:An unexpected X-ray transient favors very stiff neutron-star matter论文

:An unexpected X-ray transient favors very stiff neutron-star matter论文

本文主要研究内容

作者(2019)在《An unexpected X-ray transient favors very stiff neutron-star matter》一文中研究指出:Short-duration gamma-ray bursts (SGRBs) are mysterious gamma-ray flashes with durations less than two seconds, which occur at the cosmological distances. Some of them usually not only have very tenuous medium gases and old host galaxies but also are in the outskirts of the galaxies, suggesting an origin of binary neutron star (NS) mergers [1]. This origin was confirmed undoubtedly

Abstract

Short-duration gamma-ray bursts (SGRBs) are mysterious gamma-ray flashes with durations less than two seconds, which occur at the cosmological distances. Some of them usually not only have very tenuous medium gases and old host galaxies but also are in the outskirts of the galaxies, suggesting an origin of binary neutron star (NS) mergers [1]. This origin was confirmed undoubtedly

论文参考文献

  • [1].The effects of strong magnetic fields on neutron star structure:lowest order constrained variational calculations[J]. Gholam Hossein Bordbar,Zeinab Rezaei.  Research in Astronomy and Astrophysics.2013(02)
  • [2].3PF2 neutron superfluidity in neutron stars and three-body force effect[J]. 崔常喜,左维,H.J.Schulze.  Chinese Physics B.2008(09)
  • [3].Electrically charged: An effective mechanism for soft EOS supporting massive neutron star[J]. JING ZhenZhen,WEN DeHua,ZHANG XiangDong.  Science China(Physics,Mechanics & Astronomy).2015(10)
  • [4].Asymmetric neutron stars in the presence of vacuum fluctuations[J]. Hong-Hui Guan,Chen Wu,Ji-Feng Yang.  Nuclear Science and Techniques.2016(01)
  • [5].Predicting neutron star spins from twin kHz QPOs[J]. SHI ChangSheng Department of Astronomy,Nanjing University,Nanjing 210093,China;College of Material Science and Chemical Engineering,Hainan University,Hainan 570228,China.  Science China(Physics,Mechanics & Astronomy).2010(S1)
  • [6].Microscopic calculation of the magnetic field of neutron stars[J]. 刘军,贾文志,王顺金.  中国物理C.2009(09)
  • [7].The Origin of Glitches in Pulsars—Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars[J]. Qiu-He Peng, Zhi-Quan Luo and Chih-Kang Chou School of Physics and Electronic Information, China West Normal University, Nanchong 637002 Department of Astronomy, Nanjing University, Nanjing 210093; Department of Physics, Sichuan University, Chengdu 610065National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012.  Chinese Journal of Astronomy and Astrophysics.2006(03)
  • [8].Profile of the composition fractions in neutron stars[J]. LI Wenfei, ZHANG Fengshou & CHEN LiewenCenter of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000, China;Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China;Department of Physics, Shangh.  Chinese Science Bulletin.2002(08)
  • [9].Transition density of the large mass hyperon star[J]. 赵先锋,贾焕玉.  Chinese Physics C.2014(01)
  • [10].Effects of σ* and Φ mesons on the surface redshift of a neutron star[J]. 赵先锋.  Chinese Physics B.2011(03)
  • 论文详细介绍

    论文作者分别是来自Science Bulletin的,发表于刊物Science Bulletin2019年20期论文,是一篇关于,Science Bulletin2019年20期论文的文章。本文可供学术参考使用,各位学者可以免费参考阅读下载,文章观点不代表本站观点,资料来自Science Bulletin2019年20期论文网站,若本站收录的文献无意侵犯了您的著作版权,请联系我们删除。

    标签:;  

    :An unexpected X-ray transient favors very stiff neutron-star matter论文
    下载Doc文档

    猜你喜欢