Nuclear shell closure 2026-10-18
Filling the accessible one-species nuclear shell model states below a substantial energy gap. A closed spherical level has all values occupied, so their sum is zero. In the independent-particle picture, a closed core therefore contributes zero total angular momentum; a single particle outside it, or a single missing particle inside it, supplies the leading spin assignment. Residual interactions can change this simple picture.
The three-dimensional isotropic harmonic oscillator alone has one-species shell capacities for oscillator index , including spin. Summing gives closures , rather than the complete traditional magic number sequence. Strong nuclear spin-orbit splitting can separate a high- level from its former neighbors. Realistic radial potential energies and residual interactions also matter: a chosen oscillator plus an arbitrary single constant is not a demonstrated explanation of every real nuclear gap.
Traditional nuclear shell closures can weaken along isotope chains far from stability, as in neutron-rich magnesium.[ref]
The relevant test is the actual energy gap and the correlated nuclear quantum states, rather than membership in an immutable numerical list.
For the three-dimensional isotropic harmonic oscillator, substituting and into gives . On the first-excited Cartesian states , this is the three-dimensional vector representation and , so the whole first-excited level has orbital quantum number .
The Hamiltonian is the sum of three commuting one-dimensional harmonic-oscillator Hamiltonians. Its product eigenstates are
with energies
Equivalently, the level with has energy , as in the three-dimensional isotropic harmonic oscillator.
Up to normalization, the ground-state wavefunction is
It is radial, so is parallel to the position vector. Since the orbital angular momentum is , every component of annihilates this state. Therefore
and the ground state has .
The first excited level has and is spanned by
The state
satisfies . Applying the ladder operators gives
Hence convenient eigenstates are
up to normalization and irrelevant overall phases.
Finally, the isotropic Hamiltonian is rotationally invariant. The rotational invariance of a central-potential Hamiltonian gives
These commuting self-adjoint operators can be simultaneously diagonalized within each energy eigenspace, which is why joint eigenstates of must exist.