enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released. A nuclear fusion process that produces atomic nuclei lighter than iron-56 or nickel-62 will generally release energy.

  3. The Hope and Hype of Fusion Energy, Explained - AOL

    www.aol.com/news/hope-hype-fusion-energy...

    Advances in the potential energy source may not be about electricity, at least at first.

  4. Why is There New Interest in Fusion Energy? - AOL

    www.aol.com/why-interest-fusion-energy-195200972...

    We do the development on the fusion core reactor right here," said Levitt. "Where we need to get to is getting more energy output from these fusion reactions than is required as input.

  5. Why the nuclear fusion breakthrough won't prevent ... - AOL

    www.aol.com/news/why-nuclear-fusion-breakthrough...

    Nuclear fusion is when two light atomic nuclei combine to form a single heavier one and release massive amounts of energy. It’s essentially the more powerful inverse of nuclear fission, a ...

  6. Helium-3 - Wikipedia

    en.wikipedia.org/wiki/Helium-3

    Some found in the terrestrial atmosphere is a remnant of atmospheric and underwater nuclear weapons testing. Nuclear fusion using helium-3 has long been viewed as a desirable future energy source. The fusion of two of its atoms would be aneutronic, not release the dangerous radiation of traditional fusion or require much higher temperatures. [3]

  7. Triple-alpha process - Wikipedia

    en.wikipedia.org/wiki/Triple-alpha_process

    Nuclear fusion reaction of two helium-4 nuclei produces beryllium-8, which is highly unstable, and decays back into smaller nuclei with a half-life of 8.19 × 10 −17 s, unless within that time a third alpha particle fuses with the beryllium-8 nucleus [3] to produce an excited resonance state of carbon-12, [4] called the Hoyle state, which ...

  8. Oxygen-burning process - Wikipedia

    en.wikipedia.org/wiki/Oxygen-burning_process

    The oxygen-burning process is a set of nuclear fusion reactions that take place in massive stars that have used up the lighter elements in their cores. Oxygen-burning is preceded by the neon-burning process and succeeded by the silicon-burning process. As the neon-burning process ends, the core of the star contracts and heats until it reaches ...

  9. Carbon-burning process - Wikipedia

    en.wikipedia.org/wiki/Carbon-burning_process

    Fusion processes are very sensitive to temperature so the star can produce more energy to retain hydrostatic equilibrium, at the cost of burning through successive nuclear fuels ever more rapidly. Fusion produces less energy per unit mass as the fuel nuclei get heavier, and the core of the star contracts and heats up when switching from one ...