Heavens

Laser-heated nanowires produce micro-scale nuclear fusion

image: This is the target chamber (front) and ultra-high intensity laser (back) used in the micro-scale fusion experiment at Colorado State University

Image: 
Advanced Beam Laboratory/Colorado State University

Nuclear fusion, the process that powers our sun, happens when nuclear reactions between light elements produce heavier ones. It's also happening - at a smaller scale - in a Colorado State University laboratory.

Using a compact but powerful laser to heat arrays of ordered nanowires, CSU scientists and collaborators have demonstrated micro-scale nuclear fusion in the lab. They have achieved record-setting efficiency for the generation of neutrons - chargeless sub-atomic particles resulting from the fusion process. Their work is detailed in a paper published in Nature Communications, and is led by Jorge Rocca, University Distinguished Professor in electrical and computer engineering and physics. The paper's first author is Alden Curtis, a CSU graduate student.

Laser-driven controlled fusion experiments are typically done at multi-hundred-million-dollar lasers housed in stadium-sized buildings. Such experiments are usually geared toward harnessing fusion for clean energy applications.

In contrast, Rocca's team of students, research scientists and collaborators, work with an ultra fast, high-powered tabletop laser they built from scratch. They use their fast, pulsed laser to irradiate a target of invisible wires and instantly create extremely hot, dense plasmas - with conditions approaching those inside the sun. These plasmas drive fusion reactions, giving off helium and flashes of energetic neutrons.

In their Nature Communications experiment, the team produced a record number of neutrons per unit of laser energy - about 500 times better than experiments that use conventional flat targets from the same material. Their laser's target was an array of nanowires made out of a material called deuterated polyethylene. The material is similar to the widely used polyethylene plastic, but its common hydrogen atoms are substituted by deuterium, a heavier kind of hydrogen atom.

The efforts were supported by intensive computer simulations conducted at the University of Dusseldorf (Germany), and at CSU.

Making fusion neutrons efficiently, at a small scale, could lead to advances in neutron-based imaging, and neutron probes to gain insight on the structure and properties of materials. The results also contribute to understanding interactions of ultra-intense laser light with matter.

Credit: 
Colorado State University

Movable silicon 'lenses' enable neutrons to see new range of details inside objects

image: The neutron interferometer can scan the interior of thick objects, such as this chunk of granite, providing enough detail to show the four types of rock that are mixed within it.

Image: 
Huber & Hanacek, NIST

You can't see well without lenses that can focus, whether those lenses are in your eye or the microscope you peer through. An innovative new way to focus beams of neutrons might allow scientists to probe the interiors of opaque objects at a size range they were blind to previously, allowing them to explore the innards of objects from meteorites to cutting-edge manufactured materials without damaging them.

The method, published today in Physical Review Letters, could convert what historically has been a support tool for neutron science into a full-fledged scanning technique that could reveal details ranging in size from 1 nanometer up to 10 micrometers within larger objects. The approach provides this tool, known as neutron interferometry, with what are essentially its first movable "lenses" capable of zooming in and out on details in this size range -- a range that has been difficult to probe, even with other neutron scanning methods.

More precisely, these "lenses" are silicon wafers acting as diffraction gratings, which take advantage of neutrons' wavelike properties. The gratings split and redirect a neutron beam so that the waves bounce off an object's edges and then collide with one another, creating a visible moiré interference pattern representative of the object that is easy for experts to interpret.

The method was developed by a team of researchers from the National Institute of Standards and Technology (NIST), the National Institutes of Health (NIH), and Canada's University of Waterloo. According to NIST's Michael Huber, the approach could make neutron interferometry into one of the best exploratory tools in a material scientist's kit.

"We can look at structure on lots of different levels and at different scales," said Huber, a physicist with NIST's Physical Measurement Laboratory who conducts experiments at the NIST Center for Neutron Research (NCNR). "It could complement other scanning techniques because its resolution is so good. It has a dramatic ability to focus, and we aren't limited to looking at thin slices of material as with other methods--we can easily look inside a thick chunk of rock."

Interferometry is a specialty in the world of neutron science. Before scientists can probe an object's interior with a neutron beam, they must first possess a few fundamental details about how the neutrons will bounce off the object's atomic structure. One of those details is a substance's index of refraction, a number indicating how much it will bend the beam from the direction it is traveling. (Water bends light in a related fashion--that's why your arm looks like it bends away when you dip it into a swimming pool.) Neutron interferometry is the best way to obtain that crucial measurement.

Neutron interferometry also has potential for other uses in fundamental physics, such as accurately measuring the gravitational constant. It's sensitive enough to detect how an object's gravitational force can deflect neutrons, just as the Earth attracts a flying ball (and vice versa). But the neutron method's Achilles' heel has been how slowly it works. To focus neutrons on a sample of material, an interferometer has needed a crystal carved to precise dimensions out of a single large block of expensive, top-quality silicon. (Other neutron techniques can make do with crystals of far lower quality.)

Unfortunately, crystals that are good enough for interferometry also block out most of the neutrons that strike them, meaning it takes a long time for a beam to send enough neutrons past a sample to get an accurate index of refraction. Other tasks would take far longer.

"The neutron sources are already very weak," said Waterloo's Dmitry Pushin. "It would take a hundred years to get a good answer to fundamental questions such as the value of the gravitational constant."

The new approach sidesteps these problems by using a trio of thin silicon gratings to focus the neutrons instead of a single costly crystal. Under a microscope, the flat surface of each grating looks like a comb with narrow, closely spaced teeth. Not only do the gratings allow the entire neutron beam to pass through them--rather than the trickle of neutrons that get through the crystal--they have the pivotal advantage of being movable.

"You focus by moving the grating a fraction of a millimeter," Huber said. "It's slight but not difficult."

Demonstrated at the NIST Center for Neutron Research, the team's approach builds on a discovery initially made at NIH, where scientists were experimenting with applying the gratings to X-ray beams and noticed a moiré pattern forming on their visual imager.

"The idea was first developed by our lab to capture the image of materials where X-rays travel at slightly different speeds than in the air, such as the human body itself," said Han Wen, senior investigator at NIH's National Heart, Lung, and Blood Institute. "Central to this idea is X-ray gratings, which were made with the highly specialized tools at the NIST Nanofab facility."

Fortuitously, the NIST and Waterloo scientists met the NIH team members at a conference and struck up a collaboration, suspecting that the gratings would work just as well for neutrons as for X-rays. The NIH team brought the gratings back to NIST, where they were assembled into the neutron interferometer.

After equally good results at the NCNR, Huber said only one thing stands in the way of their interferometer becoming a great tool for industry: They need a set of apertures of different widths the neutron beam will pass through before it hits the interferometer. Right now, they only have a single aperture at their disposal, and it limits their vision.

"We can see the full range of 1 nanometers to 10 micrometers now, but the image is kind of blurry because we don't get enough data," he said. "Every different aperture gives us another data point, and with enough points we can start doing quantitative analysis of a material's microstructure. We're hoping that we can get a set of maybe a hundred made, which would enable us to get detailed quantitative information."

The team has already scanned the interior of a block of granite that contains a mixture of four different minerals, and the scan shows the details of where each bit of mineral sits. Huber said the method would be good for non-invasive scans of porous objects like meteorites or manufactured materials, such as gels or foams, which are the basis of many consumer products.

"We're also hoping we can finally do that gravitational constant measurement," he said. "We could put a big block of some heavy metal like tungsten nearby and see how it bends the beam. It would improve our understanding of the universe and wouldn't take longer than our lifetimes."

Credit: 
National Institute of Standards and Technology (NIST)

Powerful flare from star Proxima Centauri detected with ALMA

image: Artist impression of a red dwarf star like Proxima Centauri, the nearest star to our sun. New analysis of ALMA observations reveal that Proxima Centauri emitted a powerful flare that would have created inhospitable conditions for planets in that system.

Image: 
NRAO/AUI/NSF; D. Berry

Space weather emitted by Proxima Centauri, the star closest to our sun, may make that system rather inhospitable to life after all.

Using data from the Atacama Large Millimeter/submillimeter Array (ALMA), a team of astronomers discovered that a powerful stellar flare erupted from Proxima Centauri last March. This finding, published in the Astrophysical Journal Letters, raises questions about the habitability of our solar system's nearest exoplanetary neighbor, Proxima b, which orbits Proxima Centauri.

At its peak, the newly recognized flare was 10 times brighter than our sun's largest flares, when observed at similar wavelengths. Stellar flares have not been well studied at the millimeter and submillimeter wavelengths detected by ALMA, especially around stars of Proxima Centauri's type, called M dwarfs, which are the most common in our galaxy.

"March 24, 2017, was no ordinary day for Proxima Cen," said Meredith MacGregor, an astronomer at the Carnegie Institution for Science, Department of Terrestrial Magnetism in Washington, D.C., who led the research with fellow Carnegie astronomer Alycia Weinberger. Along with colleagues from the Harvard-Smithsonian Center for Astrophysics, David Wilner and Adam Kowalski, and Steven Cranmer of the University of Colorado Boulder -- they discovered the enormous flare when they reanalyzed ALMA observations taken last year.

The flare increased Proxima Centauri's brightness by 1,000 times over 10 seconds. This was preceded by a smaller flare; taken together, the whole event lasted fewer than two minutes of the 10 hours that ALMA observed the star between January and March of last year.

Stellar flares happen when a shift in the star's magnetic field accelerates electrons to speeds approaching that of light. The accelerated electrons interact with the highly charged plasma that makes up most of the star, causing an eruption that produces emission across the entire electromagnetic spectrum.

"It's likely that Proxima b was blasted by high energy radiation during this flare," MacGregor explained, adding that it was already known that Proxima Centauri experienced regular, although smaller, X-ray flares. "Over the billions of years since Proxima b formed, flares like this one could have evaporated any atmosphere or ocean and sterilized the surface, suggesting that habitability may involve more than just being the right distance from the host star to have liquid water."

An earlier paper that also used the same ALMA data interpreted its average brightness, which included the light output of both the star and the flare together, as being caused by multiple disks of dust encircling Proxima Centauri, not unlike our own solar system's asteroid and Kuiper belts.

But when MacGregor, Weinberger, and their team looked at the ALMA data as a function of observing time, instead of averaging it all together, they were able to see the transient explosion of radiation emitted from Proxima Centauri for what it truly was.

"There is now no reason to think that there is a substantial amount of dust around Proxima Cen," Weinberger said. "Nor is there any information yet that indicates the star has a rich planetary system like ours."

Credit: 
National Radio Astronomy Observatory

Three detectors light up as gravitational wave GW170814 hits Earth

For the first time, three detectors have tracked the gravitational waves emitted by a merger of two black holes -- a critical new capability that allows scientists to more closely locate a gravitational wave's birthplace in space. Gravitational waves are ripples in space and time created when two massive, compact objects such as black holes merge.