PHYS2022SHELTON16521 PHYS
Type: Undergraduate
Author(s):
Katelyn Shelton
Physics & Astronomy
Mia Bovill
Physics & Astronomy
Sachi Weerasooriya
Physics & Astronomy
Advisor(s):
Mia Bovill
Physics & Astronomy
Location: First Floor, Table 1, Position 2, 11:30-1:30
View PresentationThe first galaxies formed 12.5 billion years ago during the first billion years after the Big Bang. However, these first, faint, galaxies remain too faint for direct detection, even by our most powerful telescopes. Therefore we study them using their fossils relics, ultra-faint dwarf galaxies orbiting the Milky Way. In this work, we look at the histories of star formation in simulated analogs to the ultra-faint dwarfs. These star formation histories will allow us to study the details of how and when star formation occurred during the first billion years of cosmic time. We are particularly interested in how massive the first galaxies were when they formed the majority of their stars.
PHYS2022SINGARAVELAN46117 PHYS
Type: Undergraduate
Author(s):
Neha Singaravelan
Physics & Astronomy
Advisor(s):
Hana Dobrovolny
Physics & Astronomy
Location: Third Floor, Table 2, Position 1, 11:30-1:30
View PresentationCoinfection affects up to 60% of patients hospitalized influenza-like illnesses, however, the role of the innate immune response in coinfections is not understood. Interferons, part of the innate immune response, are a type of chemical released by infected cells that can help establish an antiviral state in cells by increasing resistance to infection and reducing production of viruses. Although the increased resistance to infection can help suppress both viruses, the reduction in the production of one virus may aid in increasing the growth of another virus during coinfection due to less competition. We will use a mathematical model to examine the interaction via interferons between respiratory syncytial virus (RSV) and influenza A virus (IAV) during coinfections. This model will measure viral titer, duration of the viral infection, and interferon production allowing us to understand how interferon production of one virus helps or hinders the secondary virus.
PHYS2022SPITTERS58954 PHYS
Type: Undergraduate
Author(s):
Benjamin Spitters
Physics & Astronomy
Advisor(s):
Hana Dobrovolny
Physics & Astronomy
Location: Second Floor, Table 5, Position 2, 11:30-1:30
View PresentationDue to the enormity of different forms of cancer and the increase in cancer rates globally, it is essential to continually develop more advanced methods of early and localized detection of cancer cells, as well as methods of targeted drug delivery. As a result, a vast amount of research has gone into the use of nano-materials such as graphene quantum dots (GQDs) as the basis for a wide variety of biomedical sensing and treatment applications. While many diagnostic biomarkers have been detected using modified GQDs, one biomarker that has not yet been successfully detected or targeted using GQDs is Transgelin-2. Transgelin-2 is a unique actin-binding protein that has been projected to be a useful biomarker and target of treatment for many different forms of cancer, as well as asthma and immune diseases such as lupus. Herein I review the structure of the Transgelin-2 protein, novel methods of GQD modification to sense cell membrane surface proteins, and ultimately determine the viability of GQDs as a method for detecting and targeting Transgelin-2. Furthermore, I develop a possible methodology by which these biophysical applications may be tested.
PHYS2022TZOKA35070 PHYS
Type: Undergraduate
Author(s):
Iakovos Tzoka
Physics & Astronomy
Advisor(s):
Hana Dobrovolny
Physics & Astronomy
Location: Basement, Table 1, Position 2, 1:45-3:45
View PresentationAntimicrobial action of micro- and nanoscale ZnO particles has been documented, but the fundamental physical mechanisms driving these actions are still not identified. We hypothesize that one of the key mechanisms behind the antibacterial action of ZnO is rooted in interactions between ZnO surfaces and extracellular material. An investigation was done of the biological components of that interaction using diffusion theory and more specifically Brownian motion computational models to look at the interaction of Zn+2 and O-2 ions with staphylococcus aureus bacteria. The analysis allowed us to find a correlation between the thickness of the staphylococcus aureus bacteria and the amount of the zinc and oxygen ions present in the solution.
PHYS2022TZOKA58785 PHYS
Type: Undergraduate
Author(s):
Iakovos Tzoka
Physics & Astronomy
Mark Hattarki
Physics & Astronomy
Riya Jadeja
Physics & Astronomy
Dustin Johnson
Physics & Astronomy
Daniel Lopez
Physics & Astronomy
John Reeks
Physics & Astronomy
Advisor(s):
Yuri Strzhemechny
Physics & Astronomy
Location: Third Floor, Table 9, Position 1, 11:30-1:30
View PresentationNano- and microscale zinc oxide (ZnO) have demonstrated potential for applications in electronic, pharmacological and chemical industries among others. At these scales, surface properties dominate, rendering surface defects highly influential. Consequently, understanding of defect- related phenomena are crucial to achieving impactful figures of merit. Many optoelectronic properties of ZnO relevant for applications have been linked to defect-related visible luminescence. Its fundamental origins are still being debated, with attributions to oxygen vacancies, zinc vacancies, oxygen antisites, donor-acceptor pairs, etc. In our studies, we contribute to this discussion by probing the relationship between crystal morphology and this luminescence. We conducted optoelectronic studies to characterize the effects of remote oxygen plasma treatment on hydrothermally-grown microscale ZnO samples with controlled morphology as a means to help elucidate the nature of the visible emission. We report on the observed changes in the photoluminescence spectra indicative of the relationship between surface defects, morphology, and electronic structure of ZnO.