超大质量黑洞吸积盘中的高能中微子辐射研究进展及展望  

Research progress and prospects of high-energy neutrino radiation in supermassive black hole accretion disks

作　　者：王凯[1] Kai Wang(Department of Astronomy,School of Physics,Huazhong University of Science and Technology,Wuhan 430074,China)

机构地区：[1]华中科技大学物理学院天文学系,武汉430074

出　　处：《科学通报》2025年第3期398-410,共13页Chinese Science Bulletin

基　　金：国家自然科学基金(12003007);中央高校基本科研业务费专项资金(2020kfyXJJS039)资助。

摘　　要：活动星系核超大质量黑洞吸积盘中被认为包含着丰富的恒星和致密星以及它们构成的双星系统,其在吸积盘上的演化会产生不同类型的天体物理爆发现象,产生包含引力波、电磁辐射和高能中微子的多信使信号.其中,高能中微子在研究超大质量黑洞吸积盘中天体物理爆发过程中可以起到重要作用.本文简要综述了近些年来活动星系核超大质量黑洞吸积盘上不同天体物理暂现源爆发过程中的高能中微子辐射研究进展,内容包括吸积盘中双恒星级黑洞并合遗迹黑洞吸积气体物质形成的喷流和外流星风、伽马射线暴和超新星在与盘物质作用过程中的高能中微子生成,并总结了对这些源的多信使探测,最后展望了下一代高能中微子探测器对理解超大质量黑洞吸积盘中天体物理过程的机遇.In recent years,with the operation of a series of gravitational wave,high-energy neutrino,and electromagnetic radiation telescopes,astronomical research has entered the era of multi-messenger research.It is believed that the accretion disks around supermassive black holes in active galactic nuclei contain a wealth of stars and compact stars,as well as binary systems they form,whose evolution on the accretion disk can produce various types of astrophysical phenomena,generating multi-messenger signals including gravitational waves,electromagnetic radiation,and high-energy neutrinos.The astrophysical activities on the accretion disks of active galactic nuclei have aroused great interest in the astrophysical community due to the uniqueness of their environment.The accretion disks and the nuclear environment of active galactic nuclei are very complex,and high-energy neutrinos can easily escape from such a complex environment,becoming a unique and effective messenger to help us understand the astrophysical burst processes in the accretion disk.This paper briefly reviews the research progress of high-energy neutrino radiation for the different astrophysical transient sources within the accretion disks of active galactic nuclei in recent years,including the jets and winds formed by the remnant black hole of binary stellar-mass black holes in the accretion disk,and the high-energy neutrino production in the interaction process of gamma-ray bursts and supernovae with disk matter.Especially for the process of binary black hole mergers and the short gamma-ray burst process of binary neutron star mergers,which is an important target for ground gravitational wave detector,if they occur on the accretion disk,they can also produce considerable high-energy neutrino radiation.For the joint detection of gravitational waves and high-energy neutrinos,current gravitational wave detection equipment and neutrino detectors have made some searches,but there are no associated detection results yet.The successful joint detection of gravitat

关 键 词：吸积盘 超大质量黑洞 高能中微子 引力波 暂现源 

分 类 号：P145.8[天文地球—天体物理]