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

Bruno Jim'enez-Fern'andez, H. van Eerten
{"title":"A Bayesian approach to modelling multimessenger emission from blazars using lepto-hadronic kinetic equations","authors":"Bruno Jim'enez-Fern'andez, H. van Eerten","doi":"10.1093/mnras/staa3163","DOIUrl":null,"url":null,"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.","PeriodicalId":8437,"journal":{"name":"arXiv: High Energy Astrophysical Phenomena","volume":"7 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2020-06-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: High Energy Astrophysical Phenomena","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1093/mnras/staa3163","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

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.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
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。
求助全文
约1分钟内获得全文 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade The galactic millisecond pulsar population : implications for the Galactic Center Excess. Spectral-temporal features of repeating ( one-off ) FRBs and Axion Star. AstroSat/UVIT observations of IC 4329A: constraining the accretion disc inner radius
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1