Constraints on Solar Axions Using the Profile Likelihood Ratio Method with the SuperCDMS Experiments
Subject Area
Physics
Abstract
Dark matter plays an essential role in understanding modern physics and particles beyond the Standard Model. Evidence suggests that dark matter accounts for approximately 85% of the universe’s matter, and 26.8% of its mass-energy composition. Key candidates for dark matter include unidentified subatomic particles like Weakly Interacting Massive Particles (WIMPs) and axions. The Super Cryogenic Dark Matter Search (SuperCDMS) employs direct detection methods to identify these elusive particles using cryogenic technologies. Su- perCDMS Soudan is the latest completed CDMS experiment in Minnesota, in preparation for the next phase experiments of SuperCDMS SNOLAB in Sudbury, Canada. At SNOLAB, the Cryogenic Underground TEst (CUTE) facility is dedicated to analyze background levels prior to the full operation of SuperCDMS SNOLAB experiments. Utilizing collected data from CDMSlite Run 3 at Soudan Underground Laboratory with minimized background interference, sensitivity limits were established for solar axions within the keV energy range using the profile likelihood ratio method. Our results show an axio-electric coupling constant constraints g_ae < 5.91×10^–11 from the atomic recombination and de-excitation, Bremsstrahlung, and Compton channels at a 90% confidence level.
Degree Date
Summer 8-6-2024
Document Type
Dissertation
Degree Name
Ph.D.
Department
Physics
Advisor
Jodi Cooley
Second Advisor
Joel Meyers
Acknowledgements
Through determination and hard work I was able to complete this long journey, but couldn't have done it without the support from my beloved family and friends.
Creative Commons License
This work is licensed under a Creative Commons Attribution-Noncommercial 4.0 License
Recommended Citation
Liu, Shilun, "Constraints on Solar Axions Using the Profile Likelihood Ratio Method with the SuperCDMS Experiments" (2024). Physics Theses and Dissertations. 19.
https://scholar.smu.edu/hum_sci_physics_etds/19