Degeneracy of Hydrogen atomic orbitals with different l-values but same n-value

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Discussion Overview

The discussion revolves around the degeneracy of hydrogen atomic orbitals, specifically the 2s and 2p orbitals, as well as the 3s, 3p, and 3d orbitals, which are said to have the same energy due to their dependence on the principal quantum number n. Participants explore the implications of angular momentum and the underlying symmetries of the hydrogen atom's potential on this degeneracy.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant expresses confusion regarding the energy degeneracy of 2s and 2p orbitals, questioning the basis for this degeneracy given their different angular momentum contributions.
  • Another participant explains that the degeneracy is a result of a hidden dynamical symmetry of the 1/r potential, specifically the existence of the Laplace-Lenz-Runge vector, which leads to l-independence in energy levels.
  • A different participant acknowledges the symmetry aspect but maintains that their reasoning about the energy contributions from angular momentum is valid, suggesting that the eigenvalues obtained from the separable Hamiltonian depend only on n.
  • Further clarification is provided regarding the radial functions of orbitals with different l-values, noting the presence of radial nodes and their relationship to centrifugal potential differences.
  • Another participant agrees with the previous points and mentions the complexity of understanding symmetry in parabolic coordinates.

Areas of Agreement / Disagreement

Participants exhibit disagreement regarding the interpretation of angular momentum's effect on energy levels, with some asserting that the degeneracy holds while others question this based on their reasoning. The discussion remains unresolved as multiple competing views are presented.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the separability of the Hamiltonian and the implications of angular momentum on energy eigenvalues, which remain unresolved.

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I am terribly confused. I have always been hearing that in the hydrogen atom, 2s and 2p orbitals have the same energy. Similarly, the 3s, 3p and 3d orbitals have the same energies. This is also suggested by the hydrogen spectrum, my professor also believes the same, and I am unable to find anything against this on the internet.

But what is the basis for this degeneracy?
Upon solving the radial equations for 2s and 2p orbitals, we get the same eigenvalue for Energy, that depends only on the principal quantum number n. However, the wave functions also have an angular part and upon solving the angular equations for 2s and 2p we get a zero value for the 2s (angular momentum=0) and a finite value for 2p (angular momentum=root(2)*hbar). This angular momentum will contribute an extra value of root(2)*hbar/(2*I) to the energy. This will immediately give 2s and 2p different energy values, so they cannot be degenerate.

Have I gone wrong somewhere?
 
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The l-degeneracy, i.e. the fact that E(n,l) = E(n) is l-independent is due to a hidden dynamical symmetry of the 1/r potential which results in an additional conserved quantity, the so-called Laplace-Lenz-Runge vector. The 1/r potential has not only the obvious SO(3) symmetry for spatial rotations but a larger SO(4) symmetry. The existence of the Laplace-Lenz-Runge vector and the l-degeneracy allows one to solve the energy eigenvalue problem algebraically w/o solving the Schrödinger equation (W. Pauli)

Just google for hydrogen atom SO(4) and you will find numerous articles, scripts and presentations. I am pretty sure that we had this disucussion here a couple of times.

Your reasoning regarding the additional l-term in Veff(r) giving the Ylm(Ω) functions a different energy is not correct b/c different l-values also affect the Rnl(r) functions. I think you can't understand the l-degeneracy by just solving the Schrödinger equation (you can derive it, but you don't see the deeper reason)
 
Thanks! :)
I get it, it has got something to do with the symmetry, I'll go and look that up.

However, I still find my reasoning contradictory to this, and I am unable to see any flaw in it.

tom.stoer said:
Your reasoning regarding the additional l-term in Veff(r) giving the Ylm(Ω) functions a different energy is not correct b/c different l-values also affect the Rnl(r) functions. I think you can't understand the l-degeneracy by just solving the Schrödinger equation (you can derive it, but you don't see the deeper reason)

I agree that different l-values affect the R(r) functions, however they don't affect the eigenvalues obtained when the separable hamiltonian acts on R, which depend only on 'n'.
 
To be more specific about the difference of radial functions for orbitals with different l, the 2s orbital has 1 radial node, 2p zero nodes. In general ns has n-1 nodes, np n-2, nd n-3 etc. These additional nodes make up for the lower centrifugal potential of states with lower l as compared to states with higher l.
 
Oh...
thanx! :)
I suppose the hamiltonian need not be separable, after all
 
Tom is correct. The symmetry is more explicit in parabolic coordinates. However, working in parabolic coordinates is not simple.
 

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