A Bayesian approach to modelling multimessenger emission from blazars using lepto-hadronic kinetic equations

Bruno Jim'enez-Fern'andez, H. van Eerten
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Abstract

Abstract Blazar TXS 0506+056 is the main candidate for a coincident neutrino and gamma-ray flare event. In this paper, we compose a detailed kinetic lepto-hadronic emission model capable of producing a photon and neutrino spectrum given a set of parameters. Our model includes a range of large-scale geometries and both dynamical and steady-state injection models for electrons and protons. We link this model with a Markov Chain Monte Carlo sampler to obtain a powerful statistical tool that allows us to both fit the Spectral Energy Distribution and study the probability density functions and correlations of the parameters. Assuming a fiducial neutrino flux, we demonstrate how multi-messenger observations can be modelled jointly in a Bayesian framework. We find the best parameters for each of the variants of the model tested and report on their cross-correlations. Additionally, we confirm that reproducing the neutrino flux of TXS 0506+056 requires an extreme proton to electron ratio either in the local acceleration process or from external injection.
用轻强子动力学方程建模耀变体多信使发射的贝叶斯方法
Blazar TXS 0506+056是中微子和伽马射线同步耀斑事件的主要候选者。在本文中,我们建立了一个详细的动力学轻强子发射模型,该模型能够在给定一组参数的情况下产生光子和中微子光谱。我们的模型包括一系列大规模的几何形状,以及电子和质子的动态和稳态注入模型。我们将该模型与马尔可夫链蒙特卡罗采样器连接起来,以获得一个强大的统计工具,使我们既可以拟合光谱能量分布,又可以研究概率密度函数和参数的相关性。假设一个基准中微子通量,我们演示了如何在贝叶斯框架中联合建模多信使观测。我们为测试的模型的每个变体找到最佳参数,并报告它们的相互关系。此外,我们证实了再现TXS 0506+056的中微子通量需要一个极端的质子电子比,无论是在局部加速过程中还是从外部注入。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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