Titus Pankey

Titus Pankey (November 20, 1925 – September 20, 2003)[1] was an American physicist and professor whose research specialties were magnetic susceptibility and cosmology, especially supernovas.

After graduation from high school, he worked as a Pullman porter on the Chesapeake & Ohio Railway, and helped to fund his four sisters' college educations.

[6] After completing his service, Pankey attended Howard University in Washington, D.C., as an undergraduate and graduated magna cum laude[7] with a degree in physics.

[8] His dissertation advisor was Herman Branson, and the title of Pankey's thesis was "Possible Thermonuclear Activities in Natural Terrestrial Minerals," submitted on 26 July 1961.

[11] Pankey's research was supported by the U.S. Geological Survey and Frank E. Senftle, and his advisory committee composed of Branson, Sohan Singh, Louis G. Swaby, and Stanton L.

[3][16][17] His hypothesis was not widely circulated and did not get immediate attention at the time, but would later be independently reinvented and developed in detail in a 1969 article by Stirling Colgate and Chester McKee.

The pair made significant contributions to molecular-beam epitaxy by demonstrating how to grow gallium arsenide films in vacuum chambers.

Pankey in the U.S. Naval Research Laboratory, circa 1964
Pankey in the U.S. Naval Research Laboratory, circa 1964
The radioactive decays of nickel-56 and cobalt-56 that produce a supernova visible light curve
The radioactive decays of nickel-56 and cobalt-56 that produce a supernova visible light curve