《度規擾動光譜方法測試廣義相對論的重力波》研討會


Seminar:- Gravitational-wave tests of general relativity with METRICS

Many of the gravitational-wave signals detected by the LIGO-Virgo-KAGRA detectors end with exponentially decaying waves emitted by the remnant black holes formed by the corresponding binary black-hole coalescence. The frequencies and lifetimes of these decaying waves are called quasinormal mode frequencies, and they are closely related to the dynamics of the spacetime near the horizon of the remnant black hole. In this connection, detecting black-hole quasinormal modes is a powerful probe into the nature of gravity. However, the challenge of computing quasinormal mode frequencies has meant that quasinormal-mode tests of gravity have remained largely statistical and model-independent. In this talk, the speaker will introduce Metric pErTuRbations wIth speCtral methodS(METRICS), a novel spectral code capable of accurately computing the quasinormal mode frequencies of black holes, including those with modifications beyond Einstein’s theory or the presence of matter. He will demonstrate METRICS’ accuracy in calculating quasinormal mode frequencies within general relativity as a validation. Then, he will show the results of the first accurate computations of the quasinormal-mode frequencies of rapidly rotating black holes in Einstein-scalar-Gauss-Bonnet gravity and dynamical Chern-Simons gravity. Finally, he will discuss how the METRICS frequencies can be used to test different gravity theories by analyzing gravitational waves.

時間:2025.01.21(二) 13:30
地點:香港城市大學 楊建文學術樓* Y4302
講者:Dr. Adrian Chung Ka-Wai 鍾嘉唯 博士 (Postdoc Research Associate, University of Illinois Urbana-Champaign, US)
語言:英語


【此屬轉載信息,以主事單位發布為準】


*Yeung Kin Man Academic Building

此活動由香港城巿大學物理系主辦。

https://www.cityu.edu.hk/phy/node/3801

Verified by MonsterInsights