A State in the infinite potential well

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The discussion revolves around the appropriate Hilbert space for solutions to the Schrödinger equation in an infinite potential well, specifically addressing the use of L^2[0,L] and C^{\infty}_0(ℝ). While L^2[0,L] is the standard Hilbert space, it does not adequately enforce boundary conditions that require the wavefunction to be zero at the well's edges. The conversation suggests that using a Sobolev-type space like H^1_0[0,L] could better express these conditions, although this approach is not commonly practiced. A specific wavefunction example, ψ(x) = Cx^{1/2}(L-x)^{1/2}, is discussed, highlighting its properties in relation to the Hilbert spaces mentioned. The thread concludes with a numerical evaluation of coefficients for the wavefunction expansion, confirming the feasibility of using energy eigenfunctions for representation.
LagrangeEuler
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General state of the infinite potential well is that ##L^2[0,L]##, where ##L## is well width, or ##C^{\infty}_0(\mathbb{R})##?
 
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Please clarify your question

##\ ##
 
BvU said:
Please clarify your question
I guess that he wants to know the correct Hilbert space for the solutions of the Schrödinger equations for the infinite potential well.
The tricky part is that ##L^2[0,L]## is the correct Hilbert space with respect to the scalar product, but it cannot express the boundary condition that the wavefunction is zero at 0 and at ##L##. Now we could interpret it as a rigged Hilbert space and try to express the boundary condition by using ##H^1_0[0,L]## instead of ##H^1[0,L]##. But I have never seen this being done, and I have no idea whether this would be correct, and whether one really cares about expressing the boundary conditions as part of the rigged Hilbert space.
 
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LagrangeEuler said:
General state of the infinite potential well is that ##L^2[0,L]##, where ##L## is well width, or ##C^{\infty}_0(\mathbb{R})##?

The Hilbert space is indeed ##L^2 [0,L]##, but it is generally too large for arbitrary states, which are regularly in the domain of self-adjointness of the observables. ##C^{\infty}_0(\mathbb{R})## is generally good enough to describe general normalizable states.
According to the boundary conditions, one can have different realizations of the observables, either self-adjoint (case in which a Sobolev-type of space is needed) or not (for example momentum for "hard-walls").
 
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dextercioby said:
The Hilbert space is indeed ##L^2 [0,L]##, but it is generally too large for arbitrary states, which are regularly in the domain of self-adjointness of the observables. ##C^{\infty}_0(\mathbb{R})## is generally good enough.
According to the boundary conditions, one can have different realizations of the observables, either self-adjoint (case in which a Sobolev-type of space is needed) or not (for example momentum for "hard-walls").
Thanks. Yes, for instance is it ##\psi(x)=Cx^{\frac{1}{2}}(L-x)^{\frac{1}{2}}## possible state in the well? I think that this function is ##L^2[0,L]##, but it is not ##C^{\infty}_0(\mathbb{R})## function. Right? Or to rephrase is it possible to write down
\psi(x)=\sum^{\infty}_{n=1}C_n\psi_n(x)
where ##\psi_n(x)=\sqrt{\frac{2}{L}}\sin \frac{n\pi x}{L}##?
 
There's no problem to Fourier transform a piece-wise continuous function. For the functions with the rigid boundary conditions ##\psi(0)=\psi(L)## the given functions ##\pi_n## are a complete set of orthonormalized functions. In this case, since there are no jumps the corresponding Fourier series converges pointwise to the function.

With Mathematica I've found the coefficients (setting ##L=2 \pi## for convenience)
$$C_n=\frac{2 \pi^{3/2}}{n} \text{J}_1(n \pi/2) \sin(n \pi/2).$$
 
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You did not normalize wave function. After normalization you should get that
C_1=\sqrt{3}J_1(\frac{\pi}{2})
however that sum
|C_1|^2+|C_2|^2+...>1.
 
Indeed I just used the unnormalized function ##\psi(x)=\sqrt{x}(2\pi-x)##. Then ##\|\psi\|^2=4 \pi^3/3##, and a numerical evaluation of ##\sum_n |c_n|^2## gives the same. There is no problem with expanding this example wrt. the energy eigenfunctions ##\psi_n=1/\sqrt{\pi} \sin(n x/2)##.

Here is a plot comparing the wave function with the expansion using the first 10 and 20 (in fact only 5 an 10, because every other coefficient is 0)

plot.png
 

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