Semi Empirical Mass Formula - Liquid Drop Model of the Nucleus

Semi-Empirical Mass Formula [Bethe-Weizsäcker Formula]

Derivation and Explanation
Statement:
The Semi‑Empirical Mass Formula (SEMF) gives the nuclear binding energy \(B(A,Z)\) of a nucleus with mass number \(A\) and atomic number \(Z\) as the sum of five macroscopic terms derived from the liquid‑drop model:
Formula :
\[B(A,Z)=a_V A - a_S A^{2/3} - a_C \frac{Z(Z-1)}{A^{1/3}} - a_A \frac{(A-2Z)^2}{A} + \delta(A,Z)\]
Sometimes the Coulomb term is written as \(a_C \dfrac{Z^2}{A^{1/3}}\) and the pairing term \(\delta\) has the usual form given below.

Derivation: Physical origin of each term :

Semi‑Empirical Mass Formula Bethe Weizsacker Formula

Volume term \(a_V A\) :

The nucleus behaves like an incompressible liquid drop. Each nucleon binds with a roughly constant number of nearest neighbours, so binding energy is proportional to \(A\). Hence \(a_V A\) with \(a_V>0\).


Surface term \(-a_S A^{2/3}\) :

Nucleons at the surface have fewer neighbours and so contribute less binding. Surface area scales as \(A^{2/3}\), giving a negative correction \(-a_S A^{2/3}\).


Coulomb term \(-a_C Z(Z-1)/A^{1/3}\) :

Protons repel by Coulomb force. Approximating the nucleus as a uniformly charged sphere of radius \(R\propto A^{1/3}\) leads to electrostatic energy \(\propto Z^2/R \sim Z^2/A^{1/3}\). The factor \(Z(Z-1)\) corrects for self‑interaction.


Asymmetry (or Pauli) term \(-a_A (A-2Z)^2/A\) :

Quantum mechanically, neutrons and protons fill Fermi levels. Minimum energy occurs when \(N\approx Z\) for small nuclei. Deviation from symmetric \(N=Z\) costs kinetic (Fermi) energy, producing a term quadratic in \(N-Z\): since \(N=A-Z\), this becomes \((A-2Z)^2/A\).


Pairing term \(\delta(A,Z)\) :

Because of pairing, nuclei with even numbers of protons and neutrons are extra stable. Empirical form: \[\delta(A,Z)=\begin{cases} +a_P A^{-1/2} & \text{even-}Z,\,\text{even-}N\\ -a_P A^{-1/2} & \text{odd-}Z,\,\text{odd-}N\\ 0 & \text{if } A \text{ is odd}\end{cases}\] This term is small and alternates sign depending on nucleon parity.


Notes on coefficients and units :
Typical fitted values(approximately): \(a_V = 15.5 \, MeV\)
\(a_S = 17.0 \, MeV\)
\(a_C = 0.71 \, MeV\)
\(a_A = 23.0 \, MeV\)
\(a_P = 11.0 \, MeV\)

These are empirical — obtained by fitting measured nuclear masses.

Short derivation sketch for asymmetry term :

Treat protons and neutrons as independent Fermi gases. Fermi energy scales as \(E_F\propto (n)^{2/3}\) where density \(n\) differs when \(N\ne Z\). Expanding the total kinetic energy to second order in the neutron excess gives an energy contribution \(\propto (N-Z)^2/A\), producing the asymmetry term shown above.

Example / application & remarks :

Binding energy per nucleon \(B/A\) predicted by SEMF peaks near \(A\sim 56\), explaining iron‑group stability and why heavy nuclei fission while light nuclei fuse. SEMF also predicts approximate mass parabolae and decay energetics (Q‑values) qualitatively well.

Anomalous Zeeman Effect and Paschen-Back Effect

Anomalous Zeeman Effect

Zeeman and Paschen Back Effect Diagram
Definition:
The Anomalous Zeeman Effect is the splitting of spectral lines into more than three components when an atom is placed in an external magnetic field, typically observed in atoms having unpaired electron spin and non-zero total angular momentum.

Explanation :

  1. In the normal Zeeman effect only orbital angular momentum is considered and energy levels split into three (a triplet) because of simple magnetic interaction.
  2. Most atoms, however, have both orbital L and spin S angular momenta which couple to give total angular momentum J. The interaction with the magnetic field depends on the Landé g-factor (gJ), not just on orbital motion.
  3. Each atomic level splits into (2J + 1) magnetic sublevels labelled by mJ, producing multiple components in the observed spectral lines. Selection rules (ΔmJ = 0, ±1) determine which transitions are allowed, giving a complex pattern of π and σ lines.
  4. The anomalous effect thus reveals the role of electron spin and the vector coupling of L and S, and was historically important evidence for the existence of electron spin and for quantum theory.

Key formula:

\[\Delta E = \mu_B\, g_J\, B\, m_J\]

where \(\mu_B\) is the Bohr magneton, \(B\) is the magnetic field, \(g_J\) is the Landé g-factor, and \(m_J\) is the magnetic quantum number.

Paschen Back Effect :

In very strong magnetic fields, the coupling between orbital angular momentum \(L\) and spin \(S\) breaks down. The magnetic interaction becomes dominant compared to spin orbit coupling, causing \(L\) and \(S\) to align independently with the field. This leads to a simpler splitting pattern than the anomalous Zeeman effect, similar to the normal Zeeman effect.

This occurs When magnetic energy \(\mu_B B\) is much greater than spin orbit interaction energy.

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Threshold Energy For Nuclear Reaction

Threshold Energy in Nuclear Reactions

Nuclear Reaction Diagram

In nuclear physics, the threshold energy is the minimum kinetic energy that a projectile particle must possess in order to make a particular nuclear reaction occur.

Definition

The threshold energy for a nuclear reaction is defined as the minimum energy of the incoming particle required to overcome the energy difference between the reactants and the products, ensuring the reaction can proceed while conserving both energy and momentum.

Explanation

If a reaction absorbs energy (i.e., it is endothermic), the projectile must supply not only this reaction energy but also additional energy to satisfy momentum conservation. Thus, the actual threshold energy is slightly higher than the reaction’s Q-value (when Q is negative).

Threshold Energy (Eth) = −Q × (1 + ma / MA)

where Q is the reaction energy, ma is the mass of the projectile, and MA is the mass of the target nucleus.

Example

In the reaction p + ³H → ³He + n, if the reaction Q-value is negative, the proton must have at least the threshold energy computed from the above relation for the reaction to take place.

Summary

The concept of threshold energy helps determine the minimum energy requirement for initiating endothermic nuclear reactions and plays a vital role in nuclear reactor design and particle accelerator physics.