Rogue echoes from exotic compact objects
Aaron Zimmerman, Richard N. George, Yanbei Chen

TL;DR
This paper suggests that gravitational wave echoes from exotic compact objects could have extremely long delays, making them uncorrelated with GW events and challenging to detect with current methods.
Contribution
It introduces a new perspective on GW echo timing, showing delays can be billions of years, which has implications for detection strategies.
Findings
Time delays between GW events and echoes can be billions of years.
Rogue echoes may not be correlated with original GW events.
Current searches may miss these long-delayed echoes.
Abstract
Binary systems containing exotic compact objects may emit repeated bursts of gravitational waves (GWs) following coalescence. Such GW echoes would provide a clear signature of new physics, but searches for them have not yielded a convincing detection. Here we argue that the typical time delay between a GW event and its echoes is much greater than generally expected, due to long propagation times through objects that mimic black holes. We provide a simple recipe for computing the time delay and several examples. These time delays can be billions of years, resulting in rogue echoes that are not correlated with GW events and evade all current constraints. They would be detectable only by searches for individual echoes or GW bursts.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Seismology and Earthquake Studies
