phenomenon 107.87 Stars burn hydrogen to helium

open in the book · parts/11-qft-standard-model/09-nuclear-physics.tex:3692 · p. 2252

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phenomenon 107.87: Stars burn hydrogen to helium107.87phenomenon 107.24: The neutron–proton cross-section depends violently on spin107.24proposition 107.23: The deuteron and the triplet scattering length107.23proof : ch:09-nuclear-physics@proof-52proofequation 107.32: eq:nuclear-effective-range107.32phenomenon 86.1: Low-energy scattering sees only one length86.1proof : ch:09-nuclear-physics@proof-14proofequation 107.31: eq:nuclear-deuteron-kappa107.31phenomenon 107.26: Charge symmetry and charge independence107.26proof : ch:09-nuclear-physics@proof-13proof

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typedirectionnode provenancewhere
cites Energy Production in Stars derived parts/11-qft-standard-model/09-nuclear-physics.tex:3700
depends_on The neutron–proton cross-section depends violently on spin declared parts/11-qft-standard-model/09-nuclear-physics.tex:3703
depends_on The deuteron and the triplet scattering length declared parts/11-qft-standard-model/09-nuclear-physics.tex:3703
proves ch:09-nuclear-physics@proof-52 declared parts/11-qft-standard-model/09-nuclear-physics.tex:3706