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tasks. Job Description Primary Duties & Responsibilities: Lead theoretical and mathematical modeling of ultrasonic thin-film and pintle atomization, interfacial instabilities, acoustic streaming, and wave
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number of health and wellbeing initiatives to support you. Closing Date: 19 October 2026 The Role The successful candidates will join a collaborative team, ABMHydro (https://www.abmhydro.com/), engaged in
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, including dark matter detection (ADMX, ALPS, SuperCDMS), experimental particle physics (Belle II, COHERENT, CMS, DUNE, SBND), gravitational wave detection (LIGO, LISA, NANOGrav), theoretical astrophysics, and
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interactions between acoustic wavefields and the dynamic ocean, including the effects of temperature structure, salinity, pressure, internal waves, mesoscale variability, seabed composition, bathymetry, and
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, gravitational waves, neutrino astrophysics, cosmology, and galactic astronomy. The department is committed to building an inclusive and collegial environment in which faculty, staff, and students of all
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. Current projects span visible, near-infrared, and short-wave infrared imaging and include applications in dermatology, vascular disease, tissue injury, and physiologic monitoring. The laboratory works at
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regions, but also at all latitudes and at all local times. The probe is currently in its second mission extension phase, with an end date currently scheduled for October 2028. The Juno/Waves instrument
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pipelines for searching continuous gravitational waves and/or dark matter candidates. Depending on the candidate's interests, the project may also involve black hole ringdown studies and preparations for next
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systems for use in breaking waves, both in the field and in the lab Contribute to analysis of images, and development of the open-source analysis software PyOPIA (https://github.com/SINTEF/pyopia
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and classical physics as well as between quantum and bio-molecular science. We develop universal matter-wave interferometry in the limit of high mass and high complexity, from organic molecules to metal