Expansion of position kets in terms of angular momentum

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Discussion Overview

The discussion revolves around the expansion of position kets in quantum mechanics, specifically the representation of the state ##|x,y,z\rangle## in terms of angular momentum eigenstates ##|l,m\rangle##. Participants explore the implications of Hamiltonian symmetry on the ability to separate radial and angular components of wave functions, addressing both theoretical and conceptual aspects of this topic.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants assert that while eigenvectors of an observable form a complete basis, the position ket ##|x,y,z\rangle## can only be partially expanded in terms of the angular momentum eigenstates ##|l,m\rangle##, specifically the angular-dependent part, leaving the radial part unexpanded.
  • Others propose that if the Hamiltonian allows for the separation of radial and angular variables, the wave function can be expressed as a sum of radial-dependent coefficients and spherical harmonics, indicating that the radius part is represented by these coefficients.
  • A participant questions whether the inability to fully expand ##|x,y,z\rangle## in terms of ##|l,m\rangle## is related to the degrees of freedom, noting that ##|x,y,z\rangle## has three degrees while ##|l,m\rangle## has two.
  • Another participant elaborates on the conditions under which the Hamiltonian's symmetry permits the separation of variables, emphasizing that different systems (e.g., hydrogen-like atoms vs. diatomic molecules) may require different bases for expansion based on their symmetries.
  • There is a discussion about the implications of commuting operators with the Hamiltonian and how this affects the choice of basis for wave function expansion.

Areas of Agreement / Disagreement

Participants express differing views on the conditions necessary for expanding position kets in terms of angular momentum eigenstates. There is no consensus on the implications of Hamiltonian symmetry or the relationship between degrees of freedom and the ability to perform such expansions.

Contextual Notes

Limitations include the dependence on the specific symmetry of the Hamiltonian and the unresolved nature of how different systems may affect the expansion process. The discussion highlights the complexity of transitioning between Cartesian and spherical coordinates in quantum mechanics.

hokhani
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TL;DR
Why we cannot expand entirely the position kets in ##|l,m\rangle## ?
As far as I know, in QM, the eigenvectors of an observable form a complete base. However, in the expansion of ##|x,y,x\rangle## in terms of the eigenvectors of angular momentum operators ##L^2## and ##L_z## , i.e., ##|l,m\rangle##, we can only expand the angular dependent part of ##|x,y,x\rangle## in terms of ##|l,m\rangle## and the radius part cannot be expanded! Any help is appreciated.
 
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If the symmetry of the Hamiltonian allows separating the radial and angular variables, then you can think of the wave function
$$
\psi(r, \vartheta, \varphi) = \sum_{l,m} c_l(r) Y_{lm}(\vartheta, \varphi)
$$
as being expanded in the ##Y_{lm}(\vartheta,\varphi) \equiv \langle \vartheta, \varphi|l,m\rangle## basis, with radial-dependent coefficients ##c_l(r)## (that have to be determined by solving the "leftover" radial Schrödinger equation). So the radius part
hokhani said:
(...) the radius part cannot be expanded!
is just the radial-dependent expansion coefficient. That being said, the transformation from Cartesian to spherical coordinates (or to any other curvilinear coordinates, for that matter) is one of the examples in which the rigid use of the Dirac bra-ket notation leads to confusion.
 
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div_grad said:
If the symmetry of the Hamiltonian allows
Do you mean that, in general, if the system doesn't have the required symmetry, then we cannot expand ##|x,y,z\rangle## in terms of ##|l,m\rangle##?
Isn't it related to the number of degrees of freedom (DOF) so that for ##|x,y,z\rangle##there are three DOF while two for ##|l,m\rangle##?
 
hokhani said:
TL;DR Summary: Why we cannot expand entirely the position kets in ##|l,m\rangle## ?

As far as I know, in QM, the eigenvectors of an observable form a complete base. However, in the expansion of ##|x,y,x\rangle## in terms of the eigenvectors of angular momentum operators ##L^2## and ##L_z## , i.e., ##|l,m\rangle##, we can only expand the angular dependent part of ##|x,y,x\rangle## in terms of ##|l,m\rangle## and the radius part cannot be expanded! Any help is appreciated.
You can always do the expansion but you need to indicate a radial basis, angles are not enough.
 
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hokhani said:
Do you mean that, in general, if the system doesn't have the required symmetry, then we cannot expand ##|x,y,z\rangle## in terms of ##|l,m\rangle##?
The quantum system is defined by its Hamiltonian ##H##, and the appropriate wave function satisfies the Schrödinger equation ##\mathrm{i} \hbar \partial_t \Psi(q, t) = H \Psi(q, t)## - I denote by ##q## the set of all coordinates on which ##\Psi## depend. Now, if the Hamiltonian does not depend explicitly on time, then the first separation-of-variables that you can do is put ##\Psi(q, t) = \psi(q) \exp\left\{-\mathrm{i}Et/\hbar\right\}## and solve the eigenvalue problem ##H\psi(q) = E\psi(q)##. There are various ways in which you can solve such problems, for example using some variational principle or numerically-exact propagators. One effective way of simplifying the solution of the eigenvalue problem is to use basis expansions. In the case of the time-independent Schrödinger equation, you look for the operators ##A_i## which commute with the Hamiltonian, ##\left[H, A_i\right]=0##, because then the eigenvectors of ##A_i## are simultaneously the eigenvectors of ##H## - and, in general, it is way easier to find the eigenvectors of the appropriate ##A_i## than to find the eigenvector ##\psi(q)## of the total Hamiltonian.

For example, if the symmetry of the Hamiltonian ##H## is such that the angular momentum operators ##L^2## and ##L_z## commute with ##H##, then you can find the eigenvectors of ##L^2## and ##L_z## - which are the spherical harmonics ##|l,m\rangle## - and expand ##|\psi\rangle## in the basis of these eigenvectors (the expansion coefficients themselves depend on the radial variables). The problem is thus simplified because, in this case, the angular variables have been effectively separated-out from ##H\psi(q) = E\psi(q)##. This is the case, e.g., for the hydrogen-like atoms, where you have the spherically-symmetric potential energy ##V(r)##. But in the case of, say, diatomic molecules, the potential is no longer spherically-symmetric because of the existence of "privileged" direction in space, defined by the internuclear axis. In this case, ##H## commutes with ##L_z## - the angular momentum projection onto the internuclear "z-axis" - but it does not commute with ##L^2##. So the basis in which you expand the wave function of a diatomic molecule is different from ##|l, m\rangle##.

For spatial-homogeneous systems, the momentum operator commutes with ##H## and you can therefore expand the wave function in the basis of momentum eigenfunctions - which is effectively the Fourier transform of ##\psi(q)##. And so on, and so forth. It all depends on the symmetry of the Hamiltonian and on the set of mutually commuting operators ##A_i## that also commute with ##H##.
 
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hokhani said:
Isn't it related to the number of degrees of freedom (DOF) so that for ##|x,y,z\rangle##there are three DOF while two for ##|l,m\rangle##?
Yes, it is. For a single free particle, the wave function in Cartesian variables would be written as a product ##f_x(x) f_y(y) f_z(z)## of functions depending solely on one of the three coordinates. And in the spherical coordinates, the free-particle wave function would likewise be a product ##f_r(r) f_{\vartheta}(\vartheta) f_{\varphi}(\varphi)##. So indeed, if you "separate-out" the angular variables (by using spherical harmonics) then you're still left with the radial function ##f_r(r)##. This is why the expansion coefficients depend on ##r## when you expand total wave function in the basis of solely-angle-dependent functions like ##|l,m\rangle##.
 
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