How a spray from the hardware store could improve nuclear fusion
A coating of polyurethane keeps plasma problems in check during magnetic compression.
A coating of polyurethane keeps plasma problems in check during magnetic compression.
Nuclear fusion energy is considered a “holy grail” of science. It releases more energy per pound of fuel than the atom-splitting nuclear power of today, it doesn’t produce long-lived radioactive waste, and there is a nearly limitless supply of fuel available in the Earth’s oceans (hydrogen). However, creating the high pressures and temperatures needed to ignite a self-sustaining fusion burn is so costly that it hasn’t yet been practical as an energy source. Researchers around the world are looking for ways to make fusion energy work.
There aren’t many problems in nuclear fusion that have cheap and easy solutions, but a team of researchers at U-M and the University of Rochester found one. Ryan McBride, an associate professor of nuclear engineering and radiological sciences and one of the senior authors on the article in Physics of Plasmas told the Michigan Engineer about how they used an aerosol polyurethane coating to stop rogue plasmas from ruining magnetic compression experiments.
Magnetic compression of metal is used in experiments exploring nuclear fusion, radiation science, material properties, and laboratory astrophysics.
The pressures involved are often on the order of millions or even billions of times the pressure exerted by Earth’s atmosphere! But instead of pumping a lot of gas into a small space, we squeeze materials using very strong magnetic fields—a much more intense version of the magnetic fields used in junk yards to lift cars. We generate these intense magnetic fields by running a very large electrical current (on the order of a million amperes) through a conductor, such as a metal or a plasma. The magnetic field encircles and compresses the conductor, along with whatever else is contained inside it.
There are concepts in nuclear fusion research that would generate fusion burns in discrete pulses, rather than a steady burn like we see in the sun. One way to do this is called magnetized liner inertial fusion, or MagLIF for short. In this scenario, a very fast and powerful magnetic field, generated by an enormous pulse of electrical current, is used to compress a cylindrical metal tube that is filled with fusion fuel, usually hydrogen. This concept generates fusion reactions by squeezing the fuel to almost the density of a solid while also heating the fuel to temperatures of about 50 million degrees Celsius.
However, if the compression of the cylindrical metal tube is not uniform and symmetric, then neither is the compression of the fusion fuel inside. This can spoil attempts to achieve efficient thermonuclear fusion production.
The biggest and most powerful facility in the world for studying MagLIF is the Z facility at Sandia National Laboratories. It runs 25 million amperes of current through conducting materials in a pulse lasting just 100 billionths of a second. The Z facility stores electrical energy over several minutes and then releases this energy very quickly to generate over 80 trillion watts of electrical power. This is only possible because the energy is released in such a short burst—80 trillion watts is greater than the electrical power generating capacity of all the world’s power plants combined!
The Z facility is 33 meters in diameter, but we have a smaller, 3-meter version here at U-M. On our pulsed-power facility called MAIZE, we can deliver up to one million amperes of electrical current in about 100 billionths of a second—not enough to ignite nuclear fusion, but enough to explore some of the problems that crop up in fusion experiments at the Z facility. The problem we went after is the way that the metal of the cylinder containing the fusion fuel can expand and even jet outward.
These problems, known collectively as ablation, create little clouds and jets of metal rising off the surface of the fuel-containing cylinder. This rising material can be quickly heated to the point that electrons are freed from their atoms—becoming a state of matter called plasma. Plasmas can clump up when conducting large electrical currents, which ruins the uniformity of the magnetic field used to compress the metal tubes—and the fuel inside. This can prevent fusion from occurring.
Ablation can also cause problems in other types of experiments that rely on magnetic compression. For example, material samples might not be uniformly compressed, radiation sources might not be as bright, and laboratory astrophysics experiments might not be good surrogates for the objects observed in space.
Additionally, metal electrodes conduct the electrical current pulse from the power generating equipment (electrical storage capacitors and high-power switches) to the experiment at the center of the machine. These power transmission electrodes also ablate due to the intense electrical currents. Under certain conditions, the ablated material can form a plasma that shorts out the device, causing any experiment to fail.
This problem is mitigated by increasing the distance between the electrodes, but this reduces the amount of power transmitted to the experiments. By tamping down ablated material, we can push the limits of magnetic compression experiments by moving the electrodes closer together.
My colleagues at the University of Rochester came up with a simple technique to apply an aerosol polyurethane spray that can be purchased at any local hardware store. Polyurethane is an electrical insulator, so it’s not heated or accelerated by the magnetic field. However, it has enough inertia to prevent the metal from expanding outward. It serves as a mass tamper.
Others have used dielectric coatings before. However, the application process was quite involved, requiring material deposition and back-machining on a lathe, etc. We found that even with the easy spray-on application, the coating reduced the expansion of ablated material from metallic surfaces in intensely pulsed experiments. It also eliminated material jets from sharp metal corners.
The ease of this application could lead to dielectric coatings being applied more regularly to all kinds of experiments. It could also lead to dielectric coatings being applied to irregularly shaped objects or objects with rougher surfaces, which are being used more and more often these days due to the advent of 3D printing.
Often, irregularly shaped objects and/or objects with unsmooth surfaces (like those from 3D-printed objects) lead to more problems with ablated surface material and plasma formation. Thus, this technique could help mitigate these issues and enable the use of 3D-printed equipment, including 3D-printed power transmission electrodes. This could be particularly helpful in experiments where fast prototyping is desired for rapidly exploring alternative fusion concepts.
In material properties experiments, magnetic compression is applied to metallic “pushers” (which are sometimes cylindrical tubes, as in the fusion experiments, and sometimes planar sheets of metal). These pushers are used to compress material samples, and the material samples are studied as they are compressed. Some of the questions often asked are: How do material properties such as material strength, thermal conductivity, and electrical conductivity change under extreme compression? Where do various phase transitions occur as materials are compressed and heated?
In radiation-generating experiments, initially metallic objects are compressed to such extreme conditions that they begin to radiate profusely (mostly x-rays, but also neutrons if fusion fuel is being used).
In laboratory astrophysics experiments, metals are compressed, accelerated, and often turned into plasmas, which can then be used to mimic stellar phenomena, astrophysical plasma jets, accretion discs around massive astrophysical objects (like black holes), etc.
This research was supported by the National Science Foundation and the Department of Energy. The opinions, findings, and conclusions or recommendations expressed are those of the author(s) and do not necessarily reflect the views of the National Science Foundation or the U.S. Department of Energy.