and 
Molecules are amongst the most complex objects that can be controlled and studied at the individual quantum state level. In this talk, I will introduce some of the extraordinary advances made in the last decade by the application of AMO physics tools, including cavity-enhanced optical frequency comb and microwave techniques, to such quantum-state-resolved spectroscopy.
With reception in the h-bar afterwards.
Abstract: Neutral atoms trapped in optical tweezer arrays have emerged as a promising platform for quantum computing, and for the analog simulation of various spin models. In this work, we apply the programmable control provided by optical tweezer arrays to new domains in quantum science by means of interfacing optical tweezers with a Hubbard-regime optical lattice, and extending the optical tweezer toolbox to new atomic species (namely alkaline earth atoms).
Coffee, tea and cookies will be available in G1B31 (across from G1B20) from 3:30–3:50 p.m.
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Coffee, tea and cookies will be available in G1B31 (across from G1B20) from 3:30–3:50 p.m.
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Abstract: Abstract: Simple measures of the productivity and prominence vary enormously across both individual scientists and across institutions. But, how much do these sometimes enormous inequalities represent genuine meritocratic differences, and how much are they biased by non-meritocratic factors that may limit scientific progress?
Abstract: I last came to CU in 2015, and talked almost entirely about molecules in galaxies. Now I'm 8 years older, and 8 years more esoteric: 2023 Desika is going to talk all about dust! But seriously, dust is awesome. It impacts almost every astrophysical observation that you make, is a critical ingredient to thermal balance in the ISM, and is used to trace obscured star formation at all redshifts. I'll present the results from a new model for dust in galaxy simula
Abstract: For the past decade we have begun to explore the origin of planetary compositions which are set in the natal protoplanetary disk.
