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A standard expectation of primordial cosmological inflation is that itdilutes all relics created before its onset to unobservable levels. We presenta counterexample to this expectation by demonstrating that a network of cosmicstrings diluted by inflation can regrow to a level that is potentiallyobservable today in gravitational waves~(GWs). In contrast to undiluted cosmicstrings, whose primary GW signals are typically in the form of a stochastic GWbackground, the leading signal from a diluted cosmic string network can bedistinctive bursts of GWs within the sensitivity reach of current and future GWobservatories.

Gravitational Wave Bursts as Harbingers of Cosmic Strings Diluted by Inflation