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Modeling asymmetric binaries: state of the art in gravitational self-force theory

组织者

拉尔斯•安德森 , Alejandro Torres Orjuela , 张笑然

演讲者

Adam Pound

时间

2025年03月14日 16:00 至 17:00

地点

A3-2-301

线上

Zoom 787 662 9899 (BIMSA)

摘要

Asymmetric binaries, such as intermediate- and extreme-mass-ratio inspirals (IMRIs and EMRIs), will be critical sources for next-generation gravitational-wave detectors such as LISA. These systems are modelled with an asymptotic approximation method known as self-force theory. In this talk, I discuss the foundations of self-force theory, its applications to gravitational waveform modeling, and the current state of the art in the field.