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Nuclear Energy Conference & Expo (NECX)
September 8–11, 2025
Atlanta, GA|Atlanta Marriott Marquis
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From operator to entrepreneur: David Garcia applies outage management lessons
David Garcia
If ComEd’s Zion plant in northern Illinois hadn’t closed in 1998, David Garcia might still be there, where he got his start in nuclear power as an operator at age 24.
But in his ninth year working there, Zion closed, and Garcia moved on to a series of new roles—including at Wisconsin’s Point Beach plant, the corporate offices of Minnesota’s Xcel Energy, and on the supplier side at PaR Nuclear—into an on-the-job education that he augmented with degrees in business and divinity that he sought later in life.
Garcia started his own company—Waymaker Resource Group—in 2014. Recently, Waymaker has been supporting Holtec’s restart project at the Palisades plant with staffing and analysis. Palisades sits almost exactly due east of the fully decommissioned Zion site on the other side of Lake Michigan and is poised to operate again after what amounts to an extended outage of more than three years. Holtec also plans to build more reactors at the same site.
For Garcia, the takeaway is clear: “This industry is not going away. Nuclear power and the adjacent industries that support nuclear power—and clean energy, period—are going to be needed for decades upon decades.”
In July, Garcia talked with Nuclear News staff writer Susan Gallier about his career and what he has learned about running successful outages and other projects.
Carl H. Distenfeld and Robert D. Colvett
Nuclear Science and Engineering | Volume 26 | Number 1 | September 1966 | Pages 117-121
Technical Paper | doi.org/10.13182/NSE66-A17194
Articles are hosted by Taylor and Francis Online.
The Special Measurements Group at the Brookhaven Alternating Gradient Synchrotron has conducted detailed experiments to evaluate and understand radiations emanating from the accelerator. As a part of this group study, skyshine and attenuation through Long Island sand was measured. Attenuation 90° from the apparent line source followed a half thickness of about one foot of sand through at least four decades. This corresponds to an attenuation length in sand of 80 g/cm2., Skyshine was measured out to 1000 m from the target. The empirical results fit the following expression for 4.2 × 1011 protons/sec on target: I = (3000/r2) exp(-r/600) [1 - exp(r/47)] where I is the dose rate in mrem/h and r is the source detector distance in meters. The source luminosity was determined, and a skyshine function was derived, based on the luminosity and the expected attenuation in air based on sand results. The empirical function was found to be within 25% of the derived expression.