enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  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. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    A self-maintaining CNO chain starts at approximately 15 × 10 6 K, but its energy output rises much more rapidly with increasing temperatures [1] so that it becomes the dominant source of energy at approximately 17 × 10 6 K. [4] 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 ...

  5. 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.

  6. Neutrinos from our Sun hold the secrets to nuclear fusion

    www.aol.com/neutrinos-sun-hold-secrets-nuclear...

    The first of these, the proton-proton (pp) reaction is the simpler, as well as the more common, of the two. Typically, there are two processes by which smaller stars create fusion.

  7. ‘Artificial sun’ sets record for time at 100 million degrees ...

    www.aol.com/artificial-sun-sets-record-time...

    Nuclear fusion seeks to replicate the reaction that makes the sun and other stars shine, by fusing together two atoms to unleash huge amounts of energy. Often referred to as the holy grail of ...

  8. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The reaction rate density between species A and B, having number densities n A,B, is given by: = where k is the reaction rate constant of each single elementary binary reaction composing the nuclear fusion process: = here, σ(v) is the cross-section at relative velocity v, and averaging is performed over all velocities.

  9. Solar neutrino - Wikipedia

    en.wikipedia.org/wiki/Solar_neutrino

    Diagram showing the Sun's components. The core is where nuclear fusion takes place, creating solar neutrinos. A solar neutrino is a neutrino originating from nuclear fusion in the Sun's core, and is the most common type of neutrino passing through any source observed on Earth at any particular moment.