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A universal scaling for short and long gamma-ray bursts: E_{X,iso}-E_{gamma,iso}-E_{pk}

机译:短距离和长距离伽马射线爆发的通用缩放:   E_ {X,IsO} {-E_伽马,异} {-E_ pK}

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摘要

The comprehensive statistical analysis of Swift X-ray light-curves,collecting data from six years of operation, revealed the existence of auniversal scaling among the isotropic energy emitted in the rest frame 10-10^4keV energy band during the prompt emission (E_{gamma,iso}), the peak of theprompt emission energy spectrum (E_{pk}), and the X-ray energy emitted in the0.3-10 keV observed energy band (E_{X,iso}). In this paper we show that thisthree-parameter correlation is robust and does not depend on our definition ofE_{X,iso}. It is shared by long, short, and low-energetic GRBs, differentlyfrom the well-known E_{gamma,iso}-E_{pk} correlation. We speculate that theultimate physical property that regulates the GRB properties is the outflowLorentz factor.
机译:对Swift X射线光曲线进行的全面统计分析(收集了六年的运行数据)显示,在瞬态发射期间,静止帧10-10 ^ 4keV的能带中发射的各向同性能量之间存在普遍缩放关系(E_ { γ,iso},即时发射能谱的峰(E_ {pk})和在0.3-10 keV观测能带(E_ {X,iso})中发射的X射线能量。在本文中,我们证明了这种三参数相关性是鲁棒的,并且不依赖于我们对E_ {X,iso}的定义。它与长,短和低能量的GRB共享,这与众所周知的E_ {gamma,iso} -E_ {pk}相关性不同。我们推测调节GRB特性的最终物理特性是流出Lorentz因子。

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