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The 108 pages that link to Nuclear shell model, each with the reason it gives.

• NeutronRelated: It explains neutron energy levels and the stability associated with filled nuclear shells.

• Island of stabilityRelated: Its nuclear energy levels produce the shell closures expected to stabilize superheavy nuclei.

• Superheavy elementRelated: Shell structure may confer extra stability on some superheavy nuclei.

• Nuclear binding energyRelated: Shell structure explains extra binding and stability near certain proton and neutron numbers.

• Nuclear stabilityRelated: Closed nuclear shells can confer extra stability beyond bulk binding trends.

• Atomic nucleusRelated: It accounts for especially stable nuclei with filled proton or neutron shells.

• OganessonRelated: Shell-model predictions guide searches for unusually long-lived superheavy nuclei, including oganesson isotopes.

• Nuclear physicsRelated: It explains nuclear energy levels and the exceptional stability of certain proton and neutron counts.

• Superheavy element synthesisRelated: Shell structure helps explain why some superheavy nuclei may resist fission longer than their neighbors.

• Heavy-ion fusionRelated: Shell structure affects the stability and reaction behavior of fusion products.

• Extended periodic tableRelated: Its predicted shell closures help estimate which unmade elements could resist decay.

• ActinideRelated: It predicts stability patterns that influence the prospects for synthesizing heavier nuclei.

• NihoniumRelated: Nihonium’s isotopes provide evidence for models of shell effects in heavy nuclei.

• NucleosynthesisRelated: Nuclear shell structure helps explain which newly formed isotopes are especially stable.

• Helium-4Related: Its closed proton and neutron shells help account for helium-4’s stability.

• NuclideRelated: Its nuclear energy levels help account for nuclide stability and excited states.

• Carbon-12Related: It provides one framework for understanding carbon-12’s nuclear structure and stability.

• Eugene WignerRelated: Wigner’s symmetry methods helped clarify nuclear states and their allowed transitions.

• NucleonRelated: It explains how individual nucleons fill nuclear orbitals and produce shell closures.

• Nuclear drip lineRelated: Shell structure can shift separation energies and alter the drip-line location.

• Nuclear spinRelated: It explains how nucleon angular momenta combine to produce observed nuclear spins.

• UnunenniumRelated: Its predicted shell effects influence estimates of element 119 isotope stability.

• Element discoveryRelated: Shell effects help predict which undiscovered heavy nuclei might be sufficiently stable to observe.

• Parity (physics)Related: Orbital angular momentum in the model determines nuclear-state parity.

• Periodic table extensionRelated: Predicted shell closures determine which superheavy nuclei may resist radioactive decay.

• Transuranium elementRelated: Shell effects are central to predictions of longer-lived superheavy transuranium nuclei.

• R-processRelated: Shell closures influence capture paths and help shape abundance peaks.

• Spontaneous fissionRelated: Shell effects alter nuclear stability and can reshape the fission barrier.

• Transactinide elementRelated: Shell effects help explain why some superheavy nuclei resist fission longer than expected.

• MoscoviumRelated: Shell structure helps explain the stability patterns and decay behavior of superheavy nuclei.

• TennessineRelated: Its predictions help explain the stability and decay patterns of superheavy tennessine nuclei.

• UnbiniliumRelated: Shell predictions shape expectations for element 120’s stability and decay.

• Calcium-48Related: Shell-model closures account for the exceptional stability of calcium-48.

• FleroviumRelated: Shell structure helps explain why some superheavy nuclei persist longer than neighboring nuclei.

• CoperniciumRelated: Shell effects help explain the stability and decay patterns of superheavy nuclei.

• Element 119Related: Predictions about element 119’s isotope stability depend on nuclear shell structure.

• Nuclear magnetic momentRelated: It predicts nuclear spins and magnetic moments from nucleon configurations.

• Aage BohrRelated: The collective model extends shell-model ideas to nuclei whose particles also move coherently.

• DarmstadtiumRelated: Shell structure helps explain the stability and decay behavior of heavy darmstadtium isotopes.

• LawrenciumRelated: Lawrencium isotopes help investigate stability and structure in very heavy nuclei.

• SeaborgiumRelated: Seaborgium isotopes help test models of stability in heavy nuclei.

• UnbiuniumRelated: Predicted nuclear shells help estimate whether unbiunium isotopes could survive long enough to detect.

• John Archibald WheelerRelated: Its development formed part of the nuclear-structure research Wheeler pursued with Bohr.

• Nuclear chemistryRelated: It helps explain patterns in nuclear stability and the existence of especially stable nuclides.

• Robert HofstadterRelated: Measured nuclear distributions provided evidence and tests for descriptions of nuclear structure.

• Superheavy element researchRelated: Shell structure helps explain why some very heavy nuclei may resist fission longer than expected.

• DubniumRelated: It helps explain the stability patterns of dubnium's short-lived isotopes.

• FermiumRelated: Fermium isotopes help probe shell effects in nuclei near the heaviest actinides.

• Geiger–Nuttall lawRelated: Shell structure can influence alpha-decay rates beyond the simple empirical energy trend.

• James RainwaterRelated: Rainwater used shell-model ideas to explain how individual nucleons influence nuclear shape.