Title:Compact Binary object Coalescencealong eccentric orbit---From Template to Science
Speaker: Zhoujian Cao (Academy of Mathematics and Systems Science, CAS)
Abstract:
With the increasing discovery of novel and significant gravitational wave events by ground-based gravitational wave detectors, the development of gravitational wave astronomy is in full swing. The success of space-based laser interferometric detectors such as LISA Pathfinder, Taiji-1, and TianQin-1 has led to growing research investments in space-based gravitational wave detection by more countries and research teams. Currently, Europe and the United States have officially launched the LISA space-based gravitational wave detection project. Meanwhile, China's Taiji, TianQin, and Japan's DECIGO space-based gravitational wave detection projects are also advancing actively. Under the favorable collaboration and competition dynamics among these four initiatives, space-based gravitational wave detectors will begin operation in a decade. Gravitational wave theoretical templates serve as a crucial theoretical foundation for gravitational wave data processing. This report will begin with an overview of the current status of ground-based gravitational wave detection and data analysis, compare the requirements for gravitational wave theoretical templates needed for expected space-based detection, and introduce the current progress in modeling for space-based gravitational wave detection. Elliptical orbit binary merger systems have recently garnered widespread attention as gravitational wave sources, driven by space-based gravitational wave detection and observed events such as GW190521. This report will also delve into the profound scientific implications of gravitational wave events from elliptical orbit binary mergers.