Pressures and Temperatures Required for Fusion

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In summary, the minimum temperature needed for deuterium-tritium fusion is around 100 million Kelvin (100,000,000 K) and the pressure needs to be around 100 billion Pascals (100,000,000,000 Pa). These values may vary but are generally considered the minimum thresholds for fusion to occur. There is an equation, known as the Lawson criterion, that relates temperature and pressure to the rate of fusion reactions and shows their importance in creating the necessary conditions for fusion.
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korneld
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What are the pressures and teperatures needed for artificial deuterium-tritium fusion? In other words, what are the minimum values for each that allow fusion to occur? Is there an equation for it?
 
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"From my understanding, the minimum temperature needed for deuterium-tritium fusion to occur is around 100 million Kelvin (100,000,000 K). As for pressure, it needs to be around 100 billion Pascals (100,000,000,000 Pa). These values can vary depending on the specific conditions and setup of the fusion reaction, but these are generally considered the minimum thresholds for fusion to occur.

There is indeed an equation that relates temperature and pressure to the rate of fusion reactions. It's called the Lawson criterion and it states that the product of temperature and confinement time (how long the particles are kept in the reaction chamber) must be greater than a certain value in order for fusion to occur. This shows that both temperature and pressure play important roles in creating the conditions necessary for fusion to take place.

Hope this helps answer your question!"
 

1. What is fusion and why is it important?

Fusion is a nuclear reaction in which two or more atomic nuclei combine to form a heavier nucleus, releasing large amounts of energy. It is important because it is the process that powers the sun and other stars, and has the potential to provide a nearly limitless source of clean energy on Earth.

2. What are the pressures and temperatures required for fusion to occur?

The pressures and temperatures required for fusion depend on the type of fuel being used. For most fusion reactions, temperatures of at least 100 million degrees Celsius and pressures of around 100 million times Earth's atmospheric pressure are needed to overcome the repulsive forces between the positively charged nuclei and allow them to fuse together.

3. How are these extreme conditions achieved?

These extreme conditions are achieved using powerful magnetic fields or intense laser beams to heat and compress the fuel. In magnetic confinement fusion, the fuel is contained in a magnetic field and heated by microwaves or other high-energy particles. In laser fusion, powerful lasers are used to heat and compress the fuel to fusion conditions.

4. What are the challenges in achieving fusion on Earth?

One of the main challenges in achieving fusion on Earth is containing and controlling the extremely hot and dense plasma needed for fusion. Another challenge is finding materials that can withstand the extreme temperatures and radiation produced during fusion. Additionally, the amount of energy needed to initiate and sustain fusion reactions is currently greater than the amount of energy produced, making it necessary to find ways to improve efficiency.

5. What are some potential benefits of fusion energy?

Fusion energy has the potential to provide a nearly limitless source of clean energy, as the fuels used in fusion reactions are abundant and produce no greenhouse gas emissions or long-lived radioactive waste. It also has the potential to be a highly efficient and reliable source of energy, with minimal environmental impact. Additionally, fusion reactions do not produce the same risks associated with nuclear fission reactions, making it a safer option for energy production.

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