浙江工业大学物理学院
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Multimessenger Probes of Dark Matter Environment Around Supermassive Black Holes (第843场)
浏览量:52    发布时间:2026-01-15 12:33:52

报告题目:Multimessenger Probes of Dark Matter Environment Around Supermassive Black Holes

报告人:袁官文

报告时间:2026年1月15日(周四)下午 14:00-16:00

报告地点:浙江工业大学理学楼 二楼师生活动中心

摘要(Abstract):SMBHs can strongly enhance the local dark matter density in their surroundings due to its strong gravity.This enhancement can significantly amplify dark matter-related processes, and making potential signals more detectable than in other astrophysical environments. Recent breakthroughs in stellar dynamics in Galactic Centre(GRAVITY/Keck), horizon-scale black hole imaging (EHT), stochastic gravitational-wave background (PTAs), and early-Universe galaxy observations (IWST) provide powerful, complementary probes of the environment around SMBHs. In this talk, I will discuss how these multimessenger observations can be used to search for signatures of dark matter near SMBHs, including WIMPs, ultralight dark matter, axion-like particles.and primordial black holes. I will highlight how dark matter may influence the SMBHs observations, and how SMBHs can serve as unique laboratories for testing dark matter physics.

报告人简介(Bio)袁官文现为意大利特伦托大学博士后研究员。2018年本科毕业于四川大学,2023年博士毕业于中国科学院紫金山天文台,随后任香港科技大学与中科院高能所联合博士后。研究兴趣包括暗物质现象学、超大质量黑洞、引力波和机器学习在天文学中的应用,迄今已在PRLScience Bulletin等期刊发表学术论文30篇,INSPIRE引用约1200次。曾获中国科学院院长奖、中国天文学会奖及博士后站前特别资助等荣誉。

 

邀请人王远瞩


博学堂讲座
Multimessenger Probes of Dark Matter Environment Around Supermassive Black Holes (第843场)
浏览量:52    发布时间:2026-01-15 12:33:52

报告题目:Multimessenger Probes of Dark Matter Environment Around Supermassive Black Holes

报告人:袁官文

报告时间:2026年1月15日(周四)下午 14:00-16:00

报告地点:浙江工业大学理学楼 二楼师生活动中心

摘要(Abstract):SMBHs can strongly enhance the local dark matter density in their surroundings due to its strong gravity.This enhancement can significantly amplify dark matter-related processes, and making potential signals more detectable than in other astrophysical environments. Recent breakthroughs in stellar dynamics in Galactic Centre(GRAVITY/Keck), horizon-scale black hole imaging (EHT), stochastic gravitational-wave background (PTAs), and early-Universe galaxy observations (IWST) provide powerful, complementary probes of the environment around SMBHs. In this talk, I will discuss how these multimessenger observations can be used to search for signatures of dark matter near SMBHs, including WIMPs, ultralight dark matter, axion-like particles.and primordial black holes. I will highlight how dark matter may influence the SMBHs observations, and how SMBHs can serve as unique laboratories for testing dark matter physics.

报告人简介(Bio)袁官文现为意大利特伦托大学博士后研究员。2018年本科毕业于四川大学,2023年博士毕业于中国科学院紫金山天文台,随后任香港科技大学与中科院高能所联合博士后。研究兴趣包括暗物质现象学、超大质量黑洞、引力波和机器学习在天文学中的应用,迄今已在PRLScience Bulletin等期刊发表学术论文30篇,INSPIRE引用约1200次。曾获中国科学院院长奖、中国天文学会奖及博士后站前特别资助等荣誉。

 

邀请人王远瞩