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Explore the multi-messenger approach to hunting for galactic PeVatrons in this 38-minute conference talk. Learn about the search for cosmic ray accelerators capable of reaching petaelectronvolt (PeV) energies within our galaxy using combined observations from gamma rays, neutrinos, and cosmic rays. Discover how researchers combine data from multiple detection methods to identify and study these extreme astrophysical accelerators, which are among the most powerful particle acceleration sites in the universe. Examine the theoretical frameworks and observational strategies used to locate PeVatron candidates, understand the challenges in distinguishing between different acceleration mechanisms, and investigate the role of supernova remnants, pulsar wind nebulae, and other high-energy astrophysical sources as potential PeVatron sites. Gain insights into the latest findings from gamma-ray observatories, neutrino detectors, and cosmic ray experiments that are revolutionizing our understanding of galactic particle acceleration and the origins of the highest-energy cosmic rays observed on Earth.
