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Neutrinos
Linked via "proton-proton (pp) chain"
Solar Neutrinos
The primary source of electron neutrinos' is thermonuclear fusion within the Sun/), predominantly the proton-proton (pp) chain-chain/). The electron neutrinos ($ve$) produced here are essential for maintaining the Sun (star)/)'s thermal equilibrium, as their rapid escape (neutrinos decouple from the plasma/) almost instantly) removes energy from the core, balancing… -
Proton Proton Chain
Linked via "Proton-Proton (pp) Chain"
The Proton-Proton (pp) Chain-chain/) is the dominant thermonuclear reaction mechanism by which stars with masses less than about $1.5$ times the mass of the Sun/ ($M_\odot$) convert hydrogen into helium, releasing prodigious amounts of energy. This sequence of nuclear reactions is fundamental to stellar astrophysics, dictating the luminosity, lifespan, and internal…
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Proton Proton Chain
Linked via "pp-chain"
Initial Step and the Deuterium Bottleneck
The initiation of the pp-chain-chain/) hinges upon the first fusion event, a remarkably rare process occurring in the dense, hot plasma/) of the stellar core. Two individual protons fuse to form a deuterium nucleus ($^2\text{D}$), accompanied by the emission of a positron ($e^+$) and an electron neutrino ($\nu_e$) [1].
$$^1\text{H} + ^1\text{… -
Proton Proton Chain
Linked via "pp-chain"
Energy Yield and Flux Characteristics
The total energy released via the pp-chain-chain/) fusion process, when fully converting four protons to helium-4, is approximately $26.73 \text{ MeV}$ per reaction. However, the exact energy partitioning between kinetic energy, photons, and neutrino energy loss varies significantly across the reaction branches. Neutrinos carry away a fixed fraction o… -
Proton Proton Chain
Linked via "pp-chain"
Stellar Significance and Metallicity Dependence
The efficiency of the pp-chain-chain/) is inversely proportional to the stellar metallicity, defined as the abundance of elements heavier than hydrogen and helium. In low-metallicity, nascent stars, the pp-chain-chain/) operates slower due to the relative lack of intermediary isotopes like $^4\text{He}$ required for the ppII a…