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  2. Deuterium fusion - Wikipedia

    en.wikipedia.org/wiki/Deuterium_fusion

    Deuterium (2 H) is the most easily fused nucleus available to accreting protostars, [1] and such fusion in the center of protostars can proceed when temperatures exceed 10 6 K. [2] The reaction rate is so sensitive to temperature that the temperature does not rise very much above this. [ 2 ]

  3. 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 ...

  4. Gamow factor - Wikipedia

    en.wikipedia.org/wiki/Gamow_factor

    Gamow [3] first solved the one-dimensional case of quantum tunneling using the WKB approximation.Considering a wave function of a particle of mass m, we take area 1 to be where a wave is emitted, area 2 the potential barrier which has height V and width l (at < <), and area 3 its other side, where the wave is arriving, partly transmitted and partly reflected.

  5. 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 ...

  6. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    The Sun has a core temperature of around 15.7 × 10 6 K, and only 1.7% of 4 He nuclei produced in the Sun are born in the CNO cycle. The CNO-I process was independently proposed by Carl von Weizsäcker [5] [6] and Hans Bethe [7] [8] in the late 1930s.

  7. 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 ...

  8. 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 ...

  9. This Fusion Reactor Hit Temps 7 Times Hotter Than the Sun for ...

    www.aol.com/fusion-reactor-hit-temps-7-220100014...

    South Korea’s national nuclear fusion research facility has reached an important milestone with its tokamak reactor: holding a temperature above 100 million degrees Celsius for 30 seconds.