Testing the equation of state of neutron stars with electromagnetic observations
文献类型：期刊论文
| 作者 | Degenaar, N.; Suleimanov, V. F. |
| 出版日期 | 2018 |
| 英文摘要 | Neutron stars are the densest, directly observable stellar objects in the universe and serve as unique astrophysical laboratories to study the behavior of matter under extreme physical conditions. This book chapter is devoted to describing how electromagnetic observations, particularly at X-ray, optical and radio wavelengths, can be used to measure the mass and radius of neutron stars and how this leads to constraints on the equation of state of ultra-dense matter. Having accurate theoretical models to describe the astrophysical data is essential in this effort. We will review different methods to constrain neutron star masses and radii, discuss the main observational results and theoretical developments achieved over the past decade, and provide an outlook of how further progress can be made with new and upcoming ground-based and space-based observatories. |
| 语种 | 英语 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/282278]  |
| 专题 | 硬X射线调制望远镜卫星 高能物理研究所_粒子天体物理中心 |
| 推荐引用方式 GB/T 7714 | Degenaar, N.,Suleimanov, V. F.. Testing the equation of state of neutron stars with electromagnetic observations[J],2018. |
| APA | Degenaar, N.,&Suleimanov, V. F..(2018).Testing the equation of state of neutron stars with electromagnetic observations.. |
| MLA | Degenaar, N.,et al."Testing the equation of state of neutron stars with electromagnetic observations".(2018). |
入库方式： OAI收割
来源：高能物理研究所
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