Francis Edwin Close (born 24 July 1945) is a particle physicist who is Emeritus Professor of Physics at the University of Oxford and a Fellow of Exeter College, Oxford.
From Oxford he went to Stanford University in California for two years as a Postdoctoral Fellow on the Stanford Linear Accelerator Center. In 1973 he went to the Daresbury Laboratory in Cheshire and then to CERN in Switzerland from 1973 to 1975. He joined the Rutherford Appleton Laboratory in Oxfordshire in 1975 as a research physicist and was latterly head of Theoretical Physics Division from 1991. He headed the communication and public education activities at CERN from 1997 to 2000. From 2001, he was professor of theoretical physics at Oxford. He was a visiting professor at the University of Birmingham from 1996 to 2002.
Close lists his recreations as writing, singing, travel, squash and Real tennis, and he is a member of Harwell Squash Club.
His 2010 book Neutrino discusses the Neutrino emitted from radioactive transitions and generated by stars. Also discussed are the contributions of John Bahcall, Ray Davis, Bruno Pontecorvo, and others who made a scientific understanding of this fundamental building block of the universe.
In The Infinity Puzzle: Quantum Field Theory and the Hunt for an Orderly Universe (2013), Close focuses on the discovery of the mass mechanism, the so-called Higgs-mechanism.
In his 2019 book, Trinity: The Treachery and Pursuit of the Most Dangerous Spy in History, Close recounts the life and the espionage of Klaus Fuchs who passed atomic secrets to the Soviets during the race for development of the nuclear bomb. He concludes that "it was primarily Fuchs who enabled the Soviets to catch up with Americans".
Other books include: Particle Physics: A Very Short Introduction , Antimatter and Nothing .
However, the existence of helium‑3 on the Moon was well established long before Close’s 2007 article. Apollo mission samples had confirmed the presence of solar-wind–implanted 3He in lunar regolith as early as the 1970s, with peer-reviewed publications reporting concentrations in the parts-per-billion range. For example, soil samples from Neil Armstrong's bulk sample 10084 from Apollo 11 was measured to contain approximately 11.8 ppb of 3He. By the early 2000s, remote sensing data from missions like Clementine and Lunar Prospector had been used to generate global models reaffirming the presence and distribution of helium‑3 in the lunar regolith, especially in mature, titanium-rich mare soils. Given the widespread availability of this data in the scientific literature, Close’s suggestion that “we don’t even know for certain if there is any helium‑3 on the Moon” was a significant misrepresentation. This assertion contradicts decades of well-documented lunar science.
In addition, tokamak experiments have in fact produced measurable D–3He fusion: JET reported non‑thermal D–3He fusion power of ~50–140 kW in the late 1980s–early 1990s and later pulses up to ~140 kW, using 3He as a minority species for ICRF heating.
Many of Close’s technical criticisms of helium‑3 fusion are supported by the scientific literature. It is widely accepted that deuterium–helium‑3 (D–³He) fusion is significantly more challenging to sustain than deuterium–tritium (D–T) fusion and that D–³He plasmas are not truly neutron-free. Side reactions, especially deuterium–deuterium fusion, inevitably produce tritium and neutrons, undermining claims of a “clean” process. In this respect, Close correctly challenged oversimplified narratives around lunar helium‑3 fusion.
However, Close overstated the extent of these challenges. Studies estimate that neutron production in optimized D–³He systems can be reduced to a small fraction of total fusion energy—far lower than in D–T fusion. His suggestion that using helium‑3 would effectively recreate a D–T machine overlooks this important distinction. Additionally, his claim that helium‑3 reactions produce deuterium was inaccurate; the standard helium‑3–helium‑3 fusion reaction produces two protons, not deuterium, consistent with well-established nuclear physics.
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