PHYS2022RIDDLE53019 PHYS
Type: Undergraduate
Author(s):
Nicole Riddle
Physics & Astronomy
Emilie Burnham
Physics & Astronomy
Natalie Myers
Physics & Astronomy
Advisor(s):
Peter Frinchaboy
Physics & Astronomy
Location: Second Floor, Table 6, Position 3, 11:30-1:30
View PresentationThe creation and evolution of elements throughout time across the Milky Way disk provides a key constraint for galaxy evolution models. To provide these constraints, we are conducting an investigation of the zirconium, neodymium, cerium, and barium abundances created in supernovae explosions, for a large sample of open clusters. The stars in our study were identified as cluster members by the Open Cluster Chemical Abundance & Mapping (OCCAM) survey that culls member candidates by Doppler velocity, metallicity, and proper motion. We have obtained new data for the elemental abundances in these clusters using the Subaru Observatory 8-m telescope in Hawaii with the High Dispersion Spectrograph (HDS). Analyzing these neutron-capture abundances in star clusters will lead us to new insight on star formation processes and the chemical evolution of the Milky Way galaxy.
PHYS2022SHARMA27774 PHYS
Type: Undergraduate
Author(s):
Manya Sharma
Physics & Astronomy
Advisor(s):
Hana Dobrovolny
Physics & Astronomy
Location: Second Floor, Table 5, Position 1, 1:45-3:45
View PresentationCancer is a leading cause of death worldwide with around one in every six caused by cancer, but many cancers can be cured if treated properly. Mathematically programmed cancer cell models can be used by researchers to study the use of oncolytic viruses to treat tumors. With these models, we are able to help predict the viral characteristics needed in order for a virus to effectively kill a tumor. Our approach uses both cancerous and non cancerous cells in relationship to the tumor to determine the speed at which the cells replicate, however there are several models used to describe cancer growth, including the Exponential, Mendelsohn, Logistic, Linear, Surface, Gompertz, and Bertalanffy. We study how the choice of a particular model affects the predicted outcome of treatment.
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.