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University of South Carolina

Search For Solar Axions

Abstract

dc:description.abstract

<p> Peccei and Quinn proposed an elegant solution for restoring CP symmetry to the QCD Lagrangian \cite{PhysRevD.16.1791}. This method includes an additional global U(1) symmetry included in the QCD Lagrangian which is spontaneously broken at a high energy scale, f<sub>a</sub>. Breaking the symmetry generates a Nambu-Goldstone boson called the axion. Although there are various detection mechanisms that search for the axion, this thesis focuses on the the axio-electric effect. The axio-electric is similar to the photo-electric effect in that an axion is absorbed by an atom which subsequently emits an electron. The electron's energy is equivalent to the incoming axion energy minus the binding energy. The higher shell electrons immediately replenish the missing binding energy yielding a single energy peak at the incoming axion's energy. The 14.4 keV M1 transition of <super>57</super>Fe is one possible axion source. The development of an optimum trigger algorithm has lowered the threshold for analysis in TeO<sub>2</sub> bolometers to a few keV making an axion signature accessible to CUORE related R&D experiments such as the Chinese Crystal Validation Runs (CCVR) and Three Towers Test (TTT). These TeO<sub>2</sub> crystal detectors have masses 750 and 790 grams, respectively. Each crystal has a stabilization heater and a germanium thermometer attached to its surface by an epoxy glue. The two previous experiments are R&D tests for the upcoming larger experiment, CUORE. CUORE will be made of 988 TeO<sub>2</sub> crystals arranged in 19 towers with 13 floors each, each floor with 4 detectors. This thesis examined 87.01 kg&middot;days of Three Towers data for an axion signal. A peak is observed in the region of interest with a statistical significance less than 1&sigma; over the expected background fluctuations, yielding a total background rate of 0.185 &plusmn; 0.001 (Stat.) &plusmn; 0.006 (Syst.) Counts/kg/day at 95% C.L. This places an experimental limit on the coupling constant f<sub>a</sub> of $f<sub>a</sub> (S = 0.50)&ge;1.16\times10<super>6</super> GeV at 95% C.L. Projecting the TTT result to the CUORE mass and a five year run time we can expect a limit of $f<sub>a</sub>(S = 0.50)&ge;2.21\times10<super>6</super> GeV at 95% C.L. Improvements in granularity can strengthen the bound on $f<sub>a</sub> by 8% and 25% for background reductions by a factor of 2 and 10, respectively.</p>

Degree

thesis:*
Name thesis:degree_name
Ph.D.
Level thesis:degree_level
Campus Access Dissertation
Discipline thesis:degree_discipline
Physics and Astronomy
Year
2011

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Newman, Seth
Contributors dc:contributor
  • Frank T Avignone

Subjects

dc:subject × 4

Rights

dc:rights
Statement dc:rights
  • © 2011, Seth Newman

Identifiers

dc:identifier.*
Repository record dc:identifier
https://scholarcommons.sc.edu/etd/1758
OAI identifier oai:identifier
oai:scholarcommons.sc.edu:etd-2759

Chain of custody

source
Harvested from
University of South Carolina
Base URL
scholarcommons.sc.edu/do/oai/
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
citation

Newman, Seth. Search For Solar Axions. Campus Access Dissertation thesis, 2011. https://scholarcommons.sc.edu/etd/1758