Nuclear Shell Model and Schrödinger Equation

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Questions and Answers

What key assumption does the independent particle model make within the context of the nuclear shell model?

  • Nucleons interact strongly with each other through complex potentials.
  • Nucleons are uniformly distributed within the nucleus.
  • The nuclear potential is highly irregular and varies significantly with nucleon position.
  • Each nucleon moves independently in a common potential well. (correct)

What is the significance of the 'magic numbers' (e.g., 2, 8, 20, 28, 50, 82, 126) in nuclear physics?

  • They correspond to nuclei with unusually high stability, analogous to filled electron shells in atoms. (correct)
  • They represent the nucleon numbers at which nuclei are least stable.
  • They indicate nucleon numbers that predict a spherical nucleus.
  • They are arbitrary numbers with no physical significance.

In the context of the nuclear shell model, what does the Woods-Saxon potential aim to improve compared to simpler models like the infinite square well?

  • It completely neglects the interactions between nucleons.
  • It introduces a more realistic potential shape that better approximates the nuclear potential. (correct)
  • It accounts for relativistic effects within the nucleus.
  • It simplifies calculations by assuming a constant potential inside the nucleus.

What does the L⋅S coupling term in the nuclear shell model account for?

<p>The interaction between the spin and orbital angular momentum of nucleons. (B)</p> Signup and view all the answers

If a nucleus has a non-zero quadrupole moment (Q > 0), what can be inferred about its shape?

<p>It is elongated along one axis, like a rugby ball (prolate). (A)</p> Signup and view all the answers

What aspects of nuclei can the shell model explain?

<p>Nuclear properties such as spin, parity, and magnetic moment (B)</p> Signup and view all the answers

What limitation does the shell model have regarding the shape of the nucleus?

<p>It assumes the nucleus is perfectly spherical, which is not always the case (B)</p> Signup and view all the answers

What observation led to the formulation of the nuclear shell model?

<p>Certain nuclei with specific numbers of protons or neutrons exhibited exceptional stability (A)</p> Signup and view all the answers

Why is the infinite square well potential not considered a good approximation for the nuclear potential?

<p>It requires an infinite amount of energy to remove a nucleon from the nucleus. (C)</p> Signup and view all the answers

In the context of L-S coupling, if a level with a specific orbital angular momentum (l) splits into two levels with $j = l + 1/2$ and $j = l - 1/2$, which level lies lower in energy?

<p>The $j = l + 1/2$ level (D)</p> Signup and view all the answers

How is the total energy of the nuclei affected when two nucleons (either two neutrons or two protons) pair up in the same orbital with opposite spins?

<p>The energy of the nucleus decreases, resulting in greater stability. (C)</p> Signup and view all the answers

For nuclei with one unpaired nucleon outside a closed shell, what does the shell model accurately predict?

<p>The spin and parity of the nucleus (D)</p> Signup and view all the answers

What does a non-zero quadrupole moment of a nucleus indicate?

<p>The nucleus deviates from a spherical shape. (C)</p> Signup and view all the answers

According to the content, what is a weakness of the shell model related to its symmetry assumptions?

<p>It assumes a spherically symmetric potential, which is an oversimplification. (C)</p> Signup and view all the answers

If the magic numbers correctly predict the configuration of nucleon numbers as 2, 8, 20, 40, 70, 112, and 168. What parameters are used in this configurations?

<p>Harmonic oscillator potential (D)</p> Signup and view all the answers

Using the boundary condition with $R(r=0) = 0$ and $R(r=r_0) = 0$, what can you say about $r_0$?

<p>$r_0 &gt; 0$ (A)</p> Signup and view all the answers

What are the limitations of the standard shell model?

<p>The shell model struggles to accurately describe excited states. (A)</p> Signup and view all the answers

What is the significance of pairing energy in nuclei?

<p>It reduces the total energy of the nucleus, enhancing stability. (D)</p> Signup and view all the answers

In relation to the shell model, what is the expression that best describes the radial equation for 3D harmonic oscillator potential?

<p>$U(r) = \frac{1}{2} m \omega^2 r^2$ (C)</p> Signup and view all the answers

How does the effect of the potential compare with that is the harmonic oscillator?

<p>Remove the $I$ degeneracy (D)</p> Signup and view all the answers

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Flashcards

Magic Numbers

Numbers of protons or neutrons (2, 8, 20, 28, 50, 82, 126) that result in particularly stable nuclei.

Nuclear Shell Model

A quantum mechanical model that describes the structure of the nucleus in terms of energy levels, analogous to electron shells in atoms.

Common Potential Well

The average potential experienced by a single nucleon due to the presence of all other nucleons in the nucleus.

Orbital Angular Momentum

Labels (s, p, d, f, g, h...) denoting the orbital angular momentum quantum number (l) of nucleons within the nucleus.

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L-S Coupling

Term introduced into the expression for energy, that accounts for the interaction between a particle's spin and its orbital angular momentum.

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Woods-Saxon potential

Single particle potential that has the form Ueff = U(r) − f(r) L.S

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Quadrupole Moment

A measure of the deviation of a nucleus's charge distribution from perfect spherical symmetry.

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Positive Quadrupole Moment

Indicates a prolate shape (elongated along one axis, like a rugby ball).

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Negative Quadrupole Moment

Indicates an oblate shape (flattened, like a discus).

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Study Notes

Nuclear Shell Model

  • Nuclei with proton or neutron numbers 2, 8, 20, 28, 50, 82, and 126 exhibit unique behavior compared to neighboring nuclei, designated as "magic numbers".
  • The shell model explains nuclear properties like spin, parity, and magnetic moment.
  • It is the quantum mechanical form of the independent particle model.
  • The independent particle model assumes nucleons move independently in a common potential well, which is the spherical average of nuclear potential by other nucleons.

Schrödinger Equation

  • Energy Eigen values are derived by solving the Schrödinger equation.
  • 1/r² d/dr(r² d/dr Ψ(r,θ, φ)) + (2μ/ħ²)[E – U(r)]Ψ(r,θ, φ) = 0.
  • Solving the equation requires knowledge about the potential, specifically assuming a well shape for U(r): U(r) = 0 for 0 < r < ro, and U(r) = ∞ for r ≥ ro.
  • With the central potential dependent on r only, and the total wave function dependent on (θ, φ), Ψ(r,θ, φ) = ψ(r) Y™(θ,φ)
  • ψ(r) = R(r)/r, allowing transformation into: -ħ²/2m (d²/dr²) R(r) + [U(r) + ħ²l(l+1)/2mr²] R(r) = ER(r).
  • R(r) represents the radial wave function, where Y™ (θ,φ) are spherical harmonics, and m symbolizes the mass of a nucleon.

Equations for r < ro

  • -ħ²/2m (d²/dr²) R(r) + [ħ²l(l+1)/2mr²] R(r) = ER(r)
  • Solution to the equation: R(r) = rı(K,ro).
  • K = √(2mE/ħ²).
  • Applies the boundary conditions R(r = 0) = 0 and R(r = ro) = 0.
  • rolı(Kro) = 0 where ro ≠ 0 and lı(Kro) ≠ 0

Infinite Square Well Potential

  • The infinite square well potential predicts nucleon numbers 2, 8, 20, 34, 40, 58, 92, and 138, which are not magic numbers.
  • It isn't a good approximation for the nuclear potential.
  • Separating a neutron or proton requires infinite energy.
  • Nuclear shell model labels such as s, p, d, f, g, h... denote the orbital angular momentum quantum number (l) of nucleons in the nucleus where
  • l = 0:s
  • l = 1: p
  • l = 2: d
  • l = 3: f
  • l = 4: g
  • l = 5: h
  • l = 6: i
  • l = 7: j
  • Occupancy = 2(2l + 1)

Harmonic Potential

  • The radial equation for 3D harmonic oscillator potential is given by U(r) = (1/2)mw²r² with boundary conditions U(r = ∞) = 0 and U(r = 0) = 0.
  • (-ħ²/2m d²/dr² + (1/2)mw²r² + ħ²l(l+1)/2mr²)R(r) = ER(r)
  • The boundary condition energy of a nucleon E: E = (2n' + l + 3/2)ħω, involving l = 0, 1, 2... and n' = 0, 1, 2... representing the radial quantum number.
  • E = (N + 3/2)ħω uses the number of modes n in the interval [0,∞], n = n' + 1 = 1,2,3... where N = 2n' + l = 0, 1, 2.......
  • Closed shell configurations of nucleon numbers predicted are 2, 8, 20, 40, 70, 112, and 168 but aren't experimentally obtained magic numbers
  • The harmonic oscillator requires infinite separation and doesn't have a sharp edge.

Woods-Saxon Potential

  • A more realistic model is the Woods-Saxon Model.
  • The Woods–Saxon potential is defined as U(r) = -Uo / (1 + exp((r - R) / a))
  • R = 1.25 A^(1/3)
  • a = 0.52 fm,
  • Uo = 50 MeV
  • This removes the l degeneracy of the magic numbers to the model yields 2, 8, and 20.

L-S Coupling

  • The L-S Coupling was suggested by Mayer, Havel, and Suess.
  • Splitting energy levels are due to spin (S) and orbital angular momentum (L).
  • Spin-orbit coupling introduces L.S term into energy
  • j = l + 1/2 level is below j = l – 1/2 level
  • Splitting increases with l, naturally from L.S form of spin orbit
  • Adjusting the Woods-Saxon Model involves adding a spin-orbit coupling term.
  • Ueff = U(r) − f(r) L.S = -Uo /(1 + exp((r - R) / a)) - f(r) L.S
  • Considering that (ħ²/2) L.S = j(j + 1) – l(l + 1) - s(s + 1) and assuming a nucleon with s = 1/2, when j = (l + 1/2): (ħ²/2) L.S = l

More on L-S Coupling

  • When j = (l - 1/2): (ħ²/2) L.S = -(l + 1)
  • With Ueff = U(r) − f(r)(ħ²/2) {l, if j = l + 1/2 spin up; -(l+1), if j = l − 1/2 spin down},
  • The splitting is larger given larger splitting
  • Sub-level sequences can alter without affecting closed shell configuration and magic numbers; energy levels' sequence in a shell are inferred from experimental data.
  • Proton energies (Z > 20) > neutron energies.
  • Filling order differences exist when Z > 50.
  • Filling order for protons in the 6th shell: 1g9/2, 2d5/2, 1h11/2, 2d3/2, and 3s1/2
  • Filling order for neutrons: 2d5/2, 1g7/2, 1h9/2, 3s1/2, 2d3/2
  • Light nuclei see Columbic interaction as ineffective, leading to almost the same energy level schemes.
  • Larger nuclei have effective Columbic interaction
  • Nucleons fill from bottom up while keeping the nucleus's total energy at a minimum

Spin-Parity of Nuclei

  • The shell model can predict nuclear spin and parity of nuclei in their ground state
  • Nuclei with N and Z both equal to a magic number have a closed configuration.
  • The Pauli Exclusion Principle couples intrinsic spin and orbital angular momentum vectors of the nucleons, giving zero total angular and magnetic momentum, in agreement w/ measured nuclear spin (j).
  • Pauli Exclusion Principle predicts the nucleus' total angular momentum equals the total angular momentum of the unpaired nucleon only when any of the nucleons is one type of nucleon is equal to a magic number and another type is equal to one number above or below the magic number.

Spectroscopic Notation Examples

  • Nitrogen-15 (¹⁵N):
    • p = 7, n = 8, j = 1/2, P = (-1)¹ = -1
    • Spectroscopic notation: ¹⁵N is 1/2⁻
  • Oxygen-17 (¹⁷O):
    • p = 8, n = 9, j = 5/2, P = (-1)² = 1
    • Spectroscopic notation: ¹⁷O is 5/2⁺
  • Carbon-13 (¹³C):
    • p = 6, n = 7, j = 1/2, P = (-1)¹ = -1
    • Spectroscopic notation: ¹³C is 1/2⁻

More on Spectroscopic Notation, Pairing Energy and Quadrupole Moment

  • The "pairing energy" is the phenomenon where energy is reduced when two nucleons (neutrons/protons) pair up in the same energy level with opposing spins. The amount the total energy reduces is of a greater magnitude in larger I states.
  • Nucleons paired in the same orbital with opposite spins have total spin canceled, stabilizing the nucleus.
  • When calculating the formula uses:
  • Q is the quadrupole moment
  • j is the nuclear spin
  • <r²> is the mean square radius of the nucleus
  • For nucleus w/ unpaired nucleons:
  • Q = (2j-1)/(2j+1) <r²> for j = l ± 1/2
  • The shell model strengths: predicts magic numbers, ground-state properties, and single nucleon states for unpaired nucleons outside a closed shell.
  • The shell model weakness: simplifies spherical symmetry

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