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Taking Measure

Just a Standard Blog

Pushing the Quantum Limit in the Search for Dark Matter

Map of dark matter (in pink) in the universe

Map of dark matter (in pink) in the universe. 

Credit: Kilo-Degree Survey Collaboration/H. Hildebrandt & B. Giblin/ESO

Here’s a surprising fact: We don’t know what makes up 80 percent of the matter in the universe. I don’t mean that the matter is made of atoms, and we just don’t know which kind of atoms. What I mean is that four-fifths of the universe appear to be made of something that isn’t atoms at all, or more to the point, it’s not made from any of the fundamental particles that we know of.

Why do we think that this mystery matter exists? The short answer is that Albert Einstein’s theory of gravity, general relativity, has painted us into a corner. When we look through telescopes at stars and galaxies moving through the universe, something we can’t see is causing their motion to bend in a particular way. Einstein’s theory of gravity tells how much of this invisible mass—physicists call it “dark matter”—there must be to bend the trajectory of things we can see.

Faced with a situation like this, we make guesses (hypotheses) that we hope explain our strange observations. A good hypothesis should both be consistent with every known fact and have other detectable consequences. If we look for these other consequences and don’t find them, we discard or revise our hypothesis.

Superconducting axion detector
A close-up, taken with a scanning electron microscope, of our circuit that showed us where the microwave signals produced by certain kinds of dark matter weren’t. The superconducting Josephson junctions (in red) are what makes the detector sensitive enough for us to be confident that we didn’t overlook dark matter microwave signals in the frequency range where we looked. The square holes forming the “waffle” pattern are 5 microns on a side.
Credit: M. Malnou/NIST/JILA

Somewhat to my surprise, I find myself working on an experiment designed to look for the consequences of a hypothetical dark matter particle known as the axion. This was surprising because physicists, like those in all professions, divide themselves up into distinct sub-fields. Predictably there are rivalries between, and stereotypes associated with, different cultures that build up around the subfields—the rough equivalent of engineering versus sales in the corporate world.

My subfield is quantum physics. In my work, we construct devices that control and measure electricity (current and voltages), as well as quantum mechanics, will allow us. Quantum mechanics is a theory that describes the behavior of small things like individual atoms and their constituents, or larger man-made objects like electrical circuits if they are very cold. That’s quite far from cosmology, nuclear physics, and high energy physics, the usual domain of dark matter experiments. But one of the detectable consequences of the axion is that it can create an extraordinarily feeble electrical current oscillating at an unknown frequency somewhere between about 500 megahertz (MHz) and 500 gigahertz (GHz).

And it just so happens that measuring tiny microwave-frequency electrical signals is an experimental challenge that I have a deep affection for.

Indeed, for reasons unrelated to searching for axions, my NIST colleagues and I had constructed devices that measure microwave frequency signals in the range of 4 – 8 GHz. We were interested in understanding both how close a measurement could come to the limit imposed by quantum mechanics, which restricts the precision with which you can measure two complementary properties of a system, such as a particle’s position and direction of travel, at the same time, and to what degree that limit could be circumvented. Coincidentally, these devices had just the right properties to be used in an axion search apparatus called the HAYSTAC that was being constructed at Yale. In 2012, I entered into a collaboration with scientists from Yale, the University of California, Berkeley, and Lawrence Livermore National Laboratory to search for axions. Our role was to build the devices that would perform the delicate measurement of electrical currents at the quantum limit.

Close-up of Josephson junctions on axion detector
A zoom in on the Josephson junctions. Two layers of niobium are visible in the image, with the upper film colored blue and the lower film colored red. Josephson junctions are formed in the circular pits (they look a bit like an element of a muffin tin) where the two layers overlap (green).
Credit: M. Malnou/NIST/JILA

We just published the results of our preliminary search. Did we find an axion? No, but we found where it isn’t. In other words, we searched a range of possible frequencies for axion-induced currents sufficiently well to be confident that no axion signal will be found at these frequencies. That’s important because other scientists will design their experiments to search elsewhere.

Even so, the time required to search the whole frequency range is prohibitively long. In order to speed up this search, it will be necessary to somehow beat the limitations on electrical measurement imposed by quantum mechanics. Fortunately, because we know that quantum mechanics only limits certain types of simultaneous knowledge, in this case, the height of a wave’s peak (amplitude) and the time that the peak occurs (phase), we can modify our devices so that they only detect the amplitude or the phase of the oscillating current, but not both at the same time. Quantum mechanics doesn’t impose a limit on the sensitivity of a measurement of just one of these two quantities. My future work in the axion collaboration will be to deploy these beyond-quantum-limited measurements in the search apparatus.

When we can routinely detect electrical currents better than the quantum limit, we will begin observing many results that we could never have anticipated and potentially open the door to new physics—a very exciting prospect. I certainly never expected to find myself working in a nuclear physics collaboration, but in my line of work, it pays to keep an open mind and expect the unexpected!

About the author

Konrad Lehnert

Konrad Lehnert is a 1993 graduate of Harvey Mudd College. He received a Ph.D. from the University of California at Santa Barbara in 1999 and did post-doctoral research at Yale. In 2003 he joined JILA and NIST. He is known for his development of quantum-limited microwave amplifiers and for investigating the quantum physics of micro-mechanical structures. While at Harvey Mudd, Konrad ran track and cross country, and he still holds the school’s record for the slowest time in an official 5K race.

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"And it just so happens that measuring tiny microwave-frequency electrical signals is an experimental challenge that I have a deep affection for." : likewise, I'm personally fond of raising the Dead myself.
Where do you place your detectors?
Thanks for your question! The detectors are inside a device called the HAYSTAC, which resides at Yale University's Wright Lab.
There is a simple explanation for dark matter which is supposed to hold the outermost stars in the galaxies from being flung out into space. Rather its the galaxies magnetic field in total thats holding it all together. Every star is a powerful magnet with a large magnetic field,multipy that by 100/200 billion plus stars and the extremely powerful magnetic field of the black hole at the center and there you have it. People doing research on dark matter now are not doing science for science sake FFS! For a demonstration of the magnetic effect checkout YouTube ""Amazing discovery with magnets""
Konrad, Wish I had gone to Harvey Mudd. I could have easily defeated your 5K record and become immortalized.... Just one more regret in my life...

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