{"title":"Unified Theory of Negative and Positive Spectral Lags in the Gamma-Ray Burst Prompt Phase due to Shear Comptonization from a Structured Jet","authors":"Mukesh Kumar Vyas, Asaf Pe’er and Shabnam Iyyani","doi":"10.3847/2041-8213/ad887c","DOIUrl":null,"url":null,"abstract":"Positive spectral lags are commonly observed in gamma-ray burst (GRB) prompt phase where soft photons lag behind hard ones in their spectral studies. In contrast to this pattern, a fraction of GRBs show a negative spectral lag where hard photons arrive later compared to soft photons. Similarly, recent Fermi-Large Area Telescope observations show a late onset of high-energy photons in most GRB observations. A fraction of GRBs show a transition from positive to negative lags. Such negative lags and the spectral lag transition have no convincing explanation. We show that a structured GRB jet with velocity shear naturally produces both positive and negative spectral lags. The high-energy photons gain energy from repeated scattering with shearing layers and subsequently escape from higher altitudes. Hence, these photons are delayed compared to soft photons producing a negative spectral lag. The inner jet has no shear, and a positive lag appears to provide a unified picture of spectral lags in GRBs. The theory predicts a flip in spectral lag from positive to negative within the evolution of the prompt phase. Comparison of the observed lags with the prediction of the theory limits the possible range of GRB jet Lorentz factors to a few tens.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"6 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-11-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Astrophysical Journal Letters","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3847/2041-8213/ad887c","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Positive spectral lags are commonly observed in gamma-ray burst (GRB) prompt phase where soft photons lag behind hard ones in their spectral studies. In contrast to this pattern, a fraction of GRBs show a negative spectral lag where hard photons arrive later compared to soft photons. Similarly, recent Fermi-Large Area Telescope observations show a late onset of high-energy photons in most GRB observations. A fraction of GRBs show a transition from positive to negative lags. Such negative lags and the spectral lag transition have no convincing explanation. We show that a structured GRB jet with velocity shear naturally produces both positive and negative spectral lags. The high-energy photons gain energy from repeated scattering with shearing layers and subsequently escape from higher altitudes. Hence, these photons are delayed compared to soft photons producing a negative spectral lag. The inner jet has no shear, and a positive lag appears to provide a unified picture of spectral lags in GRBs. The theory predicts a flip in spectral lag from positive to negative within the evolution of the prompt phase. Comparison of the observed lags with the prediction of the theory limits the possible range of GRB jet Lorentz factors to a few tens.
在伽马射线暴(GRB)瞬时阶段通常会观测到正光谱滞后现象,即软光子的光谱研究落后于硬光子。与这种模式相反,一部分伽马射线暴显示出负光谱滞后,即硬光子比软光子晚到达。同样,最近的费米-大面积望远镜观测结果表明,在大多数 GRB 观测中,高能光子的出现时间较晚。一小部分巨脉冲辐射暴显示出从正滞后到负滞后的转变。这种负滞后和光谱滞后的转变没有令人信服的解释。我们的研究表明,具有速度剪切的结构化GRB射流会自然产生正负两种光谱滞后。高能光子在与剪切层的反复散射中获得能量,随后从更高的高度逃逸。因此,与产生负谱滞后的软光子相比,这些光子被延迟了。内部喷流没有剪切力,正滞后似乎提供了一个关于 GRB 光谱滞后的统一图景。该理论预测,在瞬发阶段的演化过程中,光谱滞后会从正值翻转到负值。将观测到的滞后与理论预测进行比较,可以将古雷暴喷流洛伦兹因子的可能范围限制在几十个。