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Field
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of Transition Edge Sensor (TES) bolometers for studies of the Cosmic Microwave Background (CMB), while also supporting the exploration of novel applications for superconducting detectors. As a member of Argonne’s
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Position Description The Simons Observatory (SO) is a leading cosmic microwave background (CMB) experiment located in the Atacama Desert of northern Chile. SO is a collaborative effort among
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parallel, the rare-earth solid-state system will be coupled to microwave resonators to explore future connections to superconducting qubits. The project will conclude with a demonstration of quantum gate
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devices exploiting the nonlinear kinetic inductance of thin superconducting films, including microwave resonators for frequency-domain multiplexed readout of single photon detectors (kinetic inductance
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electronic instrumentation is essential. Desirable skills include: • Solid experience in electronic measurement systems and instrumentation. • Familiarity with RF/microwave techniques and fast signal
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with complementary techniques such as Kelvin probe force microscopy, scanning microwave impedance microscopy, cathodoluminescence, Raman spectroscopy, and electron microscopy to connect local chemical
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, for on-chip magnon quantum sensing Position Requirements Superconducting resonator design, simulation and nanofabrication. Microwave circuit design and characterization, including vector network analyzer
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: accelerator, cyclotron, linear accelerator, heavy ion, beam, charged particle, electronic circuit, electrical system, instrumentation, electromagnetic field analysis, radio frequency, microwave, accelerating
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have a PhD in wireless communication, electrical engineering, antenna and electromagnetic engineering, telecommunications engineering, microwave engineering, or a closely related field, and you bring a
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, semiconductor or hybrid semiconductor-superconductor quantum electronic devices, and microwave approaches applied to quantum circuits. About the Department School of Physics and Astronomy: https://cse.umn.edu