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within fusion reactors, especially plasma-facing materials (PFMs) exposed to intense heat fluxes and energetic particles. Understanding and predicting how these materials degrade under such conditions is
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particle and photon sources owing to their ability to sustain accelerating fields on the scale of hundreds of GV/m — three orders of magnitude higher than radio-frequency accelerators. At DESY, we're
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of Nora Brambilla at the Technical University of Munich. The project aims at unravelling a QCD derived description of the XYZ exotics observed in the sector of two heavy quarks at the accelerator
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the research findings to the broader aviation community, through publications, conferences, and workshops, to accelerate the adoption of these optical measurement capabilities for future system development
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of particle acceleration and the Sun's interaction with the local interstellar medium. See https://spacephysics.princeton.edu/ for more information about the Space Physics Group at Princeton University