Free particle in spherical polar coords

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SUMMARY

The discussion focuses on solving the time-independent Schrödinger equation for a free particle in spherical polar coordinates, specifically with an azimuthal quantum number of l=0. The radial equation simplifies to \(\frac{d^2u}{dr^2}=-k^2u\), leading to the solution \(u = A\sin(kr) + B\cos(kr)\). To ensure a normalizable wavefunction, it is determined that \(B=0\), resulting in the radial wavefunction \(R(r) = \frac{A}{r}\sin(kr)\). Normalization involves integrating the squared modulus of \(R(r)\) over the volume element \(dv = r^2 \sin\theta dr d\theta d\varphi\), accounting for the factor of \(4\pi\) from angular integration.

PREREQUISITES
  • Understanding of the time-independent Schrödinger equation
  • Familiarity with spherical polar coordinates
  • Knowledge of wavefunction normalization techniques
  • Basic concepts of quantum mechanics, including azimuthal quantum numbers
NEXT STEPS
  • Study the normalization of wavefunctions in quantum mechanics
  • Learn about the Dirac delta function and its applications in quantum mechanics
  • Explore the implications of angular momentum in quantum systems
  • Investigate the solutions to the Schrödinger equation in different coordinate systems
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Students and professionals in quantum mechanics, particularly those studying wavefunctions and the Schrödinger equation in spherical coordinates. This discussion is beneficial for anyone looking to deepen their understanding of quantum particle behavior in three-dimensional space.

cscott
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Homework Statement



Consider the time-independent Schrödinger equation in spherical polar coordinates for a free particle, in the case where we have an azimuthal quantum number [itex]l=0[/itex].

(a) Solve the radial equation to find the (unnormalized) radial wavefunction [itex]R(r)[/itex].
(b) Normalize [itex]R(r)[/itex], using the definition of the dirac delta function [itex]\delta(k'-k)[/itex].

Homework Equations



Radial Equation:

[tex]u(r) = rR(r)[/tex]

[tex]-\frac{\hbar^2}{2m}\frac{d^2u}{dr^2} + \left[V + \frac{\hbar^2}{2m}\frac{l(l+1)}{r^2}\right]u = Eu[/tex]

The Attempt at a Solution



For a free particle, [itex]V=0[/itex], and with [itex]l = 0[/itex] the radial equation reduces to,

[tex]\frac{d^2u}{dr^2}=-k^2u,~~k=\frac{\sqrt{2mE}}{\hbar}[/tex],

with solution,

[tex]u = A\sin(kr) + B\cos(kr)[/tex],

but [itex]u(r)=rR(r)[/itex], so [itex]B=0[/itex] for a normalizable wavefunction (considering r->0). Therefore,

[tex]R(r) = \frac{A}{r}\sin(kr)[/tex]

and to normalize,

[tex]\int_{0}^{\inf} r^2|R(r)|^2~dr = 1[/tex]

[tex]|A|^2 \int_{0}^{\inf} \sin^2(kr)~dr=1[/tex]

How do I use the dirac delta function?
 
Last edited:
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Should I keep [itex]u[/itex] as,

[tex]u(r)=Ae^{ikr}[/tex]

[tex]R(r)=\frac{A}{r}e^{ikr}[/tex]
 
Hi

Sorry, but I don't see why do you need to use the delta of k'-k. I would integrate the sine square but the problem is that you forgot the integration for the angular variables. Thus there is a "4 times pi" factor missed which should be at RHS of the last equation as denominator of 1/(4*pi) since the 4*pi is the result of the integration of

[tex]\int sin\theta d\theta \int d\varphi[/tex]

This comes from the fact that to normalize you have to integrate in a volume whose differential element is

[tex]dv= r^2 sin\theta dr d\theta d\varphi[/tex]

But I don't see anything else to be added.
 

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