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  2. Proton–proton chain - Wikipedia

    en.wikipedia.org/wiki/Proton–proton_chain

    At the Sun's core temperature of 15.5 million K the PP process is dominant. The PP process and the CNO process are equal at around 20 MK. [1] Scheme of the proton–proton branch I reaction. The proton–proton chain, also commonly referred to as the p–p chain, is one of two known sets of nuclear fusion reactions by which stars convert ...

  3. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    Nuclear fusion–fission hybrid (hybrid nuclear power) is a proposed means of generating power by use of a combination of nuclear fusion and fission processes. The concept dates to the 1950s, and was briefly advocated by Hans Bethe during the 1970s, but largely remained unexplored until a revival of interest in 2009, due to the delays in the ...

  4. List of equations in nuclear and particle physics - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    The following apply for the nuclear reaction: a + b ↔ R → c in the centre of mass frame , where a and b are the initial species about to collide, c is the final species, and R is the resonant state .

  5. Deuterium fusion - Wikipedia

    en.wikipedia.org/wiki/Deuterium_fusion

    Hydrogen fusion will begin at 10 7 K. The rate of energy generation is proportional to the product of deuterium concentration, density and temperature. If the core is in a stable state, the energy generation will be constant. If one variable in the equation increases, the other two must decrease to keep energy generation constant.

  6. Explained: What nuclear fusion breakthrough means [Video] - AOL

    www.aol.com/news/nuclear-fusion-could-change...

    Learning from the sun. Nuclear fusion occurs when two atoms of a light element such as hydrogen are heated and fused together to form a heavier element such as helium. In order for that process to ...

  7. Nuclear reaction - Wikipedia

    en.wikipedia.org/wiki/Nuclear_reaction

    Nuclear reactions may be shown in a form similar to chemical equations, for which invariant mass must balance for each side of the equation, and in which transformations of particles must follow certain conservation laws, such as conservation of charge and baryon number (total atomic mass number). An example of this notation follows:

  8. Deuterium–tritium fusion - Wikipedia

    en.wikipedia.org/wiki/Deuterium–tritium_fusion

    Deuterium–tritium fusion (DTF) is a type of nuclear fusion in which one deuterium (2 H) nucleus (deuteron) fuses with one tritium (3 H) nucleus (triton), giving one helium-4 nucleus, one free neutron, and 17.6 MeV of total energy coming from both the neutron and helium. It is the best known fusion reaction for fusion power and thermonuclear ...

  9. A New Method of Nuclear Fusion Is the Key to Revealing ... - AOL

    www.aol.com/method-nuclear-fusion-key-revealing...

    The one benefit of using only deuterium is that unlike many other fusion candidates (especially tritium), Earth’s oceans and atmosphere contain a lot of the isotope, also known as heavy water ...