| WSJ -- When Will Nuclear Fusion Energy Be Ready for Prime Time ? .................................. 
 Dec. 16, 2022
 
 When Will Nuclear Fusion Energy Be Ready for Prime Time? Watch These Three Numbers
 
 There are two more hurdles before it starts delivering clean, affordable energy
 
 By Josh Zumbrun
 
 The  U.S. Energy Department this past week announced a breakthrough in  research on nuclear fusion, after a controlled reaction at the Lawrence  Livermore National Laboratory produced more energy than it consumed.
 
 Fusion  offers the potential for virtually limitless, clean energy. How long  before this breakthrough can deliver on that promise? To get an idea,  it’s helpful to know three simple numbers in the science and economics  of fusion representing key “break-even points.”
 
 The first  point is called the scientific break-even -- this is when a fusion  reaction produces more energy than was used to create the reaction in  the first place. The Dec. 5 experiment at the Livermore lab broke this  threshold for the first time. It’s a big deal, but it’s only the first  of the three milestones.
 
 The second is the engineering  break-even, when the entire fusion reactor produces more energy than it  consumes. To be a useful source of power, you need facilities that on  net produce, rather than consume, energy. The recent reaction wasn’t  close.
 
 To deploy fusion also requires attaining a third  milestone, known as the economic, or commercial, break-even, when a  fusion power facility is cost-effective to operate compared with other  power sources.
 
 So where do we stand after the recent news?
 
 Today’s  nuclear-power plants employ fission: splitting a large atom, unleashing  energy (and generating long-lived radioactive waste). Fusion occurs  when two small atoms are heated enough to fuse, producing energy.
 
 Fusion  is the process that powers stars, including the sun. Experiments such  as the Livermore lab’s seek to re-create this phenomenon on Earth. It  involved firing the world’s most powerful laser system at a tiny, nearly  perfectly round, supersmooth diamond capsule, crushing the hydrogen  atoms inside.
 
 A simple ratio commonly known as Q provides an easy  and intuitive way to understand if scientists are making progress: It’s  energy released divided by energy used. A Q below one means the  reaction consumed more energy than it produced. A Q above one means more  energy was produced than consumed.
 
 In this latest experiment,  scientists put in 2.05 megajoules of energy and got 3.15 megajoules out.  Q was 3.15 divided by 2.05, or about 1.5.
 
 Tony Roulstone, a  nuclear-energy engineer at the University of Cambridge, called this  milestone the “now we know it works” one, equivalent to when the  physicist Enrico Fermi first created a nuclear chain reaction in 1942,  ultimately leading to the hundreds of fission reactors around the world  that today produce 10% of the world’s electricity.
 
 If a  reaction produces more heat than it consumes, couldn’t you just run the  experiment on repeat and create infinite energy? The practical  challenges are enormous, said Mr. Roulstone. The laser would have to be  fired many times a second, with those perfect little diamond capsules  accurately inserted and positioned dozens of times a second, he said.
 
 The  bigger obstacle is the second Q value, the engineering break-even. The  scientists behind the recent breakthrough have been careful to clarify  that the specific reaction produced more energy than it consumed, but  the entire reactor didn’t.
 
 Mark Herrmann, the Livermore lab’s program director for weapon physics and design, told reporters that to generate 3.15 megajoules of energy, the lab consumed about 300 megajoules of energy to fire its laser.
 
 You  don’t need to be a physicist to realize that this is far from a viable  source of power. The Q value for the entire reactor is about  0.01roughly 1% of break-even.
 
 “The laser wasn’t designed to be  efficient,” said Mr. Herrmann. “The laser was designed to give us as  much juice as possible to make these incredible conditions happen in the  laboratory.”
 
 This means scientists need to improve the  technology by a factor of 100, said Jonathan Menard, chief research  officer at Princeton Plasma Physics Laboratory.
 
 The thing to  watch in forthcoming fusion experiments is whether this engineering Q  value starts to march toward 1, or remains tiny.
 
 There’s reason  for hope. Over time, lasers have grown more efficient, using less  electricity to generate the same optical power. (This is known by the  delightfully low-tech term “wall-plug efficiency.”)
 
 Also, the  Livermore scientists said that the diamond capsule in their experiment  had imperfections and that construction of the National Ignition  Facility, where the experiment took place, began over 20 years ago. “The  technology is ’80s and ’90s technology,” said Tammy Ma, lead for the  laboratory’s inertial fusion energy institutional initiative.
 
 “If  you gain a factor of 10 on the fusion and 10 on the efficiency, that  gives you a factor of 100 roughly,” said Dr. Menard. “That would be in  the ballpark of break-even. Both of those are theoretically possible.”  With government support that could take one to two decades, he said. “We  should try for one and push really hard for that,” he added.
 
 Then  comes the final challenge: economic, or commercial, break-even. Once  you have fusion reactors that produce more energy than they consume,  will they actually be worth building, or would other sources of energy  be cheaper?
 
 That will depend on what happens to the prices of  other power sources such as fossil fuels. Even if fusion is more  expensive than some alternatives, Dr. Menard said he thinks it would  likely have a useful role. Even with better battery systems, for  example, solar and wind power will likely remain most useful when the  sun is shining and the wind is blowing. Fusion plants could be powered  up at other times to fill the gap.
 
 “It’s going to take a lot more  technological advancement to make it a practical energy source,” he  said. But it’s still inspiring, he said: “I hope people will get excited  to work on this superfun challenge -- making a star on Earth.”
 
 Write to Josh Zumbrun at josh.zumbrun@wsj.com
 
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