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彭桓武科教合作中心量子论坛第四百八十三讲:Non-Hermitian Structures in Black Hole Quasinormal Spectra

发布人:日期:2026-06-23浏览数:

报告题目:Non-Hermitian Structures in Black Hole Quasinormal Spectra

报  告 人:王鹏 教授,四川大学

研究方向:黑洞物理学、数值相对论、弦低能有效理论及规范/引力对偶

报告时间:2026年6月29日(星期一)下午15:00

报告地点:格物楼326教室

报告摘要:

This talk discusses non-Hermitian structures in black-hole quasinormal-mode spectra and their implications for black hole spectroscopy. Using hairy black holes in Einstein-Maxwell-scalar theory as a physical setting, we show that spectrally stable and unstable QNM families can coexist, while early-time ringdowns are mainly governed by the more spectrally stable modes. We then identify an exceptional point at which two QNM branches coalesce, and show that the corresponding waveform is more naturally described by an EP ansatz containing a resonant term linear in time. These results clarify how non-Hermitian spectral phenomena appear in both frequency-domain spectra and time-domain ringdown modeling.

报告人简介:

王鹏,四川大学教授,博士生导师。本科毕业于北京大学,于美国加州理工学院获得博士学位。主要研究领域为引力理论和弦理论,目前研究兴趣主要集中于黑洞物理学、数值相对论、弦低能有效理论及规范/引力对偶等。

一审:王梦杰

二审:贺兵香

三审:廖洁桥