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production at LHCb https://arxiv.org/pdf/2507.13447 - Theory-Informed Neural Networks for Particle Physics. Knowledge & Experience Essential Background in high energy particle physics and/or advanced quantum
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PLEASE NOTE- Applications MUST be submitted to the Harvard Academic Positions website in order to be considered. https://academicpositions.harvard.edu/postings/15491 The Gravity, Spacetime, and Particle
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involving giant impacts around the Sun and other stars. The project applies state-of-the-art computational physics methods, particularly Smoothed Particle Hydrodynamics (SPH) with self-gravity, shocks
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, Cosmology , Experimental or Theoretical Physics , GR-Cosmology (gr-qc) , Gravitational Physics , Gravitational Waves , hep , HEP-Phenomenology (hep-ph) , HEP-Theory (hep-th) , Particle/Cosmology Theory
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, particle physics, and mathematical physics. The Astroparticle and Cosmology group (https://astrocosmolapth.com ) conducts research on cosmic large-scale structure, cosmic microwave and infrared backgrounds
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University of North Carolina at Chapel Hill | Chapel Hill, North Carolina | United States | about 1 hour ago
of particle physics) to the very large (the realm of astronomy, while expanding the boundaries of knowledge in the many subfields spanning length scales between. Forefront physics and astronomy research
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6 Mar 2026 Job Information Organisation/Company CNRS Department Institut de planétologie et d'astrophysique de Grenoble Research Field Chemistry Physics Technology Researcher Profile Recognised
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T.Vickey@sheffield.ac.uk or look at the University’s website: https://www.sheffield.ac.uk/postgraduate/phd. Further Information on the Particle Physics group in Sheffield and our projects can be found here
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Helmholtz-Zentrum Dresden-Rossendorf - HZDR - Helmholtz Association | Dresden, Sachsen | Germany | 21 days ago
or strong interest in interfacial physics/chemistry, surface science, wetting, thin films, and colloidal/interfacial phenomena # Experience in or strong interest in bubble-particle interactions, especially
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plasmas, (2) compressible and incompressible magnetohydrodynamic (MHD) turbulence in Cartesian and spherical geometries, and (3) wave-particle interactions and parametric instabilities. Simulation