News and Events

Wed, Sep 16, 4:00 PM (C215 ESC, and online)
The Sound of Speed: Rocket Launch Noise, Sonic Booms, and Explosions

Although high-speed turbulent jets have been studied since the 1950s, predicting the sound they produce remains a challenging problem in physics. In the BYU Physics and Aerospace Student-Centered Acoustics Laboratory (PASCAL), we investigate aircraft and rocket noise, asking age-old questions important to both physics and philosophy: Where does it come from? What makes it unique? Where is it going? Why does it matter?

In this presentation, I’ll discuss recent PASCAL research on rocket noise, including cases when things go right (launch noise and sonic booms) and when they don’t (explosions). We’ll talk about how these sounds affect structures, humans, and wildlife. I’ll also share lessons from measurement successes and failures, as well as from engaging with government officials, the media, and local communities.

What does this image look like to you? Many see a giraffe facing right, with neck stretched high and long legs mid-stride (but some may see a squirrel instead). The featured image shows LDN 1295, also called the Giraffe Nebula, in the constellation of the mythical queen of Aethiopia (Cassiopeia). It is an object in the Lynds Catalogue of Dark Nebulas, compiled in 1962 by American astronomer Beverly Lynds, a pioneer for women in astronomy and astrophysics. Dark nebulas are interstellar clouds of dust and gas that block the visible light of the stars behind them. These nebulas are often faint and challenging targets for astrophotographers. Why do we see animal shapes and faces in nebulas, clouds, and pretty much everywhere? It is due to pareidolia, our tendency to look for familiar patterns. Pareidolia may provide animals with an evolutionary advantage, for example in identifying (and avoiding) predators. APOD's main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod
Temp:  67 °FN2 Boiling:75.9 K
Humidity: 32%H2O Boiling:   368.5 K
Pressure:86 kPaSunrise:7:04 AM
Wind:1 m/s   Sunset:7:43 PM
Precip:0 mm   Sunlight:0 W/m²  
Brian Anderson and his students celebrated BYU's 150th birthday by blowing out candles using high-intensity focused sound waves.
John Ellsworth received the 2025 President's Appreciation Award for his work in the Department of Physics and Astronomy.
Get a deeper look into what has been happening at the New Microscopy Facility

Selected Publications

Devin M. Lewis, Tanner D. Rydalch, and David D. Allred (et al.)

We describe efforts to develop broadband mirror coatings with high performance that will extend from the far-ultraviolet (FUV) to infrared wavelengths. Our team at the Goddard Space Flight Center has developed a reactive physical vapor deposition (rPVD) process that combines a fluorination with a XeF2 gas (which grants a thin AlF3 layer) in between the Al and the metal-fluoride protection layer (either LiF or MgF2) that are done with the conventional PVD process. This recently developed rPVD process produces protected Al mirrors coatings with an improved average FUV reflectance between 10% and 15% higher (when compared with conventionally prepared samples). We have termed these coatings as XeLiF when the dielectric overcoat is LiF or XeMgF2 when the dielectric overcoat is MgF2. The XeLiF-coated Al mirrors meet current goals for advanced broadband mirrors in the FUV (R>70% at 103 nm and R>80 above 110 nm), whereas the XeMgF2 provides R>80% above 115 nm. The IR/Vis/UV reflectance for either XeLiF or XeMgF2 mirrors is similar to the theoretical reflectance of bare aluminum at wavelengths >200 nm. In addition, long-term lifetime testings of XeLiF mirrors indicate the rPVD process produces more environmentally stable coatings, where a XeLiF sample showed a degradation in the average FUV reflectance of around 1% to 2% when stored in a relative humidity of 40% over a period of 3.5 years. These results are a remarkable improvement when compared with conventionally prepared Al+LiF samples that would degrade their FUV reflectance in a matter of weeks or months when exposed to those kinds of relative humidity levels. Surface topographies on several XeLiF samples with varying Al and LiF thicknesses have been measured with an atomic force microscope (AFM). The root mean square (RMS) roughness (σ) values derived from these AFM results have ranged between 0.6 and 0.9 nm. For comparison, samples without the Xe process start off by having an RMS roughness that is 30% larger than samples treated with the XeF2 gas. We have also determined that these roughness values are showing a slight increase, ranging between 0.9 and 1.0 nm, when samples are exposed to room temperature and relative humidity as high as 50% over one week. Both of these key performance parameters (environmental stability in reflectance and smoothness of ≤1 nm) are key considerations for using the XeLiF coating in the primary and secondary mirrors of the Habitable Worlds Observatory (HWO). We also show evidence that the rPVD coating process is compatible with deposition on Si-based gratings. It is known that XeF2 vapor is a strong Si etchant, thus the demonstration that the native SiO2 layer on Si test samples is sufficient to protect the groove profile of E-beam-ruled Si gratings from degradation is an important and significant finding.

Spencer Gardiner, Daniel H. Ess, and Dennis Della Corte (et al.)

Computational enzyme design remains a powerful yet imperfect tool for optimizing biocatalysts, especially when targeting non-natural substrates. Using design tools we investigated Pseudomonas aeruginosa LipA, a lipase with a flexible lid domain crucial for substrate binding and turnover, aiming to enhance its hydrolysis of the industrially relevant substrate Roche ester. We generated an initial set of single-point mutations based on structural proximity to the active site and evaluated their effects using a computational pipeline integrating molecular dynamics (MD) simulations, density functional theory (DFT) calculations, and ensemble-based energy scoring. While we identified several active variants, attempts to rank them by activity using structural features, such as hydrogen bond formation or residue flexibility, failed. Deep learning models, applied post hoc for structural analysis via AlphaFold3, produced nearly identical active site geometries across variants, irrespective of activity. Reaction pathway analysis revealed energy barriers varying by 5–15 kcal/mol depending on substrate conformation, with the nucleophile addition step consistently rate-limiting. However, these small energetic shifts, likely critical for incremental activity changes, were indistinguishable by current computational or deep learning methods. Our results highlight the limitations of existing approaches in resolving subtle functional differences and underscore the need for improved benchmarks, reactive force fields, and more sensitive ranking metrics. Advancing these areas will be essential for designing enzymes with gradual, evolution-like activity improvements and for bridging the gap between structural prediction and catalytic function.

We provide experimental evidence for the absence of a magnetic moment in bulk RuO2, a candidate altermagnetic material, by using a combination of Mössbauer spectroscopy, nuclear forward scattering, inelastic X-ray and neutron scattering, and density functional theory calculations. Using complementary Mössbauer and nuclear forward scattering, we determine the Ru magnetic hyperfine splitting to be negligible. Inelastic X-ray and neutron scattering-derived lattice dynamics of RuO2 are compared to density functional theory calculations of varying flavors. Comparisons among theory with experiments indicate that electronic correlations, rather than magnetic order, are key in describing the lattice dynamics.

Hanna M. Pavill and Micah R. Shepherd

The glockenspiel is a bright, resonant percussion instrument with a series of simple bars mounted next to each other in a frame. Its acoustic radiation remains underexplored, particularly in its full instrument configuration. This study investigates the acoustic radiation and vibrational behavior of a glockenspiel bar in different mounting conditions. Directivity measurements and the scanning laser Doppler vibrometer were used to compare a single bar in free-free, baffled, and full-instrument configurations. The results show that the mounting significantly alters radiation patterns of the bar, particularly at higher modes. Torsional modes exhibited greater deviation from free-free predictions than bending modes, especially in the full-instrument case. The findings highlight the importance of considering frame and structural interactions in modeling glockenspiel vibration and radiation.

Aiden V. Harbick and Mark K. Transtrum

Modern superconducting radio frequency (SRF) applications demand precise control over material properties across multiple length scales—from microscopic composition, to mesoscopic defect structures, to macroscopic cavity geometry. We present a time-dependent Ginzburg-Landau (TDGL) framework that incorporates spatially varying parameters derived from experimental measurements and ab initio calculations, enabling realistic, sample-specific simulations. As a demonstration, we model Sn-deficient islands in Nb3Sn and calculate the field at which vortex nucleation first occurs for various defect configurations. These thresholds serve as a predictive tool for identifying defects likely to degrade SRF cavity performance. We then simulate the resulting dissipation and show how aggregate contributions from multiple small defects can reproduce trends consistent with high-field 𝑄-slope behavior observed experimentally. Our results offer a pathway for connecting microscopic defect properties to macroscopic SRF performance using a computationally efficient mesoscopic model.

J. Peatross, S. Kunzler, S. Christiansen, and M. Ware


It has been known for decades that microscopic dust particles can become trapped near the focus of a continuous laser beam when surrounded by ambient gas such as air. In this photophoretic interaction, the laser heats the particle, which interacts with surrounding gas molecules. Trapped particles typically scatter significant laser light as they are suspended in midair and can be easily observed from the side of the beam. We report on the first on-axis images of photophoretically trapped particles together with the laser-beam profile responsible for the trapping. The radial structure of the laser is recorded using 1:1 imaging, where the 1 W beam must be strongly attenuated without introducing distortion. The trapped particle is weakly illuminated using a different wavelength, chosen to transmit through the filters used to attenuate the laser.