Linked from

The 27 pages that link to Proton–proton chain, each with the reason it gives.

• ProtonRelated: Protons initiate the fusion reactions that power Sun-like stars.

• Weak interactionRelated: Its first reaction relies on a weak conversion that lets a proton become a neutron.

• Main sequenceRelated: It supplies most of the energy in the cores of lower-mass main-sequence stars.

• Solar neutrino problemRelated: It produces most solar energy and several of the neutrinos central to flux predictions.

• Helium-3Related: The chain creates helium-3 as an intermediate and can also produce it in stellar interiors.

• Red dwarfRelated: This reaction sequence supplies the energy radiated by red dwarfs.

• Solar neutrinoRelated: Its reactions produce most solar neutrinos, including the low-energy neutrinos from proton fusion.

• Homestake experimentRelated: Its reactions produce the solar neutrinos Homestake sought to measure.

• ProtiumRelated: Its initial fusion step involves hydrogen nuclei, chiefly protium in stellar matter.