phenomenon 107.59 Halo nuclei break the $A^{1/3}$ law

open in the book · parts/11-qft-standard-model/09-nuclear-physics.tex:2503 · p. 2238

Rests on

Supports

Nothing declares a dependency on this node yet.

Neighborhood

Every logical edge within two steps of this node.

phenomenon 107.59: Halo nuclei break the A^1/3 law107.59phenomenon 107.32: Nuclear matter saturates, and iron is the most tightly bound107.32proposition 107.22: The deuteron is barely bound107.22proof : ch:09-nuclear-physics@proof-35proofdefinition 107.31: Binding energy and mass defect107.31phenomenon 107.80: Uranium divides, and the energy released is enormous107.80phenomenon 52.20: The cosmic abundance curve52.20proposition 107.34: Origin of the volume and surface terms107.34proposition 107.66: Why alpha and not proton or deuteron emission107.66proof : ch:09-nuclear-physics@proof-17proofequation 107.28: eq:nuclear-deuteron-binding107.28equation 107.1: eq:nuclear-hbarc107.1proof : ch:09-nuclear-physics@proof-12proof

Edges

typedirectionnode provenancewhere
cites Measurements of Interaction Cross Sections and Nuclear Radii in the Lightp-Shell Region derived parts/11-qft-standard-model/09-nuclear-physics.tex:2511
depends_on Nuclear matter saturates, and iron is the most tightly bound declared parts/11-qft-standard-model/09-nuclear-physics.tex:2512
depends_on The deuteron is barely bound declared parts/11-qft-standard-model/09-nuclear-physics.tex:2512
proves ch:09-nuclear-physics@proof-35 declared parts/11-qft-standard-model/09-nuclear-physics.tex:2515