2004/03/11 by R. X. Xu, Renxin Xu, Xu, R. X.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Pulsars and Gravitational Waves Research #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0403280
3 pages, no figure. Proceedings of CAS Symposium No.365/The 18th Guo Shoujing Summer School on Astrophysics: "Beyond the Milky Way: Progress in Extragalactic X-Ray Astronomy with Chandra and XMM-Newton" (September 21-24, 2003), Eds: Fuzhen Cheng, Junhan You, and K. Makishima
arxiv created 2004/03/11 · openalex publication_date 2004/03/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
After a brief introduction to the necessary of quark stars in modelling pulsars, I present a qualitative analysis of the solidification of quark matter with low-temperature but high-density. The reason, that a solid neutron star could not be possible, is also given.