Constructing Echo Waveform from Kerr-like Background

Document #:

LIGO-T1900363-v4

Document type:

T - Technical notes

Abstract:

Gravitational wave (GW) echoes, the GWs reflected from the surface of an exotic compact object (ECO), may provide information about the Planck-scale structure near the horizon. Previous work on GW echoes is mostly done for non-rotating ECOs described by Schwarzschild metric. In more general cases, a theoretical model for GW echoes from spinning ECOs is of importance in the searches for echoes in LIGO/Virgo data. In this project, we derive the echo waveforms for a spinning ECO, incorporate them into current search pipelines, and study the stability of spinning ECOs.

Files in Document:

• Final report (376850, file is not accessible)

Other Files:

• InterimReport1.pdf (file is not accessible)
• InterimReport2.pdf (file is not accessible)
• Shuo_FinalPresentation.pdf (file is not accessible)
• Shuo_FinalPresentation_v2.pptx (file is not accessible)
• report.pdf (file is not accessible)

Topics:

• GW source predictions

Authors:

• Shuo Xin
• Yanbei Chen
• Baoyi Chen
• Ka-Lok Lo
• Ling Sun

Keywords:

SURF19

Notes and Changes:

Final report is added.

Referenced by:

• LIGO-T1900757: Final reports from LIGO SURF program, Summer 2019