv.org/abs/0712.4310}, citeulike-linkout-1 = {http://arxiv.org/pdf/0712.4310}, day = {28}, eprint = {0712.4310}, keywords = {1122hz, quark}, month = {Dec}, posted-at = {2008-01-07 21:47:44}, priority = {2}, title = {Is XTE J1739-285 a quark star masquerading as a neutron star}, url = {http://arxiv.org/abs/0712.4310}, year = {2007} }

TY - ELEC ID - citeulike:2205122 L3 - citeulike-article-id:2205122 N2 - The recent discovery of burst oscillation at 1122Hz in the X-ray transient XTE J1739-285 supports the suggestion that it contains a submillisecond pulsar\cite{1}. We here find for the first time the enormous dissipation effect in the transition boundary layer between quark matter core and hadron matter envelope. Just combining the estimation with previous dissipation mechanism together, we show that XTE J1739-285 can be uniquely restricted to a quark star masquerading as a neutron star (hybrid star) that contains a pure quark matter or mixed quark-hadron matter core from synthesizing both gravitational wave radiation (r-mode) instability and Keplerian motion constraints at 1122Hz lever. Such constraints allow the radii in the range $9{\rm km}\leq R\leq 12{\rm km}$ and the masses in the range $1.2M_\odot\leq M\leq 2.0M_\odot$. The normal neutron stars, hyperon stars and strange stars within the mass-radius limits are excluded. TI - Is XTE J1739-285 a quark star masquerading as a neutron star KW - 1122hz KW - quark AU - Xiaoping, Zheng AU - Nana, Pan AU - Li, Zhang PY - 2007/Dec/28/ UR - http://arxiv.org/abs/0712.4310 ER -