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The lag and duration–luminosity relations of gamma-ray burst pulses

机译:伽马射线脉冲脉冲的滞后与持续时间-发光度关系

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Context. Relations linking the temporal or/and spectralproperties of the prompt emission of gamma-ray bursts (hereafter GRBs)to the absolute luminosity are of great importance as they bothconstrain the radiation mechanisms and represent potential distanceindicators. Here we discuss two such relations: the lag-luminosityrelation and the newly discovered duration-luminosity relation ofGRBpulses. Aims. We aim to extend our previous work on the origin ofspectral lags, using the duration-luminosity relation recentlydiscovered by Hakkila etal. (2008, ApJ, 677, L81) to connect lagsand luminosity. We also present a way to test this relation which hasoriginally been established with a limited sample of only12pulses. Methods. We relate lags to the spectral evolution and shape ofthe pulses with a linear expansion of the pulse properties aroundmaximum. We then couple this first result to the duration-luminosityrelation to obtain the lag-luminosity and lag-duration relations. Wefinally use a Monte-Carlo method to generate a population of syntheticGRBpulses which is then used to check the validity of theduration-luminosity relation. Results. Our theoretical results for the lag andduration-luminosity relations are in good agreement with the data. Theyare rather insensitive to the assumptions regarding the burst spectralparameters. Our MonteCarlo analysis of a population of syntheticpulses confirms that the duration-luminosity relation must be satisfiedto reproduce the observational duration-peak flux diagram of BATSE GRBpulses. Conclusions. The newly discovered duration-luminosity relationoffers the possibility to link all three quantities: lag, duration andluminosity of GRB pulses in a consistent way. Some evidence for itsvalidity have been presented but its origin is not easy to explain inthe context of the internal shock model. Key words: gamma-rays bursts: general - radiation mechanisms: non-thermal
机译:上下文。将伽马射线突发(以下简称GRB)的即时发射的时间或/和光谱特性与绝对光度联系起来的关系非常重要,因为它们既限制了辐射机制,又代表了潜在的距离指示符。在这里,我们讨论两个这样的关系:滞后-发光关系和新发现的GRBpulses的持续时间-发光关系。目的我们的目的是利用Hakkila等人最近发现的持续时间-光度关系来扩展先前关于谱滞的起源的工作。 (2008,ApJ,677,L81)连接滞后和亮度。我们还提出了一种测试这种关系的方法,该方法最初仅以12个脉冲的有限样本建立。方法。我们将滞后与脉冲的频谱演化和形状相关,脉冲特性在最大附近线性扩展。然后,我们将此第一个结果耦合到持续时间-亮度关系,以获得延迟-亮度和延迟-持续时间的关系。我们最终使用蒙特卡洛方法生成一组合成GRBpulses,然后将其用于检查持续时间-发光度关系的有效性。结果。我们的滞后和持续时间-光度关系的理论结果与数据非常吻合。它们对有关突发频谱参数的假设不敏感。我们对一组合成脉冲的蒙特卡洛分析证实,必须满足持续时间与光度的关系才能重现BATSE GRBpulss的观测持续时间峰值通量图。结论。新发现的持续时间-发光度关系提供了以统一的方式链接所有三个量的可能性:滞后,GRB脉冲的持续时间和发光度。已经提出了一些证明其有效性的证据,但在内部冲击模型的背景下很难解释其起源。关键词:伽马射线爆发:一般-辐射机理:非热

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