Implication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars

Jiarong Li; Miao Kang; Nana Pan; Shuhua Yang; Xiaoping Zheng; Xuewen Liu

REVIEW

Implication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0609011 v2 pith:NZJAFD5Y submitted 2006-09-01 astro-ph hep-phnucl-th

Implication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars

Xiaoping Zheng , Nana Pan , Shuhua Yang , Xuewen Liu , Miao Kang , Jiarong Li This is my paper

classification astro-ph hep-phnucl-th

keywords starshybridneutronexistencematterpulsarsquarksubmillisecond

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

We derive the bulk viscous damping timescale of hybrid stars, neutron stars with quark matter core. The r-mode instability windows of the stars show that the theoretical results are consistent with the rapid rotation pulsar data, which may give an indication for the existence of quark matter in the interior of neutron stars. Hybrid stars instead of neutron or strange stars may lead to submillisecond pulsars.

Implication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars

discussion (0)