Quakes in solid quark stars | |
Zhou, AZ; Xu, RX; Wu, XJ; Wang, N | |
刊名 | ASTROPARTICLE PHYSICS |
2004-10-01 | |
卷号 | 22期号:1页码:73-79 |
关键词 | pulsars neutron stars elementary particles |
ISSN号 | 0927-6505 |
通讯作者 | rxxu@bac.pku.edu.cn |
英文摘要 | A starquake mechanism for pulsar glitches is developed in the solid quark star model. It is found that the general glitch natures (i.e., the glitch amplitudes and the time intervals) could be reproduced if solid quark matter, with high baryon density but low temperature, has properties of shear modulus mu(c) = 10(30-34) erg/cm(3) and critical stress sigma(c) = 10(18similar to24) erg/cm(3). The post-glitch behavior may represent a kind of damped oscillations. (C) 2004 Elsevier B.V. All rights reserved. |
学科主题 | 致密天体、高能和基础物理 |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics ; Physics, Particles & Fields |
研究领域[WOS] | Astronomy & Astrophysics ; Physics |
关键词[WOS] | STRANGE STARS ; NEUTRON-STARS ; FREE PRECESSION ; PULSAR ; MATTER ; DENSITY ; DROPLETS ; MODEL ; QCD |
收录类别 | SCI |
资助信息 | National Nature Sciences Foundation of China (10273001);Special Funds for Major State Basic Research Projects of China (G2000077602) |
语种 | 英语 |
WOS记录号 | WOS:000224490500006 |
公开日期 | 2013-03-06 |
内容类型 | 期刊论文 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/117] |
专题 | 脉冲星研究团组 新疆天文台_射电天文研究室 新疆天文台_其它 |
作者单位 | 1.Peking Univ, Sch Phys, Beijing 100871, Peoples R China 2.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Urumqi Stn, Urumqi 830011, Peoples R China |
推荐引用方式 GB/T 7714 | Zhou, AZ,Xu, RX,Wu, XJ,et al. Quakes in solid quark stars[J]. ASTROPARTICLE PHYSICS,2004,22(1):73-79. |
APA | Zhou, AZ,Xu, RX,Wu, XJ,&Wang, N.(2004).Quakes in solid quark stars.ASTROPARTICLE PHYSICS,22(1),73-79. |
MLA | Zhou, AZ,et al."Quakes in solid quark stars".ASTROPARTICLE PHYSICS 22.1(2004):73-79. |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论