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Physical Sciences

Geochemical Analysis of Amphiboles at Mt Hillers, UT

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Author(s): Zoe Fischer, Parker Tenney, Chloe FitzGerald Taylor, Logan Chappell, Spencer Hahnem

Raman Imaging of Carbon Materials

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Author(s): Seth Stringham

The Stability of Isolated Bovine Milk Derived Extracellular Vesicles

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Author(s): Elley Colledge, McCoy Smith, Ian Cutler

Increased Efficiency in Nonlinear Wireless Power Transfer

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Author(s): Zachary Butler, Kendall Rosenkrantz, Yoonji Yo

Fluoride Speciation Analysis of the Great Salt Lake Utah

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Author(s): Danielle Kemmer, Dillon Reynolds, Alyssa Brown, Benjamin Judd, Dean V. Smith, Tyler Jenkins, Asha Ahmed, Amber Thornton Miller, Dylan Jenkins, Nashly Cruz-Guzman

Synthetic Routes for Norbornyl Derivatives

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Author(s): Brigham Warner, Chloe Adams

Student's perceptions on the use of Virtual Reality in organic and inorganic chemistry

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Author(s): Isabelle Smith, Alexandra Routsis, Laryssa Larson, Josie Wright, Kaden Jensen

Lensless High-Resolution Imaging with Laser Interference

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Author(s): Ulises Thornock, Brian Weaver, Jackson Phippen

Optical Scattering for Rapid UTI Detection

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Author(s): Feng Guo, Elise Bauer, Kimball Henstrom, Caroline Torgersen, Hannah Thrupp, Isaac Zabriskie, Alex Martinez, Keaton Fuller, Clint Flinders

A Preliminary Paleomagnetic Test for Incremental Pluton Emplacement

December 30, 0020 12:00 AM
Parsons, Travis; Lippert, Peter; Bartley, John (University of Utah)
Faculty Advisor: Lippert, Peter (University of Utah - College of Mines and Earth Science, Geology & Geophysics); Bartley, John (University of Utah - College of Mines and Earth Science, Geology & Geophysics)

Field observations and geochronological measurements of plutons in Yosemite Valley suggest that plutons grow incrementally as a series of stacked sheets of smaller intrusions (i.e., dikes and sills) (Coleman et al., 2004; Glazner et al., 2004; Bartley et al., 2006). This interpretation is in contrast to the traditional view of pluton emplacement through crystallization of a single, massive magma chamber. Most of the observations supporting incremental pluton emplacement use the relationship between zircon U-Pb dating of pluton sections and estimated granitic magma cooling rates to argue that a single magmatic event would crystallize significantly faster than the geochronologic data permit. Incremental pluton emplacement also predicts specific relationships between the age of intruded sheets of magma and the original orientation of these sheets, such that older sheets are expected to be tilted or deformed more than younger sheets. Here we test this prediction of differential tilting by measuring the paleomagnetic inclination preserved in well-dated and structurally characterized sheets of the Tuolumne Intrusive Suite. Magnetic inclination provides a tilt-meter with respect to the Earth's magnetic field direction at the time of pluton emplacement; the reference inclination assuming an untitled pluton is known from independent data sets. We also present rock magnetic data (temperature-dependent magnetic susceptibility, magnetic remanence characteristics) and results from petrographic investigations to characterize the mineralogy and stability of the magnetization. Our results suggest that the low-titanium magnetite remanence carriers are primary and are not biased by secondary magnetizations. The distribution of magnetic inclinations in our sample set — in which older sheets on the periphery of the pluton are shallower than those in younger, more interior sheets, and with respect to the reference inclination — is consistent with predictions from the incremental pluton emplacement hypothesis.

Binding Trends of simple hosts and guests with CB5, CB6, and Mc5

December 30, 0020 12:00 AM
Dearden, Heravi, Shen, Arslanian, Shrestha, Mismash, Tinsley, Pay (Brigham Young University)
Faculty Advisor: Dearden, David (Brigham Young University, Chemistry)

Using the Spartan and Ion Molecular Spectrometry Suite (IMoS), we use the 3D modeling to predict stability and molecule favorability. Previously in our experimentation we have seen and proper capping of a host molecule with cucurbit[5]uril. This was different than cucurbit[6]uril as the cap in some cases didn't bond to all the upward oxygens because on the molecular symmetry, thus host enclosure was less favorable in cucurbit[6]uril than cucurbit[5]uril. We also observed in our lab the energy differences using the Extensible Computation Chemistry Environment (ECCE) of cucurbit[5]uril host transfer based on cap and host interactions. These studies show that cucurbit[5]uril with methane as a host is more favorable than outside the cavity. It also shows that methane inside cucurbit[5]uril is more favored than in decamethylcucurbit[5]uril. The studies using computational study will be testable using mass spectrometry, and we predict that the same behavior trend will show using other caps and hosts with cucurbit[5]uril and decamethylcucurbit[5]uril.

The Power of Wind on Rock: Yardang Formation in Argentina

December 30, 0020 12:00 AM
Sevy, Jonathon; Radebaugh, Jani; McDougall, Dylan; Kerber, Laura; Rabinovitch, Jason (Brigham Young University)
Faculty Advisor: Radebaugh, Jani (Brigham Young University, Geology)

Yardangs are wind-carved linear ridges that are found selectively on Earth and extensively on Mars. The history of the morphologic development of yardangs is not well known. In the Puna high plateau of Argentina there are ignimbrite deposits, many of which have been eroded into yardang fields, commonly called fleets. Yarding fleets are evenly spaced forms, facing into the wind, that resemble a fleet of boats sailing. A prominent fleet, known as Campo de las Piedras Pomez (CCP) was studied to more fully understand their formation and morphology, including field research in December 2018 and 2019. Some physical characteristics looked at in the field included: dedos direction and lengths; heights and lengths of yardangs; structural features; wind and gravel ripple direction. In addition, relationships between yardang organization and structural control have been analyzed. The dedos on the fronts of yardangs averaged 4.0cm in length, while the reverse dedos were 3.3cm. From this it was determined that: Two wind directions, with one dominant, are present; Structural features can shape morphology of yardangs.

A Yarrowing Experience: The Tumor Inhibition and Toxicity of Utah's Native Achillea millefolium

December 30, 0020 12:00 AM
Parada, Michelle (Weber State University)
Faculty Advisor: Schramm, Katharina (Weber State University, Botany)

This research focuses on anti-tumor and the biotoxicity of A. millefollium (yarrow).
Yarrow is an interesting plant with a long history of medicinal uses, but very little has been done to research and prove the different beneficial properties claimed. There are two simple bench-top assays performed in this study, the potato disc assay which inoculates potato slices with Agrobacterium tumefaciens as well as different concentrations of yarrow extracts and assesses the resulting tumor formation and the brine shrimp toxicity assay to assess the LD-50 of the extracts. My results will indicate whether or not the native yarrow extracts inhibit or do not inhibit tumor formation and its toxicity level. The results of this research could lead to further studies of the phytochemicals in the plant to be used for cancer treatments.

An Aperture Correction for GeMS MCAO SBF Distance Measurements

December 30, 0020 12:00 AM
Sundstrom, Rebecca; Jensen, Joseph B. (Utah Valley University)
Faculty Advisor: Jensen, Joseph (Utah Valley University, Physics)

We will measure Surface Brightness Fluctuations (SBF) in three galaxies (ESO137-G006, NGC 3309, and NGC 5128) using images from two cameras: the GeMS Multi-Conjugate Adaptive Optics (MCAO) system and the FLAMINGOS-2 (F-2) near-infrared imaging spectrograph, at the 8-meter Gemini South Telescope in Chile. To make an accurate measurement we need to first determine a photometric calibration for the MCAO system by comparing flux, or captured light, from both detectors. This is necessary because MCAO collects crisp, sharp images but omits some of the total incoming flux from the stars in the galaxies. F-2 takes broader images but includes more measurable flux. By finding the ratio of the flux collected by MCAO to the flux collected by F-2 we can take this "missing" light into account without compromising the crisp, sharp resolution MCAO provides.

A Worldwide Phylogenetic Study of the Family Baetidae

December 30, 0020 12:00 AM
Backman, Natalia; Ogden, Heath (Utah Valley University)
Faculty Advisor: Ogden, Heath (Utah Valley University, Biology)

The Family Baetidae, is in the order Ephemeroptera, also commonly known as Mayflies. The first baetids were described around 1815 by Leach, and since there are more than 900 species have been described. The family Baetidae is an important group of mayflies because of their position on the mayfly tree of life in that they are a key to understanding evolutionary trends, such as the origin of wings and flight. Taxon sampling for this study consisted of over 100 taxa, representing ??? genera, from lineages distributed geographically worldwide, except Antarctica. Two main datasets were constructed. The genes 12s, 16s, H3, 18s, 28s and CO1 were used as part of a traditional dataset. Targeted capture sequencing was used to generate a phylogenomic dataset, consisting of over 400 loci. Trees were reconstructed from the aligned datasets, and the results were compared. The phylogenomic data resulted in a much more resolved topology.