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Explore a hydrosimulations-based approach to relate the Fast Radio Burst (FRB) dispersion measure-redshift relation to cosmic structure in this 22-minute conference talk. Learn how computational hydrodynamic simulations can be used to understand the relationship between FRB dispersion measures and their redshift distribution, providing insights into the cosmic web and intergalactic medium. Discover how this methodology connects FRB observations to theoretical models of cosmic structure formation and evolution. Gain understanding of how dispersion measure measurements from FRBs can serve as probes of the universe's large-scale structure and the distribution of baryonic matter between galaxies. This presentation was delivered as part of the FTSky program at the International Centre for Theoretical Sciences, focusing on fast radio transients and their applications in astrophysics and cosmology.
