Past Events

The Chemistry of Color!

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Begin your weekend Saturday morning with Chris Marelli, Director of CU Boulder's General Chemistry Laboratories, as he presents entertaining & COLORFUL demonstrations! Chemistry is both a science and an art...bring the family to campus to learn all about the chemistry of colors!
CU Wizards shows are in-person, FREE and geared for grades K-8 and families.

Steering spin–valley polarizations through phonons and photons

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Control of spin and valley polarizations opens opportunities for spintronic and quantum information applications. Monolayer transition-metal dichalcogenides (TMDs) offer an appealing platform to harness such polarizations. TMDs host excitons in valley-shaped regions of their band structure, featuring well-defined carrier spins and obeying chiral optical selection rules. However, the technological potential of excitons in TMDs is impeded by rapid spin–valley relaxation.

Nonlinearity and Dissipation as a Resource for Engineered Quantum Systems – or a tale of cats and sharks

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Abstract: Engineered quantum systems, encompassing artificial mesoscopic structures governed by the principles of quantum mechanics, represent a cornerstone of modern quantum science. Notable examples include superconducting circuits, ultracold trapped atoms and ions, as well as electro and optomechanical systems. These systems are not only fascinating from a fundamental physics perspective but also serve as essential building blocks for technological applications.

Unlocking the Moon, Unlocking the Solar System

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The Moon offers multiple types of resources. It is a scientific resource, an exploration resource, and also a commercial resource. The Moon is a cornerstone for multiple science disciplines, not just lunar; it can help us learn how to effectively explore further into the Solar System with humans and robots, and it can enable commercial activities that support science and exploration. Intuitive Machines has conducted two lunar surface missions, including the first commercial landing in February 2024.

Nanoscale Imaging: Soft X-ray STXM and Ptychography at the ALS

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Abstract: Advancements in materials research increasingly require visualization of structure, composition, and functionality at the nanometer scale. Soft X-ray Ptychography and Scanning Transmission X-ray Microscopy (STXM) are two complementary techniques that leverage the brightness and coherence of synchrotron radiation at the Advanced Light Source (ALS) to probe materials with high spatial resolution and enhanced chemical sensitivity.

Magnetism on Crystalline Lattices

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Abstract: Magnetism is a striking example of how quantum mechanics and interactions among electrons combine to generate entirely new forms of collective behavior—phenomena that deepen our understanding of matter, as well as power modern technologies. Over the past decades, discoveries in magnetism have often heralded new paradigms in condensed matter physics, exemplified by antiferromagnetism and Mott insulators, and quantum spin liquids with their fractionalized excitations. In real materials, however, spins are inseparable from the crystalline lattices that host them.

Plasma Physics of the Turbulent Solar Corona: Old Questions, New Eyes

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The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic field, and ultimately expands into interplanetary space as the supersonic solar wind. This complex and unpredictable system varies over many orders of magnitude in space and time, so it's not surprising that we still do not have a complete theoretical understanding of its origins. In this talk, I will present some new observations and theoretical concepts that are helping us get closer to finally identifying and characterizing the physical processes responsible for the corona and solar wind.

Exploring the Fates of Atmospheric Peroxy Radicals with Model- and Computation-informed Environmental Chamber Experiments

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Abstract: Non-methane volatile organic compounds (NMVOC) are emitted into the Earth’s atmosphere by varied biogenic and anthropogenic sources. Though the concentrations of these compounds are minute, they exert an outsized influence on atmospheric composition, primarily through their oxidation chemistry. This chemistry leads to the formation of key secondary species including tropospheric ozone, a harmful pollutant, and secondary organic aerosol (SOA), a key component of atmospheric particulate matter with implications for climate and air quality.

How electron interactions generate giant effective magnetic fields in rhombohedral graphene

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Abstract:  Interacting electrons in strong magnetic fields give rise to rich phenomena, exemplified by the quantum Hall effect. In rhombohedral graphene, remarkably similar behavior has been observed even without an external field. In this talk, I will describe how electron–electron interactions in this system can spontaneously generate giant effective magnetic fields, reaching hundreds of Tesla. These emergent fields originate from self-organized layer-skyrmion textures, whose dynamics give rise to distinctive collective shape modes that can be experimentally probed.

2025 Physics and Quantum Career & Internship Fair

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The Department of Physics at the University of Colorado Boulder in collaboration with CUbit and JILA is hosting the third annual Physics and Quantum Career & Internship Fair on Friday, October 17th from 12:00 - 3:00 p.m. in the Glenn Miller Ballroom.

This event will feature employers across all areas of theoretical, experimental, and computational physics. The fair will connect physics undergraduate and graduate students and recent alumni with laboratory and industry leaders to learn about internships and employment opportunities.

A new sectional cloud model for the NSF Community Earth System Model

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We have developed a new cloud model, CARMA Cloud, for the NCAR Community Earth System Model that is designed to simplify the cloud model and improve its representation of cloud aerosol interactions. Rapid, unexpected, global warming since 2003 seems to be due to a combination of cloud feedback to global warming and strong response to aerosol changes. While the model is currently aimed at terrestrial cloud physics, the basic code has recently been used for exo-planet studies, and an early version of the model was used for studies of Martian ice clouds.

Engineering novel quantum phases in twisted graphene multilayers

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Abstract: Strongly correlated and topological phases in condensed matter systems are at the cutting edge of fundamental physics studies, as well as being promising candidates for the next generation of technological capabilities like quantum computing. In recent years, a remarkable amount of progress has been made in creating and controlling such phases by introducing a small twist angle or lattice mismatch between two-dimensional (2D) materials.

Effects of the Sun’s trajectory through the galaxy on Earth’s climate over the past 10 million years

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Abstract: With the advent of the Gaia space mission, there has been a revolution in astronomers’ ability to precisely locate the interstellar structures the Sun may have encountered on its voyage around the galaxy. We now have the spatial resolution to trace the Sun’s trajectory back through its interstellar environment up to 60 million years in the past (4000 light-years in distance). This timescale is commensurate with the timescale over which we can reconstruct the paleoclimate of Earth from deep ocean foraminiferas.

Regulation of LRRK2: Identifying vulnerabilities for Parkinson's Disease therapeutics

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Parkinson’s Disease (PD) is the second most prevalent neurodegenerative disease, affecting ~10 million people worldwide. One of the most commonly mutated genes in PD codes for Leucine Rich Repeat Kinase 2 (LRRK2). Autosomal dominant mutations in LRRK2 cause familial PD, while mutations in LRRK2 are risk factors for sporadic PD and increased activity of LRRK2’s kinase has been linked to the sporadic form of the disease as well. This has made LRRK2 the main actionable target for PD therapeutics.

There and Back Again: A Journey to the Sun

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Parker Solar Probe successfully completed its prime mission in 2025, measuring solar wind plasma in-situ as close as 8.8 solar radii (~0.04 AU) from the solar photosphere over a series of close-approach orbits. These close approaches to the Sun enable novel exploration of fundamental stellar processes, such as solar wind acceleration, solar wind heating, interplanetary dust destruction, and radial evolution of solar surface structure. These processes leave distinct signatures in near-Sun particle and field observations that allow us to untangle the physical mechanisms driving them.

New Experimental Platforms for Molecular Polaritonics

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Abstract: Polaritons are hybrid light-matter states with unusual properties that arise from strong interactions between a molecular ensemble and the confined electromagnetic field of an optical cavity. Cavity-coupled molecules appear to demonstrate energetics, reactivity, and photophysics distinct from their free-space counterparts, but the mechanisms and scope of these phenomena remain open questions. I will discuss new experimental platforms that the Weichman Lab is developing to investigate molecular reaction dynamics under strong cavity coupling.

Altermagnetism: an unconventional quantum state of matter

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Abstract: Magnetism is the posterchild of how the interplay between electron-electron interactions and quantum physics promotes novel macroscopic phenomena. Historically, the evolution of our understanding of magnetism has been related to the discovery of new paradigms in condensed-matter physics, as exemplified by the connections between antiferromagnetism and Mott insulators, spin glasses and non-ergodic states, and spin liquids and fractionalized excitations.

Photophoretic Flyers: Novel Propulsion for Near-Space Sensing

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While photophoresis, or “light-driven motion,” has long explained how aerosol layers remain aloft in the middle atmosphere, practical applications have only recently been gaining attention. Advances in nanofabrication now allow us to build lightweight structures that can propel themselves upward using photophoretic forces alone. These “photophoretic flyers” can sustain flight in near-space (30–100 km altitudes), a region that is too high for aircraft and balloons and too low for satellites.