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Gamma-ray Bursts (GRBs) are relativistic cosmological beacons of transienthigh energy radiation whose afterglows span the electromagnetic spectrum.Theoretical expectations of correlated neutrino emission position GRBs at anastrophysical nexus for a metamorphosis in our understanding of the Cosmos.This new dawn in the era of experimental (particle) astrophysics and cosmologyis afforded by current facilities enabling the novel astronomy of high energyneutrinos, in concert with unprecedented electromagnetic coverage. In thatregard, GRBs represent a compelling scientific theme that may facilitatefundamental breakthroughs in the context of Swift, Fermi and IceCube.Scientific synergy will be achieved by leveraging the combined sensitivity ofcontemporaneous ground-based and satellite observatories, thus optimizing theircollective discovery potential. Hence, the advent of GRB multi-messengerastronomy may cement an explicit connection to fundamental physics, via nascentcosmic windows, throughout the next decade.

GRB Astrophysics in the Swift Era and Beyond