What is nuclear symmetry energy?

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SUMMARY

The discussion centers on nuclear symmetry energy, which is defined as the energy required to increase the asymmetry between neutrons (N) and protons (Z) in a nucleus. The energy density in the nuclear medium is expressed as a Taylor series, with the symmetry energy approximately equal to 29 ± 2 MeV. The asymmetry parameter α is crucial in this context, and its squared term appears in the energy density expansion due to quantum-mechanical effects, particularly the exclusion principle. The Strutinsky smearing technique is also mentioned, highlighting the importance of distinguishing between classical and quantum-mechanical energy contributions.

PREREQUISITES
  • Understanding of nuclear physics concepts, specifically the strong force and its symmetry properties.
  • Familiarity with the asymmetry parameter α = (N-Z)/A in nuclear physics.
  • Knowledge of energy density functions in the context of nuclear medium.
  • Basic grasp of quantum mechanics, particularly the exclusion principle and its implications for nuclear binding energy.
NEXT STEPS
  • Research the Strutinsky smearing technique and its application in nuclear physics.
  • Study the implications of the exclusion principle on nuclear binding energies.
  • Explore the relationship between nuclear symmetry energy and neutron star stability.
  • Investigate advanced topics in energy density functional theory in nuclear physics.
USEFUL FOR

Physicists, nuclear engineers, and students specializing in nuclear physics or quantum mechanics who seek to deepen their understanding of nuclear binding energies and symmetry energy concepts.

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in a nutshell
 
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The strong force which is binding in nuclei is symmetric under the exchange neutron <-> proton (or down <-> up). There are other forces, for instance the electromagnetic repulsion between two protons, which are not binding and not symmetric. As the name suggests, the non-symmetric part is only a perturbation. So, using the asymmetry parameter
\alpha = \frac{N-Z}{A}
and the density \rho, we develop the energy density in the nuclear medium E(\rho,\alpha) as a Taylor series
E(\rho,\alpha) = E(\rho,0) + S(\rho)\alpha^2 + O(\alpha^4) + \cdots
and expanding around the saturation density \rho_s
S(\rho) = \left.\frac{1}{2}\frac{\partial^2 E}{\partial\alpha^2}\right|_{\alpha=0,\rho=\rho_s}=a_v+\frac{p_0}{\rho_s^2}(\rho-\rho_s)+\cdots
The symmetry energy a_v\approx 29 \pm 2 MeV

source : The nuclear symmetry energy
 
So, is it useful to think of it as the energy required to increase the asymmetry between N and Z in the nucleus, say, by electron capture?
 
why in the symmetry energy only squared asymmetry parameter are exist and there is not the first power of asymmetry parameter?
 
Calculate the average potential energy of a brick in a brick wall of height N. Calculate the same for a wall of height Z. Keep the sum of the height A = Z + N fixed but allow their difference (N - Z) to be a free parameter. Find out the dependency of the total energy on that free parameter.
 
dauto said:
Calculate the average potential energy of a brick in a brick wall of height N. Calculate the same for a wall of height Z. Keep the sum of the height A = Z + N fixed but allow their difference (N - Z) to be a free parameter. Find out the dependency of the total energy on that free parameter.

Nice explanation. I would add that this topic is a little subtle because often we want to use these liquid-drop energies in the Strutinsky smearing technique, where we add in a quantum-mechanical shell correction. When we do that, we have two terms in the energy, classical and quantum-mechanical. We have to be careful not to double-count a particular energy in both the classical and the quantum-mechanical term (Strutinsky shell correction). As dauto correctly explains, the asymmetry energy is a quantum-mechanical effect arising from the exclusion principle. So you would think you should include it only in the quantum-mechanical term. However, the Strutinsky technique for, say, the neutrons, only adds a correction that represents the difference in binding energy between nucleus (N,Z) and the average of other nuclei (N+x,Z), where x is small, and this correction vanishes when the levels are uniformly spaced. So clearly the effect as described by dauto is not included in the Strutinsky correction, because it would occur even if the levels were uniformly spaced.
 

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