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Hydrogen made with muons reveals proton size conundrum

The proton accelerator at the Paul Scherrer Institute, which was used to create the muons used in this experiment.

How big is a proton? Unlike an electron or neutrino, which are fundamental particles that behave like points, a proton is a messy collection of quarks, gluons, and virtual particles that occupies what should be a measurable amount of space. And just how much space can be rather significant; as the authors of a new paper on the proton's size put it, "The proton structure is important because an electron in an S [ground] state has a nonzero probability to be inside the proton." (Emphasis ours.)

And, within experimental error, various measurements of the proton's size have all put it about 0.88 femtometers (an fm is 10-15 meters). But a team of researchers, working at a particle accelerator in Switzerland, has found a different way of measuring the proton's size: put a muon—a heavy, unstable, relative of the electron—in orbit around a proton. The resulting atom, called muonic hydrogen, can be measured during the brief time it exists before the muon decays. Those measurements have produced a new, very high-precision value for the proton's radius. Just one small problem: it differs from the other measurements by nearly seven standard deviations.

The paper describing these measurements, published in today's Science, does a nice job of illustrating how measuring the emissions of simple hydrogen atoms has a profound effect on physics. The fact that hydrogen only emits or absorbs specific frequencies as its electrons hop between orbitals was critical to the development of quantum mechanics. Better precision measurements revealed that many of these absorption or emissions lines were actually two closely spaced frequencies; that provided experimental validation of the Dirac equation. Small deviations from this equation eventually helped trigger the development of quantum electrodynamics.

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Where are our fuel cell cars?

Hyrogen-powered Chevrolet Equinox Fuel cell vehicle, with a range of 200 miles.

Fuel cells are the dream power source for vehicles: they can use hydrogen and oxygen as fuel and oxidizer, respectively, and produce only electricity and water (plus a little heat). Compared to battery-powered electric vehicles, hydrogen-powered fuel cell vehicles offer higher energy density, which leads to greater range and lower weight. Sure, they have their downsides—such as requiring a complete hydrogen infrastructure à la oil pipelines and fueling stations—but batteries vs. fuel cells is a debate for another day (and story).

The first hydrogen fuel cell vehicle (General Motors/Chevy Electrovan) was created in 1966. Researchers have been developing proton exchange membrane (PEM) fuel cells for past 15 years. So why don’t we see any in cars on the road? In a word: catalysts. Despite intense development, catalysts used in PEM fuel cells haven’t reached the levels of performance, lifetime, or cost to be commercially viable. In a recent issue of Nature, Mark Debe, senior scientist in the Fuel Cell Components Program at 3M, summed up the recent progress and prospects for fuel cell catalysts, including potential manufacturing issues.

The basics

First off, what is a catalyst? How does a fuel cell even work? What is the air-speed velocity of an unladen swallow? (African or European?) One question at a time, please.

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Voyagers travel far enough to see our own galaxy without the Sun’s interference

Hydrogen is the most abundant gas in the Universe, and provides important clues about its properties. The cosmic microwave background was created through interactions with ionized hydrogen, and emissions from hydrogen ions help us identify energetic events like star formation. They do, that is, if the events are far enough away. Ironically, the Universe conspires to keep us from seeing events in our own galaxy. Or, more accurately, the Sun has kept us from seeing them until very recently, when the Voyager probes finally got far enough from the Sun to see what our galaxy is up to.

Hydrogen's lone electron normally resides in the ground state, but various energetic events can move it to higher states. Two types of emission result from these processes. Balmer-alpha occurs when the electron drops from the second excited state to the first (and has nothing to do with Steve or thrown chairs). Lyman-alpha emissions occur when the electron drops from the first excited state back to the ground. The Lyman emissions, which occur in the UV, rarely reach us directly. There's so much hydrogen out there that it's often absorbed and re-emitted multiple times before getting very far from its source.

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