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are looking for candidates with interests in quantum mechanical condensed matter theory including: strongly correlated electron systems & mesoscopics, topological phases, ultracold atomic gases, quantum optics
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Are you passionate about experimental aerodynamics and flow visualization? Apply for a PhD position that aims at transforming flow field measurements into aerodynamic forces by pressure and friction
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Post-Doctoral Associate/Associate Research Scientist in the Division of Science (Biological Physics)
the successful candidate will collaborate closely. Applicants must have a PhD in physics or biological physics. Excellent analytical skills are required and prior experience in soft matter or biological physics
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using soft X-ray ptychography and tomography, and present and publish your results at international conferences and in peer-reviewed journals. Your Profile Completed PhD in physics, electrical engineering
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-based instruments for applications across a wide range of disciplines including adaptive optics, spectroscopy, biophysics, remote sensing, laser communications, and fusion diagnostics. We host the ESA
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relevant to have experience with analysis techniques such as AFM, WLI, contact-angle, XPS, infrared metrology. You will work in the XUV Optics group at the University of Twente, embedded in the MESA
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New York and the selected candidate will be expected to work onsite as of their effective start date. PhD in Physics, neuroscience, biology or a related field. Experience in optics, programming, and/or
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We are seeking a motivated Postdoctoral Fellow to support studies investigating the neural mechanisms underlying corneal pain and dry eye disease. The laboratory uses rodent models
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-based instruments for applications across a wide range of disciplines including adaptive optics, spectroscopy, biophysics, remote sensing, laser communications, and fusion diagnostics. We host the ESA
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Detection Sensors research within the group, in close collaboration with the optics laboratory at Ghent University (UGent). Whereas all current gravitational wave detectors operate at 1064 nm, ET and