A note on solid pulsars
| dc.creator | Xu, R. X. | |
| dc.date | 2004-03-11 | |
| dc.date.accessioned | 2026-07-07T02:12:36Z | |
| dc.date.available | 2026-07-07T02:12:36Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0403280 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0403280 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7507 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A note on solid pulsars | |
| dc.type | text |