3:30 – 5 p.m., Oct. 16, 2025 OSC Colloquium: Ben Cromey Image 3:30 – 5 p.m., Oct. 2, 2025 OSC Colloquium: Hakan Tureci Recent strides in machine learning have shown that computation can be performed by practically any controllable physical system that responds to physical stimuli encoding data [1]. This perspective opens new frontiers for computational approaches using Physical Neural Networks (PNNs) [2, 3, 4] and provides a framework to deepen our understanding of their biological counterparts—neural circuits in living organisms. Image 3:30 – 5 p.m., Sept. 25, 2025 OSC Colloquium: Stuart Shaklan One of NASA’s primary science goals is to directly image and characterize the atmospheres of Earth-like planets orbiting nearby stars. The observations are extremely challenging because the planets appear adjacent to their parent stars, near telescope diffraction limits, and their reflected light is 10 billion times fainter than the star. An elegant solution to this problem, first proposed by Lyman Spitzer in 1962, is to employ a starshade, a flower-shaped diffraction screen positioned far in front of a telescope so that it shadows the starlight without blocking the planet light. Image 3:30 – 5 p.m., Sept. 18, 2025 OSC Colloquium: Vivishek Sudhir A pre-eminent problem of modern physics is to reconcile the disparity between the laws of quantum physics – which apply at the small scale – and the laws of gravity – that apply at the large scale. This talk will motivate the nature of the fundamental problem and highlight some of the ideas we are currently pursuing to address it. In particular, a decisive confrontation of gravity and quantum theory calls for mechanical objects, massive enough to measurably gravitate with each other, prepared in quantum states of their motion. Image 3:30 – 5 p.m., Sept. 11, 2025 OSC Colloquium: Kyungtae Kim Optical atomic clocks now reach fractional frequency uncertainties below 10^-18, pressing toward a redefinition of the second. Optical lattice clocks harness laser cooling and trapping technologies for holding and probing ultracold atoms. These clocks are based on simple atomic spectroscopy, but as we continue zooming in to narrower frequency ranges, we encounter challenges that test our fundamental understanding of how atom-light and atom-atom interactions work, demanding cutting-edge laser stabilization and quantum state control. Image 3:30 – 5 p.m., Sept. 4, 2025 OSC Colloquium: Jim Burge We have all heard the saying “If you cannot measure it, you cannot make it,” for optical fabrication, but it applies to most things where precision is required. The past decades have seen fantastic advancements in optical systems from astronomical telescopes that see to the edge of the universe to virtual reality systems that enable people to experience worlds that never exist. The new optical components and systems have required new ways to measure them.
Image 3:30 – 5 p.m., Oct. 2, 2025 OSC Colloquium: Hakan Tureci Recent strides in machine learning have shown that computation can be performed by practically any controllable physical system that responds to physical stimuli encoding data [1]. This perspective opens new frontiers for computational approaches using Physical Neural Networks (PNNs) [2, 3, 4] and provides a framework to deepen our understanding of their biological counterparts—neural circuits in living organisms.
Image 3:30 – 5 p.m., Sept. 25, 2025 OSC Colloquium: Stuart Shaklan One of NASA’s primary science goals is to directly image and characterize the atmospheres of Earth-like planets orbiting nearby stars. The observations are extremely challenging because the planets appear adjacent to their parent stars, near telescope diffraction limits, and their reflected light is 10 billion times fainter than the star. An elegant solution to this problem, first proposed by Lyman Spitzer in 1962, is to employ a starshade, a flower-shaped diffraction screen positioned far in front of a telescope so that it shadows the starlight without blocking the planet light.
Image 3:30 – 5 p.m., Sept. 18, 2025 OSC Colloquium: Vivishek Sudhir A pre-eminent problem of modern physics is to reconcile the disparity between the laws of quantum physics – which apply at the small scale – and the laws of gravity – that apply at the large scale. This talk will motivate the nature of the fundamental problem and highlight some of the ideas we are currently pursuing to address it. In particular, a decisive confrontation of gravity and quantum theory calls for mechanical objects, massive enough to measurably gravitate with each other, prepared in quantum states of their motion.
Image 3:30 – 5 p.m., Sept. 11, 2025 OSC Colloquium: Kyungtae Kim Optical atomic clocks now reach fractional frequency uncertainties below 10^-18, pressing toward a redefinition of the second. Optical lattice clocks harness laser cooling and trapping technologies for holding and probing ultracold atoms. These clocks are based on simple atomic spectroscopy, but as we continue zooming in to narrower frequency ranges, we encounter challenges that test our fundamental understanding of how atom-light and atom-atom interactions work, demanding cutting-edge laser stabilization and quantum state control.
Image 3:30 – 5 p.m., Sept. 4, 2025 OSC Colloquium: Jim Burge We have all heard the saying “If you cannot measure it, you cannot make it,” for optical fabrication, but it applies to most things where precision is required. The past decades have seen fantastic advancements in optical systems from astronomical telescopes that see to the edge of the universe to virtual reality systems that enable people to experience worlds that never exist. The new optical components and systems have required new ways to measure them.
