Echoes of compact objects: new physics near the surface and matter at a distance
R. A. Konoplya, Z. Stuchl\'ik, A. Zhidenko

TL;DR
This paper investigates how echoes in gravitational wave signals from compact objects are influenced by both new physics near the surface and matter at a distance, using a wormhole model with an added shell of matter.
Contribution
It introduces a combined analysis of echoes caused by near-horizon physics and distant matter, using a traversable wormhole model with a shell to study their interplay.
Findings
Echoes are primarily attributable to near-horizon physics.
Distant matter influences the timing and amplitude of echoes.
Environmental effects are less likely to mimic signals from new physics.
Abstract
It is well known that a hypothetical compact object that looks like an Einsteinian (Schwarzschild or Kerr) black hole everywhere except a small region near its surface should have the ringdown profile predicted by the Einstein theory at early and intermediate times, but modified by the so-called echoes at late times. A similar phenomenon appears when one considers an Einsteinian black hole and a shell of matter placed at some distance from it, so that astrophysical estimates could be made for the allowed mass of the black hole environment. While echoes for both systems have been extensively studied recently, no such analysis has been done for a system featuring phenomena simultaneously, that is, echoes due to new physics near the surface/event horizon and echoes due to matter at some distance from the black hole. Here, following [9, 11], we consider a traversable wormhole obtained by…
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