Charge Independence and Pauli Exclusion Principle

In summary: L=0?2) S=1?Thanks a lot.In summary, the conversation discusses the concept of charge independence and how it relates to the force between nucleons in a nucleus. The textbook mentioned states that the average neutron-proton attraction is greater than the average neutron-neutron or proton-proton attraction. This is explained as a consequence of the Pauli Exclusion Principle, which affects the spin and isospin configurations of nucleon pairs. It is also mentioned that the nucleon-nucleon force is charge independent but isospin dependent, leading to different interactions for different isospin values. This is why the bound deuteron state is only possible for a neutron-proton pair.
  • #1
vertices
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I remember reading about charge independence; about how the energy levels of mirror nuclei (correcting for differences in the colomb term) are identical… I think this suggests that the force between any two nucleons is the same, so the attraction of neutron-proton=proton-proton=neutron-neutron.

One of my textbooks states the following:

"The average neutron-proton attraction in a nucleus is greater than the average neutron-neutron or proton-proton attraction, essentially as a consequence of Pauli Exclusion Principle."

questions:

1)is the textbook right about the force between n-p not being equal to p-p or n-n?

2)Can someone explain how Pauli EP is relavent here?

I've tried reasoning it in my head, but I'm getting confused: I probably don't know what I'm talking about but n-p has an antisymetric isospin (right?), therefore the space wavefunction has to be symetric? Is this relavent?

Thanks in advance:)
 
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  • #2
vertices said:
I remember reading about charge independence; about how the energy levels of mirror nuclei (correcting for differences in the colomb term) are identical… I think this suggests that the force between any two nucleons is the same, so the attraction of neutron-proton=proton-proton=neutron-neutron.

One of my textbooks states the following:

"The average neutron-proton attraction in a nucleus is greater than the average neutron-neutron or proton-proton attraction, essentially as a consequence of Pauli Exclusion Principle."

questions:

1)is the textbook right about the force between n-p not being equal to p-p or n-n?

2)Can someone explain how Pauli EP is relavent here?

I've tried reasoning it in my head, but I'm getting confused: I probably don't know what I'm talking about but n-p has an antisymetric isospin (right?), therefore the space wavefunction has to be symetric? Is this relavent?

Thanks in advance:)

They are including the effect of the "exchange force" (which is not really a force in the conventional sense of the word). However I don't quite understand how they draw a conclusion without saying something about spin. Assuming that they are talking about ground state and that the pp (or nn) are in the triplet state (so symmetric) the spatial wavefunction must be antisymmetric which shows up as an apparent repulsive force.
But again, this depends on the spin configuration. So it sounds a bit strange (or rather incomplete) to me.
 
  • #3
Thanks for your reply nrqed. I think I understand why the n-p force does not equal p-p or n-n (but I may be way off the mark).

just to clarify can I write:

[tex]\Psi=\psi(spacial)\psi(spin)\psi(isospin)[/tex]?

I don't know much about isopin to be honest, so I'm not sure if I am applying it rightly.

I would think a p-p or n-n pair must have an antisymettric spin wf because of Pauli EP ((I[tex]_{z}[/tex] must point up and down). Now, isospin has to be symettric (for p-p or n-n). So for the overall wf to be antisymettric (as they must be for fermions), the spatial wf must be antisymettric. So if the spatial wf is antisym, there's less overlap, so the binding energy is less.

For n-p, isospin can be sym eg. (2^-0.5){|p>[tex]_{1}[/tex]|n>[tex]_{2}[/tex] +|n>[tex]_{1}[/tex] |p>[tex]_{2}[/tex] } OR antisym eg. |n>[tex]_{1}[/tex] |p>[tex]_{2}[/tex]; therefore the spatial wf can be EITHER sym or antisym. So if spatial wf is sym, the binding energy is more.

Does this reasoning make sense?
 
  • #4
duplicate post - deleted.
 
  • #5
Yes the nuclear force is charge independent, but it is isospin dependent.

"The NN-force is to a very large extent charge independent. This means that the
interaction is the same for the same isospin T regardless of the T_3 value. This means
also that the interaction is not the same when T = 0 and T = 1. For example, the np- interaction
is different when the pair couples to T = 0 compared to when they couple
to T = 1. In the T = 0 (S = 1) case the np-pair is bound to a deuteron, while in the T =
1 (S = 0) case the np-pair is unbound. Note also that disregarding from the Coulomb
interaction, the pp- and nn-interaction is the same since these states both have T = 1."

From my lecture notes in Nuclear physics
 
  • #6
vertices said:
"The average neutron-proton attraction in a nucleus is greater than the average neutron-neutron or proton-proton attraction, essentially as a consequence of Pauli Exclusion Principle."

questions:

1)is the textbook right about the force between n-p not being equal to p-p or n-n?

2)Can someone explain how Pauli EP is relevant here?
1) Yes.
2) The nucleon-nucleon force is a bit more attractive in the L=0, spin one state than in the spin zero state. Because of the Pauli principle, n-p can exist in the L=0, spin one state, while p-p and n-p can't. Incidentally that is why the bound deuteron state is only n-p.
 
  • #7
malawi_glenn said:
Yes the nuclear force is charge independent, but it is isospin dependent.

"The NN-force is to a very large extent charge independent. This means that the
interaction is the same for the same isospin T regardless of the T_3 value. This means
also that the interaction is not the same when T = 0 and T = 1. For example, the np- interaction
is different when the pair couples to T = 0 compared to when they couple
to T = 1. In the T = 0 (S = 1) case the np-pair is bound to a deuteron, while in the T =
1 (S = 0) case the np-pair is unbound. Note also that disregarding from the Coulomb
interaction, the pp- and nn-interaction is the same since these states both have T = 1."

From my lecture notes in Nuclear physics

thanks malawi_glen. I think this has cleared it up!
 
  • #8
pam said:
1) Yes.
2) The nucleon-nucleon force is a bit more attractive in the L=0, spin one state than in the spin zero state. Because of the Pauli principle, n-p can exist in the L=0, spin one state, while p-p and n-p can't. Incidentally that is why the bound deuteron state is only n-p.

thanks pam.

what do you mean by "spin one" the case of n-p? I mean, n and p have separate nuclear wells do they not? Are you talking about isospin?

And sorry for might be a stupid question but why is the nucleon-nucleon force more attractive when L=0?
 
  • #9
When L = 0 it means that the particles have no relative angular momenta and it should then correspond to the lowest lying state since higher angular momenta usally means that energy must go to give the particle relative motion (this was a very rough explanation altough)

the (bound) n-p system have J = 1 and S = 1, these two can be deduced from experiment, and it is easy to work out the L from theory and then test it by comparing it with the magnetic moment of the deutron (which can be measured).

Now the isospin follows the same algebra as ordinary spin, so according to Pauli you must couple L,S & T so that the total wave function is anti-symmetric, so it is straightforward to obtain the possible configurations of S,L and T. Then you perform experiments and find out what components you have in the N-N potential.

So the force is charge independent, but due to Pauli - the n-p system (with J=1 & S = 1)is the only 2 nucleon system) etc.
 
  • #10
thanks glenn!
 

What is charge independence?

Charge independence is a fundamental principle in physics that states that the properties and behavior of a system should remain unchanged if all particles in the system are replaced with their antiparticles, with their charges reversed.

What is the Pauli exclusion principle?

The Pauli exclusion principle is a fundamental principle in quantum mechanics that states that no two identical fermions (particles with half-integer spin) can occupy the same quantum state simultaneously. This means that two electrons, for example, cannot occupy the same energy level in an atom.

Why is charge independence important?

Charge independence is important because it allows us to understand and predict the behavior of systems at a fundamental level. It is a key principle in the Standard Model of particle physics and helps us understand the symmetries and interactions between particles and antiparticles.

How does the Pauli exclusion principle affect the structure of atoms?

The Pauli exclusion principle plays a crucial role in determining the electron configuration of atoms. It dictates that each electron in an atom must have a unique set of quantum numbers, which leads to the formation of discrete energy levels and the distinct electronic structure of atoms.

What happens if the Pauli exclusion principle is violated?

If the Pauli exclusion principle is violated, it would result in a breakdown of our current understanding of the behavior of matter at a fundamental level. It would also have significant implications for the stability and structure of atoms, which could ultimately affect the properties of the world around us.

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