\documentclass[11pt,a4paper]{article} \usepackage[utf8]{inputenc} \usepackage[]{lmodern} \renewcommand{\familydefault}{\sfdefault} \date{\today} \setlength{\topmargin}{-10mm} \setlength{\textwidth}{7in} \setlength{\oddsidemargin}{-8mm} \setlength{\textheight}{9in} \setlength{\footskip}{1in} \begin{document} \pagenumbering{gobble}% Remove page numbers (and reset to 1) \begin{center} \LARGE Statement of Research Interests\\ % \large % Nam Tran \end{center} \bigskip My work centers in an experimental search for charged lepton flavor violation (CLFV) with muons, namely the COMET experiment at J-PARC. COMET is a new experiment that aims to find the neutrinoless decay of muon to electron in a nuclear field, or muon to electron conversion, at a single event sensitivity of $10^{-17}$. The experiment has high impact as a positive result would provide an unambiguous evidence of new physics beyond the Standard Model (BSM); and a negative result will place stringent limits on theoretical models. The search is part of the Intensity Frontier in particle physics, which will provide a window to probe physics at energy scales far beyond the reach of the most powerful accelerator currently exists. I was inspired to join the COMET experiment because of its elegance: \begin{itemize} \itemsep-0.5em \item the overall idea is simple; \item the signal is clean and distinctive; \item and many novel technologies and solutions are needed to realize its goal. \end{itemize} % One issue had arisen in the preparation for COMET experiment is our knowledge % on the products of the nuclear muon capture process on aluminum target was not % sufficient. One issue that arose during the preparation for COMET is that our knowledge of the products of the nuclear capture process on aluminum was not sufficient. Protons are expected to be a significant source of hits in the tracking detector of COMET, but there was no direct measurement of the proton rate and spectrum in the relevant energy range. Neutrons could cause serious problem for the front-end electronics. Therefore, COMET and its counterpart, Mu2e at Fermilab, jointly carried out a series of measurements, in the so-called AlCap experiment, of the products emitted after nuclear muon capture on aluminum and titanium at Paul Scherer Institute (PSI), Switzerland. I did a Monte Carlo study that showed the feasibility of the experiment, and contributed to DAQ developement, and hardware and electronics works on silicon and germanium detectors. My initial analysis of proton data in 2013 showed that the proton emission rate is low enough for the tracking detector of COMET to operate normally. The smallness of proton emission rate was later confirmed by another independent analysis on a larger dataset. However, there are still discrepancies between the two analyses. Therefore we have had another run for the proton measurement in 2015. The data analysis for this run is ongoing. Since November 2014, I have been assigned as a subproject leader of COMET, responsible for monitoring the number of muons that stop in the muon stopping target. The number is evidently necessary for calculation of branching ratio and single event sensitivity of the experiment. There have been several ideas on how to achieve the goal: online measurement of muonic X-rays and delayed gamma rays from activated $^{27}$Mg; measurement of the spectrum of decay-in-orbit electrons, and the rate of protons emitted after nuclear muon capture. I have proposed another activation measurement: measure population of a long-lived activation product, namely $^{24}$Na ($T_{1/2} = 14.96$~h). The measuring scheme will be: \begin{itemize} \itemsep-0.5em \item irradiation with muon beam for 2 days, \item beam off, \item measure delayed gammas from $^{24}$Na (1368 and 2574 keV) for 2 hours, \item continue irradiating, then repeat the cycle. \end{itemize} All these methods could be used simultaneously for cross-checking and reducing systematic uncertainties. % I also involve in other works, such as Monte Carlo simulation of cosmic ray % background in COMET Phase-I, and magnetic field map calculation for both COMET % Phase-I and Phase-II. Having been working in COMET for 5 years, I have been able to work together with great collaborators, and have gained a wide range of skills needed for an experimental physicist, including simulation, detector development, data acquisition, and data analysis. Now I would like to broaden my perspective and earn more experience by joining the Muon $g-2$ experiment. I am attracted by the ambitious goal of measuring the muon anomalous magnetic moment at an unprecedented precision, its impact of the measurement in establishing a signal for new physics beyond the Standard Model, as well as the synergy between $g-2$ and $\mu-e$ conversion experiments. My areas of contribution could be Monte Carlo simulation, detector and DAQ development. Besides, I am eager to learn new skills including accelerator-related techniques, FPGA development, and data analysis using machine learning. % moving to another position. % The % transition to Mu2e would be smooth since the two % experiments have many things in common. % Personally, I would like to strengthen % my data analysis skill with a new technique: machine learning. I believe % machine learning will be used extensively as I continue working in the % Intensity Frontier. \end{document}