Spherical harmonics and P operator

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Discussion Overview

The discussion revolves around the properties of the parity operator P applied to spherical harmonics, specifically examining the relationship P|lm⟩ = (-1)^l |lm⟩. Participants explore the implications of this relationship, including mathematical proofs and counterexamples, within the context of quantum mechanics and angular momentum.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • Some participants define the operator P as P φ(𝑟) = φ(-𝑟) and inquire about proving its effect on spherical harmonics.
  • Others challenge the validity of the proposed relationship, providing specific examples, such as |1 1⟩, to illustrate discrepancies in the expected outcome.
  • One participant explains how spherical harmonics are derived from associated Legendre functions and azimuthal exponentials, detailing how parity transformations affect these components.
  • Another participant suggests that the parity operator acts on spherical coordinates as P ψ(r, θ, φ) = ψ(r, π - θ, φ + π), questioning the correctness of this transformation.
  • Some participants express a desire for a more intuitive or physical proof of the parity relationship, rather than relying solely on mathematical formulas.
  • A later reply discusses the implications of Schur's lemma, stating that parity does not depend on the quantum number m but only on l, and proposes testing the m=0 spherical harmonic to determine parity.
  • Another participant notes that all spherical harmonics with m ≠ 0 can be derived from the m=0 case, reinforcing the argument that examining the m=0 harmonic suffices for understanding parity behavior.

Areas of Agreement / Disagreement

Participants express disagreement regarding the validity of the relationship P|lm⟩ = (-1)^l |lm⟩, with some providing counterexamples and others supporting the original claim through mathematical reasoning. The discussion remains unresolved, with multiple competing views presented.

Contextual Notes

Some limitations include the dependence on specific definitions of spherical harmonics and the assumptions made regarding the transformations under the parity operator. The discussion also highlights the complexity of the mathematical relationships involved.

paweld
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Let's define operator P:
<br /> P \phi(\vec{r})=\phi(-\vec{r})<br />

Does anyone know simple and elegant prove that P|lm\rangle = (-1)^l |lm\rangle
(|lm\rangle is spherical harmonic).
 
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paweld said:
Let's define operator P:
<br /> P \phi(\vec{r})=\phi(-\vec{r})<br />

Does anyone know simple and elegant prove that P|lm\rangle = (-1)^l |lm\rangle
(|lm\rangle is spherical harmonic).

I don't think this is true.

Take:
<br /> |1 1\rangle = -(3/(8\pi))^{(1/2)}sin(\theta)e^{i\phi}<br />
<br /> P|1 1\rangle = (3/(8\pi))^{(1/2)}sin(\theta)e^{-i\phi}<br />

The \phi component screws up the relation.
 
The spherical harmonics are a product of the associated Legendre function P_{l}^{m}(x) and the azimuthal exponential. Under parity (r, \theta, \phi) changes to (r,\pi-\theta, \phi\pm\pi), which means that cos \theta changes to -cos \theta

From Rodrigos formula P_{l}^{m}(x) \mbox{ }\alpha \mbox{ } (1-x^2)^{\frac{m}{2}} \frac{d^{l+m}}{dx^{l+m}}(1-x^2)^l

where x is cos \theta. Under x-->-x this changes by (-1)^{m+l}. However, the azimuthal exponential changes by: e^{i m (\phi \pm \pi)}=(-1)^m e^{i m \phi}.

Multiplying the azimuthal and polar parts together, the result changes by (-1)^{l+m}(-1)^m=(-1)^l
 
ygolo said:
I don't think this is true.

Take:
<br /> |1 1\rangle = -(3/(8\pi))^{(1/2)}sin(\theta)e^{i\phi}<br />
<br /> P|1 1\rangle = (3/(8\pi))^{(1/2)}sin(\theta)e^{-i\phi}<br />

The \phi component screws up the relation.

In spherical coordinates P acts as follows:
<br /> P \psi(r,\theta,\phi)=\psi(r,\pi-\theta,\phi+\pi)<br />
(Am I right?)
So:
<br /> P|1 1\rangle = -(3/(8\pi))^{(1/2)}sin(\pi-\theta)e^{-i(\phi+\pi)} =- |1 1\rangle<br />
 
paweld said:
In spherical coordinates P acts as follows:
<br /> P \psi(r,\theta,\phi)=\psi(r,\pi-\theta,\phi+\pi)<br />
(Am I right?)
So:
<br /> P|1 1\rangle = -(3/(8\pi))^{(1/2)}sin(\pi-\theta)e^{-i(\phi+\pi)} =- |1 1\rangle<br />

Ah, OK. Thanks for the correction. I was going outside the domain of \theta and \phi and the \phi transformation was just wrong.
 
Last edited:
RedX said:
The spherical harmonics are a product of the associated Legendre function P_{l}^{m}(x) and the azimuthal exponential. Under parity (r, \theta, \phi) changes to (r,\pi-\theta, \phi\pm\pi), which means that cos \theta changes to -cos \theta

From Rodrigos formula P_{l}^{m}(x) \mbox{ }\alpha \mbox{ } (1-x^2)^{\frac{m}{2}} \frac{d^{l+m}}{dx^{l+m}}(1-x^2)^l

where x is cos \theta. Under x-->-x this changes by (-1)^{m+l}. However, the azimuthal exponential changes by: e^{i m (\phi \pm \pi)}=(-1)^m e^{i m \phi}.

Multiplying the azimuthal and polar parts together, the result changes by (-1)^{l+m}(-1)^m=(-1)^l

Maybe someone knows more "physical" prove? I mean prove which doesn't use of explicite formlua for spherical harmonics.
 
RedX said:
The spherical harmonics are a product of the associated Legendre function P_{l}^{m}(x) and the azimuthal exponential. Under parity (r, \theta, \phi) changes to (r,\pi-\theta, \phi\pm\pi), which means that cos \theta changes to -cos \theta

From Rodrigos formula P_{l}^{m}(x) \mbox{ }\alpha \mbox{ } (1-x^2)^{\frac{m}{2}} \frac{d^{l+m}}{dx^{l+m}}(1-x^2)^l

where x is cos \theta. Under x-->-x this changes by (-1)^{m+l}. However, the azimuthal exponential changes by: e^{i m (\phi \pm \pi)}=(-1)^m e^{i m \phi}.

Multiplying the azimuthal and polar parts together, the result changes by (-1)^{l+m}(-1)^m=(-1)^l

Maybe someone knows more "physical" prove? I mean prove which doesn't use explicite formlua for spherical harmonics.
 
paweld said:
Maybe someone knows more "physical" prove? I mean prove which doesn't use explicite formlua for spherical harmonics.

Parity and rotations commute (why?). Since parity and rotations commute, by Schur's lemma that means all states of total angular momentum \ell have the same parity. So parity does not depend on the quantum number 'm', but only '\ell' (if you're not familiar with Schur's lemma then the fact that rotations commute with parity implies that angular momentum commutes with parity, so the raising and lowering operators that are built from the angular momentum operators commute with parity - therefore states with different m but same \ell have the same parity). An easy test for parity is to test the m=0 or m=\ell spherical harmonic. The m=0 spherical harmonic coincides exactly with the Legendre function, which is odd if \ell is odd and even if \ell is even.

The important point is that you can test m=anything to determine the parity for all \ell. The spherical harmonics for m=\ell takes on the simple form: sin^{\ell} \theta e^{i\ell \phi} and that's all you have to test for parity.
 
All spherical harmonics with m ne 0 can be obtained by rotation and linear combination from the one with m=0 so it is sufficient to look at the function with m=0 (thats the Schur's lemma stuff of RedX). The harmonic with m=0 and l can be obtained from z^l by orthogonalization to the functions with l'<l. As under parity z->-z, the function transforms as z^l ->(-z)^l.
 

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