JILA Auditorium

Quantum limits to precision measurement

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Continuous-wave (CW) interferometers and oscillators lie at the core of many modern precision measurements including atomic clocks and ground and space based gravitational wave detectors. As with all measurements, quantum mechanics sets the ultimate limit on the precision of these devices. In interferometers employing only classical sources of light, such as thermal sources and lasers, sensitivity is bounded by “standard quantum limit” (SQL) scaling.

Improved quantum control of two-dimensional ion crystals in a Penning trap

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Two-dimensional crystals of trapped ions in a Penning trap have enabled advances in quantum simulation and precision measurement. Because the crystal rotates at ~180 kHz, previous experiments were limited to global interactions, and poor cooling of in-plane motion reduced experimental fidelity. In this defense, I describe using a deformable mirror (DM) to apply patterned spin rotations in the rotating frame of the crystal.

Deciphering Hydrogen-Bonding Signatures as Molecular Fingerprints: Cryogenic Ion Vibrational Spectroscopy of Anion-Receptors and Biomarkers

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Abstract: Understanding the fundamental interactions that influence molecular recognition is essential for advancing applications in drug design, sensing, and materials chemistry. This dissertation uses cryogenic ion vibrational spectroscopy (CIVS) to investigate noncovalent interactions in anion-receptor complexes by studying mass-selected gas-phase ions at cryogenic temperatures, eliminating complexities due to solvation effects.

Taming the New Zoo of Exotic Heavy Hadrons

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Abstract: A new zoo consisting of dozens of heavy subatomic particles that contain more than three quarks and antiquarks have been discovered beginning in 2003.  Although they must be described by the fundamental quantum field theory QCD, the pattern of these exotic heavy hadrons remained unexplained for more than 20 years.  I will present a simple proposal for the pattern based on the Born-Oppenheimer approximation for QCD.  There are simple calculations in lattice QCD that would corroborate the pattern.

The 229-Th nuclear optical clock - Current status and future applications

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The year 2024 was a breakthrough year towards the development of a nuclear optical clock, with three experiments reporting success in the laser spectroscopy of the lowest nuclear excited state of 229-Th. The highest accuracy was achieved at JILA via direct frequency comb spectroscopy of this, previously elusive, nuclear state. This success is the result of several decades of effort to precisely determine the transition energy and a first step towards nuclear precision spectroscopy and the development of a nuclear frequency standard of extremely high accuracy.

Blazing the Trails to Habitable Planets: Over the Experimental > Mountains and Across the Observational Deserts

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Abstract: The discovery of thousands of planets orbiting stars beyond the solar system has fundamentally shifted our view of Earth’s place in the Universe, has captivated the public imagination, and has transformed research priorities in astrophysics. We are now actively searching for atmospheres on temperate, terrestrial planets, and are developing the technical tools to find and characterize “Earth-2.0”.

No Fireworks: Black Hole Radiation Builds Gradually

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Abstract: This talk will explore how quantum radiation - known as Hawking radiation – emerges when a black hole forms in the gravitational collapse of a star. While it has long been known that black holes emit energy, its precise origin has been debated. Over the decades, some researchers proposed that this energy is released directly from the collapsing star, producing a sudden burst that may potentially disrupt the collapse.

Laboratory Measurements of Asteroid Fragmentation

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Abstract: The scales of asteroid strength, from centimeters to tens of meters or more, can in principle be connected via the well-known Weibull theory (Weibull 1951) that explains in probabilistic terms why small samples of a rock are stronger than the whole. There are fewer weak flaws to be exploited in a smaller sample. This leads to a statistical understanding of size-dependent strength that has been implemented in fragmentation and damage models for planetary materials (Melosh et al., 1992; Benz and Asphaug 1994, 1995). The Weibull analysis enabled Cotto-Figueroa et al.

What can the Standard Model actually predict?

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Abstract: The most basic requirement of a scientific theory is that it make predictions. Is the Standard Model a scientific theory? As the well-tested, reigning theory of the elementary particles and fundamental forces, the Standard Model certainly claims to be able to predict the outcomes of a wide range of experiments. Yet from inelastic nuclear scattering, to neutron stars and superconductors, the universe is filled with systems whose behavior should be predicted by the Standard Model, but for which no such predictions are forthcoming!