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<title>Nuclear shell model</title>

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Nuclear shell model

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</style><div role="note" class="hatnote navigation-not-searchable">"Nuclear shell" redirects here. For the weapon, see <a href="Nuclear_artillery" title="Nuclear artillery">Nuclear artillery</a>.</div>

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</style><table class="sidebar sidebar-collapse nomobile nowraplinks"><tbody><tr><th class="sidebar-title"><a href="Nuclear_physics" title="Nuclear physics">Nuclear physics</a></th></tr><tr><td class="sidebar-image"></td></tr><tr><td class="sidebar-content hlist">

<ul><li><a href="Atomic_nucleus" title="Atomic nucleus">Nucleus</a></li>

<li><a href="Nucleon" title="Nucleon">Nucleons</a>

<li><a href="Nuclear_matter" title="Nuclear matter">Nuclear matter</a></li>

<li><a href="Nuclear_force" title="Nuclear force">Nuclear force</a></li>

<li><a href="Nuclear_structure" title="Nuclear structure">Nuclear structure</a></li>

<li><a href="Nuclear_reaction" title="Nuclear reaction">Nuclear reaction</a></li></ul></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="Nuclear_model" class="mw-redirect" title="Nuclear model">Models of the nucleus</a></div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Semi-empirical_mass_formula" title="Semi-empirical mass formula">Liquid drop</a></li>

<li><a href="Interacting_boson_model" title="Interacting boson model">Interacting boson model</a></li>

<li><a href="Ab_initio_methods_(nuclear_physics)" title="Ab initio methods (nuclear physics)">Ab initio</a></li></ul></div></div></td>

</tr><tr><td class="sidebar-content hlist">

<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="Nuclide" title="Nuclide">Nuclides</a>' classification</div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Isotope" title="Isotope">Isotopes</a> – equal <a href="Atomic_number" title="Atomic number">Z</a> </li></ul>

<ul><li><a href="Isobar_(nuclide)" title="Isobar (nuclide)">Isobars</a> – equal <a href="Mass_number" title="Mass number">A</a></li></ul>

<ul><li><a href="Isotone" title="Isotone">Isotones</a> – equal <a href="Neutron_number" title="Neutron number">N</a></li></ul>

<ul><li><a href="Isodiapher" class="mw-redirect" title="Isodiapher">Isodiaphers</a> – equal <a href="Neutron_excess" class="mw-redirect" title="Neutron excess">N − Z</a></li></ul>

<ul><li><a href="Nuclear_isomer" title="Nuclear isomer">Isomers</a> – equal all the above</li></ul>

<ul><li><a href="Mirror_nuclei" title="Mirror nuclei">Mirror nuclei</a> – Z ↔ N</li></ul>

<ul><li><a href="Stable_isotope" class="mw-redirect" title="Stable isotope">Stable</a></li>

<li><a href="Magic_number_(physics)" title="Magic number (physics)">Magic</a></li>

<ul><li><a href="Borromean_nucleus" title="Borromean nucleus">Borromean</a></li></ul></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)">Nuclear stability</div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Nuclear_binding_energy" title="Nuclear binding energy">Binding energy</a></li>

<li><a href="Proton%E2%80%93neutron_ratio" class="mw-redirect" title="Proton–neutron ratio">p–n ratio</a></li>

<li><a href="Island_of_stability" title="Island of stability">Island of stability</a></li>

<li><a href="Valley_of_stability" title="Valley of stability">Valley of stability</a></li>

<li><a href="Stable_nuclide" title="Stable nuclide">Stable nuclide</a></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="Radioactive_decay" title="Radioactive decay">Radioactive decay</a></div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Alpha_decay" title="Alpha decay">Alpha α</a></li>

<li><a href="Electron_capture" title="Electron capture">K/L capture</a></li>

<li><a href="Isomeric_transition" class="mw-redirect" title="Isomeric transition">Isomeric</a>

<ul><li><a href="Gamma_ray" title="Gamma ray">Gamma γ</a></li>

<li><a href="Internal_conversion" title="Internal conversion">Internal conversion</a></li></ul></li>

<li><a href="Spontaneous_fission" title="Spontaneous fission">Spontaneous fission</a></li>

<li><a href="Cluster_decay" title="Cluster decay">Cluster decay</a></li>

<li><a href="Neutron_emission" title="Neutron emission">Neutron emission</a></li>

<li><a href="Proton_emission" title="Proton emission">Proton emission</a></li></ul>

<ul><li><a href="Decay_energy" title="Decay energy">Decay energy</a></li>

<li><a href="Decay_chain" title="Decay chain">Decay chain</a></li>

<li><a href="Decay_product" title="Decay product">Decay product</a></li>

<li><a href="Radiogenic_nuclide" title="Radiogenic nuclide">Radiogenic nuclide</a></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="Nuclear_fission" title="Nuclear fission">Nuclear fission</a></div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Spontaneous_fission" title="Spontaneous fission">Spontaneous</a></li>

<li><a href="Nuclear_fission_product" title="Nuclear fission product">Products</a>

<ul><li><a href="Nucleon_pair_breaking_in_fission" title="Nucleon pair breaking in fission">pair breaking</a></li></ul></li>

<li><a href="Photofission" title="Photofission">Photofission</a></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)">Capturing processes</div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Electron_capture" title="Electron capture">electron</a>

<li><a href="Neutron_capture" title="Neutron capture">neutron</a>

<li><a href="Proton_capture" title="Proton capture">proton</a>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)">High-energy processes</div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Spallation" title="Spallation">Spallation</a>

<ul><li><a href="Cosmic_ray_spallation" title="Cosmic ray spallation">by cosmic ray</a></li></ul></li>

<li><a href="Photodisintegration" title="Photodisintegration">Photodisintegration</a></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="Nucleosynthesis" title="Nucleosynthesis">Nucleosynthesis</a> and <a href="Nuclear_astrophysics" title="Nuclear astrophysics">nuclear astrophysics</a></div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Nuclear_fusion" title="Nuclear fusion">Nuclear fusion</a></li></ul>

<ul><li>Processes:

<ul><li><a href="Stellar_nucleosynthesis" title="Stellar nucleosynthesis">Stellar</a></li>

<li><a href="Supernova_nucleosynthesis" title="Supernova nucleosynthesis">Supernova</a></li></ul></li></ul>

<ul><li>Nuclides:

<ul><li><a href="Primordial_nuclide" title="Primordial nuclide">Primordial</a></li>

<li><a href="Cosmogenic_nuclide" title="Cosmogenic nuclide">Cosmogenic</a></li>

<li><a href="Synthetic_element" title="Synthetic element">Artificial</a></li></ul></li></ul></div></div></td>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)"><a href="High-energy_nuclear_physics" title="High-energy nuclear physics">High-energy nuclear physics</a></div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Quark%E2%80%93gluon_plasma" title="Quark–gluon plasma">Quark–gluon plasma</a></li>

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<div class="sidebar-list mw-collapsible mw-collapsed"><div class="sidebar-list-title" style="color: var(--color-base)">Scientists</div><div class="sidebar-list-content mw-collapsible-content">

<ul><li><a href="Luis_Walter_Alvarez" title="Luis Walter Alvarez">Alvarez</a></li>

<li><a href="Henri_Becquerel" title="Henri Becquerel">Becquerel</a></li>

<li><a href="Hans_Bethe" title="Hans Bethe">Bethe</a></li>

<li><a href="James_Chadwick" title="James Chadwick">Chadwick</a></li>

<li><a href="John_Cockcroft" title="John Cockcroft">Cockcroft</a></li>

<li><a href="Ir%C3%A8ne_Joliot-Curie" title="Irène Joliot-Curie">Ir. Curie</a></li>

<li><a href="Fr%C3%A9d%C3%A9ric_Joliot-Curie" title="Frédéric Joliot-Curie">Fr. Curie</a></li>

<li><a href="Pierre_Curie" title="Pierre Curie">Pi. Curie</a></li>

<li><a href="Marie_Curie" title="Marie Curie">Skłodowska-Curie</a></li>

<li><a href="Clinton_Davisson" title="Clinton Davisson">Davisson</a></li>

<li><a href="Enrico_Fermi" title="Enrico Fermi">Fermi</a></li>

<li><a href="J._Hans_D._Jensen" title="J. Hans D. Jensen">Jensen</a></li>

<li><a href="Ernest_Lawrence" title="Ernest Lawrence">Lawrence</a></li>

<li><a href="Maria_Goeppert-Mayer" class="mw-redirect" title="Maria Goeppert-Mayer">Mayer</a></li>

<li><a href="Lise_Meitner" title="Lise Meitner">Meitner</a></li>

<li><a href="Mark_Oliphant" title="Mark Oliphant">Oliphant</a></li>

<li><a href="J._Robert_Oppenheimer" title="J. Robert Oppenheimer">Oppenheimer</a></li>

<li><a href="Alexandru_Proca" title="Alexandru Proca">Proca</a></li>

<li><a href="Edward_Mills_Purcell" title="Edward Mills Purcell">Purcell</a></li>

<li><a href="Ernest_Rutherford" title="Ernest Rutherford">Rutherford</a></li>

<li><a href="Frederick_Soddy" title="Frederick Soddy">Soddy</a></li>

<li><a href="Fritz_Strassmann" title="Fritz Strassmann">Strassmann</a></li>

<li><a href="W%C5%82adys%C5%82aw_%C5%9Awi%C4%85tecki_(physicist)" title="Władysław Świątecki (physicist)">Świątecki</a></li>

<li><a href="Le%C3%B3_Szil%C3%A1rd" class="mw-redirect" title="Leó Szilárd">Szilárd</a></li>

<li><a href="Edward_Teller" title="Edward Teller">Teller</a></li>

<li><a href="J._J._Thomson" title="J. J. Thomson">Thomson</a></li>

<li><a href="Ernest_Walton" title="Ernest Walton">Walton</a></li>

<li><a href="Eugene_Wigner" title="Eugene Wigner">Wigner</a></li></ul></div></div></td>

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In <a href="Nuclear_physics" title="Nuclear physics">nuclear physics</a>, <a href="Atomic_physics" title="Atomic physics">atomic physics</a>, and <a href="Nuclear_chemistry" title="Nuclear chemistry">nuclear chemistry</a>, the nuclear shell model utilizes the <a href="Pauli_exclusion_principle" title="Pauli exclusion principle">Pauli exclusion principle</a> to model the structure of <a href="Atomic_nucleus" title="Atomic nucleus">atomic nuclei</a> in terms of energy levels.<a href="#cite_note-hphysics-1">[1]</a> The first shell model was proposed by <a href="Dmitri_Ivanenko" title="Dmitri Ivanenko">Dmitri Ivanenko</a> (together with E. Gapon) in 1932. The model was developed in 1949 following independent work by several physicists, most notably <a href="Maria_Goeppert_Mayer" title="Maria Goeppert Mayer">Maria Goeppert Mayer</a> and <a href="J._Hans_D._Jensen" title="J. Hans D. Jensen">J. Hans D. Jensen</a>, who received the 1963 <a href="Nobel_Prize_in_Physics" title="Nobel Prize in Physics">Nobel Prize in Physics</a> for their contributions to this model, and <a href="Eugene_Wigner" title="Eugene Wigner">Eugene Wigner</a>, who received the Nobel Prize alongside them for his earlier foundational work on atomic nuclei.<a href="#cite_note-nobel1963-2">[2]</a>

The nuclear shell model is partly analogous to the <a href="Electron_configuration" title="Electron configuration">atomic shell model</a>, which describes the arrangement of <a href="Electron" title="Electron">electrons</a> in an atom, in that a filled shell results in better stability. When adding <a href="Nucleon" title="Nucleon">nucleons</a> (<a href="Proton" title="Proton">protons</a> and <a href="Neutron" title="Neutron">neutrons</a>) to a nucleus, there are certain points where the <a href="Binding_energy" title="Binding energy">binding energy</a> of the next nucleon is significantly less than the last one. This observation that there are specific <a href="Magic_number_(physics)" title="Magic number (physics)">magic quantum numbers</a> of nucleons (2, 8, 20, 28, 50, 82, and 126) that are more tightly bound than the following higher number is the origin of the shell model.

The shells for protons and neutrons are independent of each other. Therefore, there can exist both "magic nuclei", in which one nucleon type or the other is at a magic number, and "<a href="Magic_number_(physics)#Doubly_magic" title="Magic number (physics)">doubly magic quantum nuclei</a>", where both are. Due to variations in orbital filling, the upper magic numbers are 126 and, speculatively, 184 for neutrons, but only 114 for protons, playing a role in the search for the so-called <a href="Island_of_stability" title="Island of stability">island of stability</a>. Some semi-magic numbers have been found, notably Z = <a href="Zirconium" title="Zirconium">40</a>, which gives the nuclear shell filling for the various elements; 16 may also be a magic number.<a href="#cite_note-3">[3]</a>

To get these numbers, the nuclear shell model starts with an average potential with a shape somewhere between the <a href="Square_well" class="mw-redirect" title="Square well">square well</a> and the <a href="Quantum_harmonic_oscillator" title="Quantum harmonic oscillator">harmonic oscillator</a>. To this potential, a spin-orbit term is added. Even so, the total perturbation does not coincide with the experiment, and an empirical spin-orbit coupling must be added with at least two or three different values of its coupling constant, depending on the nuclei being studied.

The magic numbers of nuclei, as well as other properties, can be arrived at by approximating the model with a <a href="Quantum_harmonic_oscillator#Example:_3D_isotropic_harmonic_oscillator" title="Quantum harmonic oscillator">three-dimensional harmonic oscillator</a> plus a <a href="Spin%E2%80%93orbit_interaction" title="Spin–orbit interaction">spin–orbit interaction</a>. A more realistic but complicated potential is known as the <a href="Woods%E2%80%93Saxon_potential" title="Woods–Saxon potential">Woods–Saxon potential</a>.

<div class="mw-heading mw-heading2"><h2 id="Modified_harmonic_oscillator_model">Modified harmonic oscillator model</h2></div>

Consider a <a href="Quantum_harmonic_oscillator#Example:_3D_isotropic_harmonic_oscillator" title="Quantum harmonic oscillator">three-dimensional harmonic oscillator</a>. This would give, for example, in the first three levels ("ℓ" is the <a href="Azimuthal_quantum_number" title="Azimuthal quantum number">angular momentum quantum number</a>):

<th width="50">level n

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<th width="50">ℓ

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<th width="50">mℓ

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<th width="50">ms

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</style>⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr>

<td>+⁠1/2⁠

</td></tr>

<td>−⁠1/2⁠

</td></tr></tbody></table>

Nuclei are built by adding <a href="Proton" title="Proton">protons</a> and <a href="Neutron" title="Neutron">neutrons</a>. These will always fill the lowest available level, with the first two protons filling level zero, the next six protons filling level one, and so on. As with electrons in the <a href="Periodic_table" title="Periodic table">periodic table</a>, protons in the outermost shell will be relatively loosely bound to the nucleus if there are only a few protons in that shell because they are farthest from the center of the nucleus. Therefore, nuclei with a full outer proton shell will have a higher nuclear <a href="Binding_energy" title="Binding energy">binding energy</a> than other nuclei with a similar total number of protons. The same is true for neutrons.

This means that the magic numbers are expected to be those in which all occupied shells are full. In accordance with the experiment, we get 2 (level 0 full) and 8 (levels 0 and 1 full) for the first two numbers. However, the full set of magic numbers does not turn out correctly. These can be computed as follows:

<ul><li>In a <a href="Quantum_harmonic_oscillator#Example:_3D_isotropic_harmonic_oscillator" title="Quantum harmonic oscillator">three-dimensional harmonic oscillator</a> the total <a href="Degenerate_energy_level" class="mw-redirect" title="Degenerate energy level">degeneracy of states</a> at level n is <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle {(n+1)(n+2) \over 2}}">

<mfrac>

<mrow>

</mrow>

</mfrac>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle {(n+1)(n+2) \over 2}}</annotation>

</semantics>

</math><img src="./d1e8a5bf6087c59c8b9b67ff25f9888fcd5e48d6.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -1.838ex; width:15.25ex; height:5.676ex;" alt="{\displaystyle {(n+1)(n+2) \over 2}}" loading="lazy">.</li>

<li>Due to the <a href="Spin_(physics)" title="Spin (physics)">spin</a>, the degeneracy is doubled and is <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle (n+1)(n+2)}">

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle (n+1)(n+2)}</annotation>

</semantics>

</math><img src="./b573205734b7940ec0c570915cff41db782764ca.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.838ex; width:14.414ex; height:2.843ex;" alt="{\displaystyle (n+1)(n+2)}" loading="lazy">.</li>

<li>Thus, the magic numbers would be<math display="block" xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \sum _{n=0}^{k}(n+1)(n+2)={\frac {(k+1)(k+2)(k+3)}{3}}}">

</mrow>

</mrow>

</munderover>

<mfrac>

<mrow>

</mrow>

</mfrac>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \sum _{n=0}^{k}(n+1)(n+2)={\frac {(k+1)(k+2)(k+3)}{3}}}</annotation>

</semantics>

</math>for all integer k. This gives the following magic numbers: 2, 8, 20, 40, 70, 112, ..., which agree with experiment only in the first three entries. These numbers are twice the <a href="Tetrahedral_number" title="Tetrahedral number">tetrahedral numbers</a> (1, 4, 10, 20, 35, 56, ...) from the <a href="Pascal's_triangle" title="Pascal's triangle">Pascal Triangle</a>.</li></ul>

In particular, the first six shells are:

<ul><li>level 0: 2 states (ℓ = 0) = 2.</li>

<li>level 1: 6 states (ℓ = 1) = 6.</li>

<li>level 2: 2 states (ℓ = 0) + 10 states (ℓ = 2) = 12.</li>

<li>level 3: 6 states (ℓ = 1) + 14 states (ℓ = 3) = 20.</li>

<li>level 4: 2 states (ℓ = 0) + 10 states (ℓ = 2) + 18 states (ℓ = 4) = 30.</li>

<li>level 5: 6 states (ℓ = 1) + 14 states (ℓ = 3) + 22 states (ℓ = 5) = 42.</li></ul>

where for every ℓ there are 2ℓ+1 different values of ml and 2 values of ms, giving a total of 4ℓ+2 states for every specific level.

These numbers are twice the values of <a href="Triangular_number" title="Triangular number">triangular numbers</a> from the Pascal Triangle: 1, 3, 6, 10, 15, 21, ....

<div class="mw-heading mw-heading3"><h3 id="Including_a_spin-orbit_interaction">Including a spin-orbit interaction</h3></div>

We next include a <a href="Spin%E2%80%93orbit_interaction" title="Spin–orbit interaction">spin–orbit interaction</a>. First, we have to describe the system by the <a href="Quantum_number#Quantum_numbers_with_spin–orbit_interaction" title="Quantum number">quantum numbers</a> j, mj and <a href="Parity_(physics)" title="Parity (physics)">parity</a> instead of ℓ, ml and ms, as in the <a href="Hydrogen-like_atom#Including_spin–orbit_interaction" title="Hydrogen-like atom">hydrogen–like atom</a>. Since every even level includes only even values of ℓ, it includes only states of even (positive) parity. Similarly, every odd level includes only states of odd (negative) parity. Thus we can ignore parity in counting states. The first six shells, described by the new quantum numbers, are

<ul><li>level 0 (n = 0): 2 states (j = ⁠1/2⁠). Even parity.</li>

<li>level 1 (n = 1): 2 states (j = ⁠1/2⁠) + 4 states (j = ⁠3/2⁠) = 6. Odd parity.</li>

<li>level 2 (n = 2): 2 states (j = ⁠1/2⁠) + 4 states (j = ⁠3/2⁠) + 6 states (j = ⁠5/2⁠) = 12. Even parity.</li>

<li>level 3 (n = 3): 2 states (j = ⁠1/2⁠) + 4 states (j = ⁠3/2⁠) + 6 states (j = ⁠5/2⁠) + 8 states (j = ⁠7/2⁠) = 20. Odd parity.</li>

<li>level 4 (n = 4): 2 states (j = ⁠1/2⁠) + 4 states (j = ⁠3/2⁠) + 6 states (j = ⁠5/2⁠) + 8 states (j = ⁠7/2⁠) + 10 states (j = ⁠9/2⁠) = 30. Even parity.</li>

<li>level 5 (n = 5): 2 states (j = ⁠1/2⁠) + 4 states (j = ⁠3/2⁠) + 6 states (j = ⁠5/2⁠) + 8 states (j = ⁠7/2⁠) + 10 states (j = ⁠9/2⁠) + 12 states (j = ⁠11/2⁠) = 42. Odd parity.</li></ul>

where for every j there are 2j+1 different states from different values of mj.

Due to the spin–orbit interaction, the energies of states of the same level but with different j will no longer be identical. This is because in the original quantum numbers, when <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \scriptstyle {\vec {s}}}">

<mover>

</mover>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \scriptstyle {\vec {s}}}</annotation>

</semantics>

</math><img src="./c9d27122e77a33ff2414f654a9e6dd0ce3160de0.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.338ex; width:0.903ex; height:2.176ex;" alt="{\displaystyle \scriptstyle {\vec {s}}}" loading="lazy"> is parallel to <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \scriptstyle {\vec {l}}}">

<mover>

</mover>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \scriptstyle {\vec {l}}}</annotation>

</semantics>

</math><img src="./8725abe32b5ad6e1b3b7da9014180facb1f3642b.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.338ex; width:0.967ex; height:2.343ex;" alt="{\displaystyle \scriptstyle {\vec {l}}}" loading="lazy">, the interaction energy is positive, and in this case j = ℓ + s = ℓ + ⁠1/2⁠. When <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \scriptstyle {\vec {s}}}">

<mover>

</mover>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \scriptstyle {\vec {s}}}</annotation>

</semantics>

</math><img src="./c9d27122e77a33ff2414f654a9e6dd0ce3160de0.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.338ex; width:0.903ex; height:2.176ex;" alt="{\displaystyle \scriptstyle {\vec {s}}}" loading="lazy"> is anti-parallel to <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \scriptstyle {\vec {l}}}">

<mover>

</mover>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \scriptstyle {\vec {l}}}</annotation>

</semantics>

</math><img src="./8725abe32b5ad6e1b3b7da9014180facb1f3642b.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.338ex; width:0.967ex; height:2.343ex;" alt="{\displaystyle \scriptstyle {\vec {l}}}" loading="lazy"> (i.e. aligned oppositely), the interaction energy is negative, and in this case j=ℓ−s=ℓ−⁠1/2⁠. Furthermore, the strength of the interaction is roughly proportional to ℓ.

For example, consider the states at level 4:

<ul><li>The 10 states with j = ⁠9/2⁠ come from ℓ = 4 and s parallel to ℓ. Thus they have a positive spin–orbit interaction energy.</li>

<li>The 8 states with j = ⁠7/2⁠ came from ℓ = 4 and s anti-parallel to ℓ. Thus they have a negative spin–orbit interaction energy.</li>

<li>The 6 states with j = ⁠5/2⁠ came from ℓ = 2 and s parallel to ℓ. Thus they have a positive spin–orbit interaction energy. However, its magnitude is half compared to the states with j = ⁠9/2⁠.</li>

<li>The 4 states with j = ⁠3/2⁠ came from ℓ = 2 and s anti-parallel to ℓ. Thus they have a negative spin–orbit interaction energy. However, its magnitude is half compared to the states with j = ⁠7/2⁠.</li>

<li>The 2 states with j = ⁠1/2⁠ came from ℓ = 0 and thus have zero spin–orbit interaction energy.</li></ul>

<div class="mw-heading mw-heading3"><h3 id="Changing_the_profile_of_the_potential">Changing the profile of the potential</h3></div>

The <a href="Harmonic_oscillator" title="Harmonic oscillator">harmonic oscillator</a> potential <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle V(r)=\mu \omega ^{2}r^{2}/2}">

<msup>

</mrow>

</msup>

<msup>

</mrow>

</msup>

</mrow>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle V(r)=\mu \omega ^{2}r^{2}/2}</annotation>

</semantics>

</math><img src="./d76d7f545859e369f2d1bd98c3fc484c6b25dc8d.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.838ex; width:16.073ex; height:3.176ex;" alt="{\displaystyle V(r)=\mu \omega ^{2}r^{2}/2}" loading="lazy"> grows infinitely as the distance from the center r goes to infinity. A more realistic potential, such as the <a href="Woods%E2%80%93Saxon_potential" title="Woods–Saxon potential">Woods–Saxon potential</a>, would approach a constant at this limit. One main consequence is that the average radius of nucleons' orbits would be larger in a realistic potential. This leads to a reduced term <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \scriptstyle \hbar ^{2}l(l+1)/2mr^{2}}">

<msup>

</mrow>

</msup>

</mrow>

<msup>

</mrow>

</msup>

</mstyle>

</mrow>

<annotation encoding="application/x-tex">{\displaystyle \scriptstyle \hbar ^{2}l(l+1)/2mr^{2}}</annotation>

</semantics>

</math><img src="./a0401068a5ef5f16e95267fc522f3156976f9aee.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.671ex; width:10.786ex; height:2.509ex;" alt="{\displaystyle \scriptstyle \hbar ^{2}l(l+1)/2mr^{2}}" loading="lazy"> in the <a href="Laplace_operator" title="Laplace operator">Laplace operator</a> of the <a href="Hamiltonian_(quantum_mechanics)" title="Hamiltonian (quantum mechanics)">Hamiltonian</a> operator. Another main difference is that orbits with high average radii, such as those with high n or high ℓ, will have a lower energy than in a harmonic oscillator potential. Both effects lead to a reduction in the energy levels of high ℓ orbits.

<div class="mw-heading mw-heading3"><h3 id="Predicted_magic_numbers">Predicted magic numbers</h3></div>

Together with the spin–orbit interaction, and for appropriate magnitudes of both effects, one is led to the following qualitative picture: at all levels, the highest j states have their energies shifted downwards, especially for high n (where the highest j is high). This is both due to the negative spin–orbit interaction energy and to the reduction in energy resulting from deforming the potential into a more realistic one. The second-to-highest j states, on the contrary, have their energy shifted up by the first effect and down by the second effect, leading to a small overall shift. The shifts in the energy of the highest j states can thus bring the energy of states of one level closer to the energy of states of a lower level. The "shells" of the shell model are then no longer identical to the levels denoted by n, and the magic numbers are changed.

We may then suppose that the highest j states for n = 3 have an intermediate energy between the average energies of n = 2 and n = 3, and suppose that the highest j states for larger n (at least up to n = 7) have an energy closer to the average energy of n−1. Then we get the following shells (see the figure)

<ul><li>1st shell: 2 states (n = 0, j = ⁠1/2⁠).</li>

<li>2nd shell: 6 states (n = 1, j = ⁠1/2⁠ or ⁠3/2⁠).</li>

<li>3rd shell: 12 states (n = 2, j = ⁠1/2⁠, ⁠3/2⁠ or ⁠5/2⁠).</li>

<li>4th shell: 8 states (n = 3, j = ⁠7/2⁠).</li>

<li>5th shell: 22 states (n = 3, j = ⁠1/2⁠, ⁠3/2⁠ or ⁠5/2⁠; n = 4, j = ⁠9/2⁠).</li>

<li>6th shell: 32 states (n = 4, j = ⁠1/2⁠, ⁠3/2⁠, ⁠5/2⁠ or ⁠7/2⁠; n = 5, j = ⁠11/2⁠).</li>

<li>7th shell: 44 states (n = 5, j = ⁠1/2⁠, ⁠3/2⁠, ⁠5/2⁠, ⁠7/2⁠ or ⁠9/2⁠; n = 6, j = ⁠13/2⁠).</li>

<li>8th shell: 58 states (n = 6, j = ⁠1/2⁠, ⁠3/2⁠, ⁠5/2⁠, ⁠7/2⁠, ⁠9/2⁠ or ⁠11/2⁠; n = 7, j = ⁠15/2⁠).</li></ul>

and so on.

Note that the numbers of states after the 4th shell are doubled triangular numbers plus two. Spin–orbit coupling causes so-called 'intruder levels' to drop down from the next higher shell into the structure of the previous shell. The sizes of the intruders are such that the resulting shell sizes are themselves increased to the next higher doubled triangular numbers from those of the harmonic oscillator. For example, 1f2p has 20 nucleons, and spin–orbit coupling adds 1g9/2 (10 nucleons), leading to a new shell with 30 nucleons. 1g2d3s has 30 nucleons, and adding intruder 1h11/2 (12 nucleons) yields a new shell size of 42, and so on.

The magic numbers are then

and so on. This gives all the observed magic numbers and also predicts a new one (the so-called <a href="Island_of_stability" title="Island of stability">island of stability</a>) at the value of 184 (for protons, the magic number 126 has not been observed yet, and more complicated theoretical considerations predict the magic number to be 114 instead).

Another way to predict magic (and semi-magic) numbers is by laying out the idealized filling order (with spin–orbit splitting but energy levels not overlapping). For consistency, s is split into j = ⁠1/2⁠ and j = −⁠1/2⁠ components with 2 and 0 members respectively. Taking the leftmost and rightmost total counts within sequences bounded by / here gives the magic and semi-magic numbers.

<ul><li>s(2,0)/p(4,2) > 2,2/6,8, so (semi)magic numbers 2,2/6,8</li>

The rightmost predicted magic numbers of each pair within the quartets bisected by / are double tetrahedral numbers from the Pascal Triangle: 2, 8, 20, 40, 70, 112, 168, 240 are 2x 1, 4, 10, 20, 35, 56, 84, 120, ..., and the leftmost members of the pairs differ from the rightmost by double triangular numbers: 2 − 2 = 0, 8 − 6 = 2, 20 − 14 = 6, 40 − 28 = 12, 70 − 50 = 20, 112 − 82 = 30, 168 − 126 = 42, 240 − 184 = 56, where 0, 2, 6, 12, 20, 30, 42, 56, ... are 2 × 0, 1, 3, 6, 10, 15, 21, 28, ... .

<div class="mw-heading mw-heading3"><h3 id="Other_properties_of_nuclei">Other properties of nuclei</h3></div>

This model also predicts or explains with some success other properties of nuclei, in particular <a href="Spin_(physics)" title="Spin (physics)">spin</a> and <a href="Parity_(physics)" title="Parity (physics)">parity</a> of nuclei <a href="Ground_state" title="Ground state">ground states</a>, and to some extent their <a href="Excited_state" title="Excited state">excited nuclear states</a> as well. Take 17 8O (<a href="Oxygen-17" title="Oxygen-17">oxygen-17</a>) as an example: Its nucleus has eight protons filling the first three proton "shells", eight neutrons filling the first three neutron "shells", and one extra neutron. All protons in a complete proton shell have zero total <a href="Angular_momentum" title="Angular momentum">angular momentum</a>, since their angular momenta cancel each other. The same is true for neutrons. All protons in the same level (n) have the same parity (either +1 or −1), and since the parity of a pair of particles is the product of their parities, an even number of protons from the same level (n) will have +1 parity. Thus, the total angular momentum of the eight protons and the first eight neutrons is zero, and their total parity is +1. This means that the spin (i.e. angular momentum) of the nucleus, as well as its parity, are fully determined by that of the ninth neutron. This one is in the first (i.e. lowest energy) state of the 4th shell, which is a d-shell (ℓ = 2), and since p = (−1)ℓ, this gives the nucleus an overall parity of +1. This 4th d-shell has a j = ⁠5/2⁠, thus the nucleus of 17 8O is expected to have positive parity and total angular momentum ⁠5/2⁠, which indeed it has.

The rules for the ordering of the nucleus shells are similar to <a href="List_of_Hund's_rules" class="mw-redirect" title="List of Hund's rules">Hund's Rules</a> of the atomic shells, however, unlike its use in atomic physics, the completion of a shell is not signified by reaching the next n, as such the shell model cannot accurately predict the order of excited nuclei states, though it is very successful in predicting the ground states. The order of the first few terms are listed as follows: 1s, 1p⁠3/2⁠, 1p⁠1/2⁠, 1d⁠5/2⁠, 2s, 1d⁠3/2⁠... For further clarification on the notation refer to the article on the Russell–Saunders <a href="Term_symbol" title="Term symbol">term symbol</a>.

For nuclei farther from the <a href="Magic_number_(physics)" title="Magic number (physics)">magic quantum numbers</a> one must add the assumption that due to the relation between the <a href="Strong_nuclear_force" class="mw-redirect" title="Strong nuclear force">strong nuclear force</a> and total angular momentum, <a href="Proton" title="Proton">protons</a> or <a href="Neutron" title="Neutron">neutrons</a> with the same n tend to form pairs of opposite angular momentum. Therefore, a nucleus with an even number of protons and an even number of neutrons has 0 spin and positive parity. A nucleus with an even number of protons and an odd number of neutrons (or vice versa) has the parity of the last neutron (or proton), and the spin equal to the total angular momentum of this neutron (or proton). By "last" we mean the properties coming from the highest energy level.

In the case of a nucleus with an odd number of protons and an odd number of neutrons, one must consider the total angular momentum and parity of both the last neutron and the last proton. The nucleus parity will be a product of theirs, while the nucleus spin will be one of the possible results of the <a href="Angular_momentum#Addition_of_quantized_angular_momenta" title="Angular momentum">sum</a> of their angular momenta (with other possible results being excited states of the nucleus).

The ordering of angular momentum levels within each shell is according to the principles described above – due to spin–orbit interaction, with high angular momentum states having their energies shifted downwards due to the deformation of the potential (i.e. moving from a harmonic oscillator potential to a more realistic one). For nucleon pairs, however, it is often energetically favourable to be at high angular momentum, even if its energy level for a single nucleon would be higher. This is due to the relation between angular momentum and the <a href="Strong_nuclear_force" class="mw-redirect" title="Strong nuclear force">strong nuclear force</a>.

The <a href="Nuclear_magnetic_moment" title="Nuclear magnetic moment">nuclear magnetic moment</a> of neutrons and protons is partly predicted by this simple version of the shell model. The magnetic moment is calculated through j, ℓ and s of the "last" nucleon, but nuclei are not in states of well-defined ℓ and s. Furthermore, for <a href="Odd-odd_nuclei" class="mw-redirect" title="Odd-odd nuclei">odd-odd nuclei</a>, one has to consider the two "last" nucleons, as in <a href="Deuterium#Magnetic_and_electric_multipoles" title="Deuterium">deuterium</a>. Therefore, one gets several possible answers for the nuclear magnetic moment, one for each possible combined ℓ and s state, and the real state of the nucleus is a <a href="Superposition_principle" title="Superposition principle">superposition</a> of them. Thus the real (measured) nuclear magnetic moment is somewhere in between the possible answers.

The <a href="Electric_dipole" class="mw-redirect" title="Electric dipole">electric dipole</a> of a nucleus is always zero, because its <a href="Ground_state" title="Ground state">ground state</a> has a definite parity. The matter density (ψ2, where ψ is the <a href="Wavefunction" class="mw-redirect" title="Wavefunction">wavefunction</a>) is always invariant under parity. This is usually the situation with the <a href="Dipole#Atomic_dipoles" title="Dipole">atomic electric dipole</a>.

Higher electric and magnetic <a href="Multipole_moments" class="mw-redirect" title="Multipole moments">multipole moments</a> cannot be predicted by this simple version of the shell model for reasons similar to those in the case of <a href="Deuterium#Magnetic_and_electric_multipoles" title="Deuterium">deuterium</a>.

<div class="mw-heading mw-heading2"><h2 id="Including_residual_interactions">Including residual interactions</h2></div>

For nuclei having two or more valence nucleons (i.e. nucleons outside a closed shell), a residual two-body interaction must be added. This residual term comes from the part of the inter-nucleon interaction not included in the approximative average potential. Through this inclusion, different shell configurations are mixed, and the energy degeneracy of states corresponding to the same configuration is broken.<a href="#cite_note-5">[5]</a><a href="#cite_note-Coraggio2009-6">[6]</a>

These residual interactions are incorporated through shell model calculations in a truncated model space (or valence space). This space is spanned by a basis of many-particle states where only single-particle states in the model space are active. The Schrödinger equation is solved on this basis, using an effective Hamiltonian specifically suited for the model space. This Hamiltonian is different from the one of free nucleons as, among other things, it has to compensate for excluded configurations.<a href="#cite_note-Coraggio2009-6">[6]</a>

One can do away with the average potential approximation entirely by extending the model space to the previously inert core and treating all single-particle states up to the model space truncation as active. This forms the basis of the no-core shell model, which is an <a href="Ab_initio_methods_(nuclear_physics)" title="Ab initio methods (nuclear physics)">ab initio method</a>. It is necessary to include a <a href="Three-body_force" title="Three-body force">three-body interaction</a> in such calculations to achieve agreement with experiments.<a href="#cite_note-barrett2013-7">[7]</a>

<div class="mw-heading mw-heading2"><h2 id="Collective_rotation_and_the_deformed_potential">Collective rotation and the deformed potential</h2></div>

In 1953 the first experimental examples were found of rotational bands in nuclei, with their energy levels following the same J(J+1) pattern of energies as in rotating molecules. Quantum mechanically, it is impossible to have a collective rotation of a sphere, so this implied that the shape of these nuclei was non-spherical. In principle, these rotational states could have been described as coherent superpositions of particle-hole excitations in the basis consisting of single-particle states of the spherical potential. But in reality, the description of these states in this manner is intractable, due to a large number of valence particles—and this intractability was even greater in the 1950s when computing power was extremely rudimentary. For these reasons, <a href="Aage_Bohr" title="Aage Bohr">Aage Bohr</a>, <a href="Ben_Mottelson" class="mw-redirect" title="Ben Mottelson">Ben Mottelson</a>, and <a href="Sven_G%C3%B6sta_Nilsson" title="Sven Gösta Nilsson">Sven Gösta Nilsson</a> constructed models in which the potential was deformed into an ellipsoidal shape. The first successful model of this type is now known as the <a href="Nilsson_model" title="Nilsson model">Nilsson model</a>. It is essentially the harmonic oscillator model described in this article, but with anisotropy added, so the oscillator frequencies along the three Cartesian axes are not all the same. Typically the shape is a prolate ellipsoid, with the axis of symmetry taken to be z. Because the potential is not spherically symmetric, the single-particle states are not states of good angular momentum J. However, a Lagrange multiplier <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle -\omega \cdot J}">

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<annotation encoding="application/x-tex">{\displaystyle -\omega \cdot J}</annotation>

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</math><img src="./f33261166836a770e962973d7d5f3dbce489fb10.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.505ex; width:6.404ex; height:2.343ex;" alt="{\displaystyle -\omega \cdot J}" loading="lazy">, known as a "cranking" term, can be added to the Hamiltonian. Usually the angular frequency vector ω is taken to be perpendicular to the symmetry axis, although tilted-axis cranking can also be considered. Filling the single-particle states up to the Fermi level produces states whose expected angular momentum along the cranking axis <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle \langle J_{x}\rangle }">

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<annotation encoding="application/x-tex">{\displaystyle \langle J_{x}\rangle }</annotation>

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</math><img src="./6bbcaac0da3e7d24e53adb7125f3770c44dc292c.svg" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.838ex; width:4.272ex; height:2.843ex;" alt="{\displaystyle \langle J_{x}\rangle }" loading="lazy"> is the desired value.

<div class="mw-heading mw-heading2"><h2 id="Related_models">Related models</h2></div>

<a href="Igal_Talmi" title="Igal Talmi">Igal Talmi</a> developed a method to obtain the information from experimental data and use it to calculate and predict energies which have not been measured. This method has been successfully used by many nuclear physicists and has led to a deeper understanding of nuclear structure. The theory which gives a good description of these properties was developed. This description turned out to furnish the shell model basis of the elegant and successful <a href="Interacting_boson_model" title="Interacting boson model">interacting boson model</a>.

A model derived from the nuclear shell model is the alpha particle model developed by <a href="Henry_Margenau" title="Henry Margenau">Henry Margenau</a>, <a href="Edward_Teller" title="Edward Teller">Edward Teller</a>, J. K. Pering, <a href="Tony_Skyrme" title="Tony Skyrme">T. H. Skyrme</a>, also sometimes called the <a href="Skyrme_model" class="mw-redirect" title="Skyrme model">Skyrme model</a>.<a href="#cite_note-8">[8]</a><a href="#cite_note-9">[9]</a> Note, however, that the Skyrme model is usually taken to be a model of the nucleon itself, as a "cloud" of mesons (pions), rather than as a model of the nucleus as a "cloud" of alpha particles.

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<ul><li><a href="Nuclear_structure" title="Nuclear structure">Nuclear structure</a></li>

<li><a href="Table_of_nuclides" title="Table of nuclides">Table of nuclides</a></li>

<li><a href="Semi-empirical_mass_formula" title="Semi-empirical mass formula">Semi-empirical mass formula</a></li>

<li><a href="Isomeric_shift" title="Isomeric shift">Isomeric shift</a></li>

<li><a href="Interacting_boson_model" title="Interacting boson model">Interacting boson model</a></li></ul>

<div class="mw-heading mw-heading2"><h2 id="References">References</h2></div>

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</style><cite class="citation web cs1"><a rel="nofollow" class="external text" href="http://hyperphysics.phy-astr.gsu.edu/hbase/nuclear/shell.html">"Shell Model of Nucleus"</a>. HyperPhysics.</cite>

</li>

<li id="cite_note-nobel1963-2"><a href="#cite_ref-nobel1963_2-0">^</a> <cite class="citation book cs1"><a rel="nofollow" class="external text" href="https://www.nobelprize.org/prizes/physics/1963/ceremony-speech/">Nobel Lectures, Physics 1963-1970</a>. Amsterdam, Netherlands: Elsevier Publishing Company. 1972. Retrieved May 19, 2023.</cite>

</li>

<li id="cite_note-3"><a href="#cite_ref-3">^</a> <cite id="CITEREFOzawaKobayashiSuzukiYoshida2000" class="citation journal cs1">Ozawa, A.; Kobayashi, T.; Suzuki, T.; Yoshida, K.; Tanihata, I. (2000). "New Magic Number, N=16, near the Neutron Drip Line". Physical Review Letters. 84 (24): 5493–5. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2000PhRvL..84.5493O">2000PhRvL..84.5493O</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1103%2FPhysRevLett.84.5493">10.1103/PhysRevLett.84.5493</a>. <a href="PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/10990977">10990977</a>.</cite> (this refers to the <a href="Nuclear_drip_line" title="Nuclear drip line">nuclear drip line</a>)

</li>

<li id="cite_note-4"><a href="#cite_ref-4">^</a> <cite id="CITEREFWangAudiKondevHuang2017" class="citation journal cs1">Wang, Meng; Audi, G.; Kondev, F. G.; Huang, W.J.; Naimi, S.; Xu, Xing (March 2017). "The AME2016 atomic mass evaluation (II). Tables, graphs and references". Chinese Physics C. 41 (3): 030003. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2017ChPhC..41c0003W">2017ChPhC..41c0003W</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1088%2F1674-1137%2F41%2F3%2F030003">10.1088/1674-1137/41/3/030003</a>. <a href="Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/11858%2F00-001M-0000-0010-23E8-5">11858/00-001M-0000-0010-23E8-5</a>. <a href="ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1674-1137">1674-1137</a>.</cite>

</li>

<li id="cite_note-5"><a href="#cite_ref-5">^</a> <cite id="CITEREFCaurierMartínez-PinedoNowackiPoves2005" class="citation journal cs1">Caurier, E.; Martínez-Pinedo, G.; Nowacki, F.; Poves, A.; Zuker, A. P. (2005). "The shell model as a unified view of nuclear structure". Reviews of Modern Physics. 77 (2): 427–488. <a href="ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/nucl-th/0402046">nucl-th/0402046</a>. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005RvMP...77..427C">2005RvMP...77..427C</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1103%2FRevModPhys.77.427">10.1103/RevModPhys.77.427</a>. <a href="S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:119447053">119447053</a>.</cite>

</li>

<li id="cite_note-Coraggio2009-6">^ <a href="#cite_ref-Coraggio2009_6-0">a</a> <a href="#cite_ref-Coraggio2009_6-1">b</a> <cite id="CITEREFCoraggioCovelloGarganoItaco2009" class="citation journal cs1">Coraggio, L.; Covello, A.; Gargano, A.; Itaco, N.; Kuo, T.T.S. (2009). "Shell-model calculations and realistic effective interactions". Progress in Particle and Nuclear Physics. 62 (1): 135–182. <a href="ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/0809.2144">0809.2144</a>. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2009PrPNP..62..135C">2009PrPNP..62..135C</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.ppnp.2008.06.001">10.1016/j.ppnp.2008.06.001</a>. <a href="S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:18722872">18722872</a>.</cite>

</li>

<cite id="CITEREFBarrettNavrátilVary2013" class="citation journal cs1">Barrett, B. R.; Navrátil, P.; Vary, J. P. (2013). "Ab initio no core shell model". Progress in Particle and Nuclear Physics. 69: 131–181. <a href="ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/0902.3510">0902.3510</a>. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2013PrPNP..69..131B">2013PrPNP..69..131B</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.ppnp.2012.10.003">10.1016/j.ppnp.2012.10.003</a>.</cite>

</li>

<li id="cite_note-8"><a href="#cite_ref-8">^</a> <cite id="CITEREFSkyrme1961" class="citation journal cs1">Skyrme, T. H. R. (February 7, 1961). "A Non-Linear Field Theory". Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences. 260 (1300): 127–138. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1961RSPSA.260..127S">1961RSPSA.260..127S</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1098%2Frspa.1961.0018">10.1098/rspa.1961.0018</a>. <a href="S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:122604321">122604321</a>.</cite>

</li>

<li id="cite_note-9"><a href="#cite_ref-9">^</a> <cite id="CITEREFSkyrme1962" class="citation journal cs1">Skyrme, T. H. R. (March 1962). "A unified field theory of mesons and baryons". Nuclear Physics. 31: 556–569. <a href="Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1962NucPh..31..556S">1962NucPh..31..556S</a>. <a href="Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2F0029-5582%2862%2990775-7">10.1016/0029-5582(62)90775-7</a>.</cite>

</li>

</ol></div></div>

<div class="mw-heading mw-heading2"><h2 id="Further_reading">Further reading</h2></div>

<ul><li><cite id="CITEREFTalmide-Shalit1963" class="citation book cs1">Talmi, Igal; de-Shalit, A. (1963). Nuclear Shell Theory. Academic Press. <a href="ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <bdi>978-0-486-43933-4</bdi>.</cite> <code class="cs1-code">{{cite book}}</code>: ISBN / Date incompatibility (help)</li>

<li><cite id="CITEREFTalmi1993" class="citation book cs1">Talmi, Igal (1993). Simple Models of Complex Nuclei: The Shell Model and the Interacting Boson Model. Harwood Academic Publishers. <a href="ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <bdi>978-3-7186-0551-4</bdi>.</cite></li></ul>

<div class="mw-heading mw-heading2"><h2 id="External_links">External links</h2></div>

<ul><li><cite class="citation audio-visual cs1">Igal Talmi (November 24, 2010). <a rel="nofollow" class="external text" href="http://ribf.riken.jp/Lecture/Talmi-24Nov2010/">On single nucleon wave functions</a>. RIKEN Nishina Center.</cite></li></ul></div><div><div class="zim-footer">

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