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Field
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experimental facilities to search for a new kind of very lightweight elementary particles, works on new concepts targeting high-frequency gravitational waves and develops related technologies.Postdoctoral
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comparable knowledge is demonstrated may be considered. Required Expertise: Candidates should have experience in: Modeling and design of MEMS resonators and acoustic wave devices Finite Element Analysis (FEA
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, Geotechnical Challenges, or similar expertise. No prior experience required. Preferred Qualifications Proficiency and experience in coastal numerical modeling tools such as circulation, flooding, wave and
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volcanic geohazards, a cryospheric sensor test bed, wind and waves in Arctic sea ice, and cross-initiative applications of infrasound sensing. Together, these initiatives bring researchers from across
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emphasis on standard and non standard finite element methods with applications to wave propagation problems and nonlinear reaction-diffusion problems. Further information about our research area and about
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or more of the listed disciplines. Proven expertise in multiphysics modeling (thermal, chemical, mechanical, hydraulic, and wave propagation processes). Proficiency in advanced programming and simulation
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Position Description The Laser Interferometer Gravitational-Wave Observatory (LIGO) has as its goal the development of gravitational wave physics and astronomy. The LIGO Laboratory is managed by
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direct current stimulation (tDCS), Temporal Interference (TI) stimulation, focused ultrasound neuromodulation, shock wave stimulation, and related neural modulation techniques. Advanced knowledge of human
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support the mission of the university through their work. Qualifications: PhD required Knowledge of ultrasonic waves and piezoelectrics FEM simulations of PZTs and acoustic wave propagation Ultrasonic
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coherence tomography concepts Basic knowledge of ultrasonic instrumentation and piezoelectrics FEM simulations of PZTs and acoustic wave propagation CAD to design device layouts Packaging of ultrasonic