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A new three-parameter correlation for gamma-ray bursts with a plateau phase in the afterglow

机译:具有平台的伽马射线爆发的新三参数相关   在余辉的阶段

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摘要

Gamma ray bursts (GRBs) have great advantages for their huge burst energies,luminosities and high redshifts in probing the Universe. A few interestingluminosity correlations of GRBs have been used to test cosmology models.Especially, for a subsample of long GRBs with known redshifts and a plateauphase in the afterglow, a correlation between the end time of the plateau phase(in the GRB rest frame) and the corresponding X-ray luminosity has been found.In this paper, we re-analyze the subsample and found that a significantlytighter correlation exists when we add a third parameter, i.e. the isotropic$\gamma$-ray energy release, into the consideration. Additionally, both longand intermediate duration GRBs are consistent with the same three-parametercorrelation equation. It is argued that the new three-parameter correlation isconsistent with the hypothesis that the subsample of GRBs with a plateau phasein the afterglow be associated with the birth of rapidly rotating magnetars,and that the plateau be due to the continuous energy-injection from themagnetar. It is suggested that the newly born millisecond magnetars associatedwith GRBs might provide a good standard candle in the Universe.
机译:伽玛射线爆发(GRB)具有巨大的优势,因为它们探测宇宙的巨大爆发能量,发光度和高红移。 GRB的一些有趣的光度相关性已被用于测试宇宙学模型,特别是对于已知红移的长GRB子样本和余辉中的平稳期,平稳阶段的结束时间(在GRB静止帧中)和在本文中,我们对子样本进行了重新分析,发现当我们考虑第三个参数,即各向同性的\γ射线能量释放时​​,存在显着更紧密的相关性。另外,长持续时间和中间持续时间GRB都与相同的三参数相关方程一致。有人认为,新的三参数相关性与以下假设相吻合:在余辉中具有平稳阶段的GRBs子样本与快速旋转的磁星的诞生有关,而该平稳阶段是由于它们不断地注入能量所致。建议与GRB关联的新生毫秒磁星可能为宇宙提供良好的标准蜡烛。

著录项

  • 作者

    Xu, M.; Huang, Y. F.;

  • 作者单位
  • 年度 2011
  • 总页数
  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
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