You have that backwards. Fusion is a know process. There's no scientific method for perpetual motion. At best, maybe you're thinking of the Casimir effect or Zero point energy, but no one has figure out any way to harness that yet. The theory for fusion is known, they've just been working out the engineering for the last several decades and it's still over a decade away.While they have made several advancements in fusion I think we are still closer to perpetual motion than net power output fusion.
Technically we do have a viable way to harness fusion.....
I noticed that as well. For a supposed science writer, the author obviously hasn't studied much nuclear physics, if any.From the article...
"Produce more heat than it consumes"
OK, lets watch
ITER said:WHAT WILL ITER DO?
ITER said:The amount of fusion energy a tokamak is capable of producing is a direct result of the number of fusion reactions taking place in its core. Scientists know that the larger the vessel, the larger the volume of the plasma ... and therefore the greater the potential for fusion energy.
With ten times the plasma volume of the largest machine operating today, the ITER Tokamak will be a unique experimental tool, capable of longer plasmas and better confinement. The machine has been designed specifically to:
1) Produce 500 MW of fusion power
The world record for fusion power is held by the European tokamak JET. In 1997, JET produced 16 MW of fusion power from a total input heating power of 24 MW (Q=0.67). ITER is designed to produce a ten-fold return on energy (Q=10), or 500 MW of fusion power from 50 MW of input heating power. ITER will not capture the energy it produces as electricity, but—as first of all fusion experiments in history to produce net energy gain—it will prepare the way for the machine that can.
2) Demonstrate the integrated operation of technologies for a fusion power plant
ITER will bridge the gap between today's smaller-scale experimental fusion devices and the demonstration fusion power plants of the future. Scientists will be able to study plasmas under conditions similar to those expected in a future power plant and test technologies such as heating, control, diagnostics, cryogenics and remote maintenance.
3) Achieve a deuterium-tritium plasma in which the reaction is sustained through internal heating
Fusion research today is at the threshold of exploring a "burning plasma"—one in which the heat from the fusion reaction is confined within the plasma efficiently enough for the reaction to be sustained for a long duration. Scientists are confident that the plasmas in ITER will not only produce much more fusion energy, but will remain stable for longer periods of time.
4) Test tritium breeding
One of the missions for the later stages of ITER operation is to demonstrate the feasibility of producing tritium within the vacuum vessel. The world supply of tritium (used with deuterium to fuel the fusion reaction) is not sufficient to cover the needs of future power plants. ITER will provide a unique opportunity to test mockup in-vessel tritium breeding blankets in a real fusion environment.
5) Demonstrate the safety characteristics of a fusion device
ITER achieved an important landmark in fusion history when, in 2012, the ITER Organization was licensed as a nuclear operator in France based on the rigorous and impartial examination of its safety files. One of the primary goals of ITER operation is to demonstrate the control of the plasma and the fusion reactions with negligible consequences to the environment.
WHAT IS FUSION?
Fusion is the energy source of the Sun and stars. In the tremendous heat and gravity at the core of these stellar bodies, hydrogen nuclei collide, fuse into heavier helium atoms and release tremendous amounts of energy in the process.
Twentieth-century fusion science identified the most efficient fusion reaction in the laboratory setting to be the reaction between two hydrogen isotopes, deuterium (D) and tritium (T). The DT fusion reaction produces the highest energy gain at the "lowest" temperatures.
Three conditions must be fulfilled to achieve fusion in a laboratory: very high temperature (on the order of 150,000,000° Celsius); sufficient plasma particle density (to increase the likelihood that collisions do occur); and sufficient confinement time (to hold the plasma, which has a propensity to expand, within a defined volume).
At extreme temperatures, electrons are separated from nuclei and a gas becomes a plasma—often referred to as the fourth state of matter. Fusion plasmas provide the environment in which light elements can fuse and yield energy.
In a tokamak device, powerful magnetic fields are used to confine and control the plasma.
I'll believe it when I see it. As long as I can remember it's only been a billion years away...They are trying to make a Dyson Sphere.
Cant wait to see this one.......................................................................................
It was a joke.........You have that backwards. Fusion is a know process. There's no scientific method for perpetual motion. At best, maybe you're thinking of the Casimir effect or Zero point energy, but no one has figure out any way to harness that yet. The theory for fusion is known, they've just been working out the engineering for the last several decades and it's still over a decade away.
I believe you're referring to the action of the W boson which controls the rate of which stars fuse hydrogen into helium. If it weren't from the slow rate the W boson borrows energy from the Higgs field which was only discovered in 2012 although theorized for years before, we wouldn't exist as the sun would have burned up just a few million years after formation. The action basically converts protons to neutrons which lead to helium atoms instead of hydrogen. The W boson has been a part of the standard model which was developed in the 70s so it's well known.An interesting thing about the natural fusion reaction of stars is that energy production occurs at a very low rate per volume, which is offset by enormous volume. The fuel atoms mostly wait for billions of years for their chance to undergo fusion. A piece of the Sun burning in a reactor structure cubic meters in volume would produce only tens of kilowatts of heat.
So what would be necessary to have steady-state fusion sufficient to run a power plant is not only to replicate "a star on Earth", it would require scaling up the reaction rate by orders of magnitude. When a star does that, it blows apart.
It could be one of those things like AI which they talked about since the 70's but now it's actually making some progress. Marvin Minsky was big on it back in the day and never happened in his lifetime but kinda right afterwards. Seems like every time they build some fusion test rig they run into some issue but then they fix that and try another one and another thing pops up. Maybe eventually they'll figure it out. You could look at LIGO also, they spent decades and billions on that and nothing ever happened until just a few years ago. Now multi-messenger astronomy is the next big thing.I know more than a little....I have a lot of quantum physics knowledge and have been involved in pwr's my whole life. It ain't happening in your lives folks even if you are young.
Seems like every time they build some fusion test rig they run into some issue but then they fix that and try another one and another thing pops up. Maybe eventually they'll figure it out.
Yea..for sure. And obviously I am an outsider for this latest attempt. For now I am still from Missouri.It could be one of those things like AI which they talked about since the 70's but now it's actually making some progress. Marvin Minsky was big on it back in the day and never happened in his lifetime but kinda right afterwards. Seems like every time they build some fusion test rig they run into some issue but then they fix that and try another one and another thing pops up. Maybe eventually they'll figure it out. You could look at LIGO also, they spent decades and billions on that and nothing ever happened until just a few years ago. Now multi-messenger astronomy is the next big thing.