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Scepticism greets pitch to detect dark energy in the lab

Give it a whirl: could a simple test detect energy that, so far, has only been measured by cosmologists? Credit: J. NEWMAN/UCB & NASA

A cosmic force that is thought to drive the accelerating expansion of the Universe could be probed using desktop electronics, two researchers have claimed.

The force — usually known as dark energy — seems to oppose gravity, making galaxies fly apart with increasing speed. Detected eight years ago, it presents one of the biggest puzzles in cosmology.

But we may not need high-powered telescopes to study it, according to Christian Beck, a mathematical physicist at Queen Mary, University of London, and mathematical biologist Michael Mackey of McGill University in Québec (C. Beck & M. C. Mackey, preprint at; 2004).

They say that noise found in a commonplace electronic device could be the fingerprint of dark energy. If it is, they predict this noise will fall quiet above a well-defined frequency. The idea has yet to be tested.

Other researchers are sceptical, however. “The paper is intriguing,” says physicist Peter Milonni of the Los Alamos National Laboratory in New Mexico, “but I think it would be a bit of a stretch to say that it holds water.”

Cosmologist Robert Caldwell of Dartmouth College in Hanover, New Hampshire, applauds the idea of lab tests but says that for this one to work, “it would have to violate things we already know to be true”.

Dark energy is estimated to account for nearly three-quarters of all the energy in the Universe — but no one really knows what it is or where it comes from. One possible source is a buzzing of empty space known as vacuum fluctuations. Quantum theory implies that a vacuum is constantly fizzing with particles that pop in and out of existence. Scientists assume that a natural mechanism cancels out the energy this produces, but some wonder if a little survives to give rise to dark energy.

The effects of vacuum fluctuations can show up in the lab. For example, they make two parallel plates separated by a vacuum attract one another, a phenomenon called the Casimir effect. They are also believed to account for some of the noise in Josephson junctions, devices in which an insulating layer is sandwiched between two superconductors.

If vacuum fluctuations are responsible for dark energy, say Beck and Mackey, then the energy density of these fluctuations should be the same as the density of dark energy that has been calculated from astronomical observations.

Calculating the energy density in Josephson-junction noise means adding up the energy at all frequencies. So far, measurements have been made up to almost a trillion hertz. They already give a density that is about equal to cosmological estimates for dark-energy density. So, Beck and Mackey argue, energies at higher frequencies should drop to zero. If that does not happen, they say, we should be looking elsewhere to explain dark energy.

Caldwell says the idea has already been disproved through lab studies of the Casimir effect at very high frequencies, in which no cut-off was observed.

Beck counters that previous estimates of vacuum fluctuations are theoretical, but the Josephson-junction approach offers a direct physical measurement. “The experiment would be cheap and easy to do,” he says.


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Ball, P. Scepticism greets pitch to detect dark energy in the lab. Nature 430, 126 (2004).

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