IHEP OpenIR  > 硬X射线调制望远镜卫星
Testing the equation of state of neutron stars with electromagnetic observations
Degenaar, N.; Suleimanov, V. F.
2018
Source PublicationTest
Abstract

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.

Correlation关注
Research Direction综述
Member Type非核心团队
Language英语
ADS Bibcode2018arXiv180602833D
major scientific facilities硬X射线调制望远镜
Citation statistics
Cited Times:6 [ADS]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/282278
Collection硬X射线调制望远镜卫星
粒子天体物理中心
Recommended Citation
GB/T 7714
Degenaar, N.,Suleimanov, V. F.. Testing the equation of state of neutron stars with electromagnetic observations[J]. Test,2018.
APA Degenaar, N.,&Suleimanov, V. F..(2018).Testing the equation of state of neutron stars with electromagnetic observations.Test.
MLA Degenaar, N.,et al."Testing the equation of state of neutron stars with electromagnetic observations".Test (2018).
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62.pdf(3796KB)期刊论文出版稿限制开放CC BY-NC-SAApplication Full Text
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