Effect of high harmonic loops on gravitational wave bounds from cosmic strings
Despoina Pazouli, Konstantinos Palapanidis, Anastasios Avgoustidis,, Edmund J. Copeland

TL;DR
This paper models how high harmonic loops in cosmic strings affect gravitational wave signals, updating event rate predictions by considering self-intersections, cusp production, and harmonic distributions.
Contribution
It introduces a binary tree model to estimate self-intersections and cusp events on high harmonic cosmic string loops, refining gravitational wave signal predictions.
Findings
Event rate of gravitational waves depends on harmonic content and cusp production.
High harmonics can significantly alter gravitational wave signals from cosmic strings.
Updated models show different redshift distributions compared to previous estimates.
Abstract
Based on a binary tree model for the self intersection of cosmic string loops containing high harmonics we estimate the number of self-intersections of the parent and daughter loops and the associated cusp production to determine the most likely number of cusp events per period on the resultant non-self intersecting loops, and provide an updated calculation for the gravitational wave signal that arrives on Earth from cusps on such loops. This is done for different numbers of cusps supported from the cosmic strings of the network, and for different harmonic distributions on the loops. We plot our results of the event rate of gravitational waves emanating from the cusps in terms of redshift, having fixed the value of and the received frequency of the signal, and compare our results to those in [1, 2].
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