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Infrastructure? No Offer Description PhD Student Scholarship Holder (f/m/x) Ref Number: JKOP/20/2026 Location: Warsaw, Poland Salary: scholarship before the mid-term evaluation: PLN 6,195.50 gross per month
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Max Planck Institute for the Structure and Dynamics of Matter, Hamburg | Hamburg, Hamburg | Germany | 6 days ago
-fast phenomena, X-ray physics and dynamical imaging in all areas of science, covering physics, chemistry and biology. 23 interdisciplinary PhD positions in Ultrafast Science and Quantum Materials – IMPRS
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metallurgy or additive manufacturing; characterisation using advanced electron microscopy and x-ray diffraction techniques; mechanical testing using macro/micro-mechanical methods and failure investigation
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, structure, defect chemistry, and ionic transport behaviour. Comprehensive materials characterisation will be undertaken using structural, thermal, and electrochemical techniques, including X-ray diffraction
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. Bert Koopmans, based at Eindhoven University of Technology. PhD candidate 1 will explore fundamental processes underlying the deterministic creation and annihilation of sub-diffraction limited skyrmions
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Chair of Biological Imaging 02.02.2026, Academic staff We now seek a highly qualified and motivated PhD student (f/m/x) to drive the advancement and application of a novel multimodal microscope. The
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Chair of Biological Imaging 02.02.2026, Academic staff We now seek a highly qualified and motivated PhD student (f/m/x) to drive the development of a novel quantum enhanced microscope. The Institute
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possess translational symmetry, the role of structure and symmetry in glasses is not established. This research programme involves the development of new x-ray and electron diffraction-based methods
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Max Planck Institute for Chemical Energy Conversion, Mülheim an der Ruhr | M lheim an der Ruhr, Nordrhein Westfalen | Germany | 10 days ago
under operando conditions, using advanced X-ray spectroscopic techniques (XAS, XES, RXES), both in-house and at synchrotron facilities. The work will be embedded in a highly collaborative
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-induced have been reported at X-ray, optical, and radio wavelengths, but confirmation and characterization has been difficult: the decisive test is whether the emission recurs on the planetary orbital