The triple Dirac delta-function well: getting KAPPA

  • Thread starter Thread starter Lylo
  • Start date Start date
  • Tags Tags
    Dirac
Lylo
Messages
4
Reaction score
1

Homework Statement



I will try to be light on the math as I am just now getting into using LaTex, and I don't want things to get too ugly from me not using it.

Hello there,

I found a thread here on PF concerning a triple delta-function potential well problem, which was a bit informative. However, my quantum professor wants us to solve several problems related to such a potential, introducing the non-dimensionalizing substitution s = x/a to 'scale the variables', resulting in the problem specified by

d2Ψ/ds2 - (ħ2/2ma2) g[∂(s) + ∂(s-1) + ∂(s+1)]Ψ = εΨ ,

where we see our scaled energy in epsilon, and g is a constant integer which describes the delta function's "strength".

I am having some trouble getting to a useful kappa, as I have done for the double potential well. I feel as though I am overlooking something very 'obvious' yet crucial to obtaining the transcendental equation for kappa, so I hope maybe someone else can offer some hints.

Homework Equations



Manifestly there exist four distinct regions of finite potentials; at s=±1 and s=0 we have the delta wells. In a previous assignment we demonstrated that the even solutions can be written as

eks
for s<-1

Beks + Ce-ks
for -1<s<0

Be-ks + Ceks
for 0<s<1

and

e-ks
for 1<s

and that's what I wish to look at here.

We also make use of the continuity equation

## \Delta (\frac{d\psi(s)}{ds})=-g(\psi(s)) ##

and note that our wavefunction must be continuous at the boundaries, and their derivatives are also continuous where their respective wavefunctions are finite (i.e., not at a delta well).

The Attempt at a Solution



Since we expect continuity at s=-1, I will use the first and second wavefunction 'pieces', evaluating them at that point and setting them equal:

## \psi_I(-1) = \psi_I{}_I(-1) ## yields $$ e^k{}^s = Be^k{}^s + Ce^-{}^k{}^s \\ e^-{}^k = Be^-{}^k + Ce^k \rightarrow 1 = B + Ce^2{}^k \rightarrow B = 1 - Ce^2{}^k ;$$
note that we recover this result for s=1, as well. At s=0, we have the unenlightening $$ B+C = B+C .$$
By the by, for good measure we can also write (from our experience with s=-1) $$ C=Be^-{}^2{}^k + e^-{}^2{}^k .$$
We note the discontinuity in ## \psi'(s) ## at, say, s=-1: ## \Delta (\frac{d\psi(1)}{ds})=-g(\psi(1)), ## meaning we need to take derivatives of psi one and psi two, and then subtract the former from the latter: $$ \psi' {}_I{}_I = ke^k{}^s - Ce^2{}^ke^k{}^s(k)-Cke^-{}^k{}^s \\ \psi' {}_I = ke^k{}^s$$ and so we get, after subtracting these two and equating their difference to ## -g\psi(-1) ## $$ -g = -2Cke^2{}^k .$$

It isn't immediately clear to me if this will be useful in getting kappa. I reckon I need to get rid of any B or C dependencies for my final transcendental in kappa, and I have a plethora of what my tyro's eye sees as a "dead-end". Perhaps I have been staring at this stuff for too long. When I did the double delta well problem a year or two ago, I remember some twisty algebra was involved in getting rid of my coefficients in the kappa equation.

Does it look like I am on the right track? Have I missed something, and need a nudge in the right direction? I have always had a bit of trouble playing with groups of equations and trying to construct an equation with only certain components; I am dyslexic so it seems really convoluted to my mind!

Thanks in advance for your help. I'll give this a few re-reads in the hopes that I'll weed out any sneaky typos.

EDIT: I also have tried getting additional equations by exploiting the continuity of the wavefunction's derivatives for finite potentials - i.e., at s=1/2. I am trying to find one of my results doing so, now. If I can find it, I'll add it to the post; if not, I'll do it again when I get time to, provided that it's necessary/useful.
 
Physics news on Phys.org
Hello,

I was going to edit my first post again, but it seems as though I cannot. I cannot find the edit option again, at least.

While walking around campus the day after I posted this, a few ideas hit me which I will be trying out tonight. I also realized some issues with my post, which I will clear up here:

The Schrödinger equation is incorrect, because of an oversight on my part. The potential V(s) is ## \frac{\hbar^2g}{2ma} (η), ## where η denotes the scaled delta-functions; however, the Schrödinger equation becomes $$ \epsilon\psi = \frac{-\partial^2\psi}{\partial s^2} - g[η]\psi $$ and we note that ## \partial(sa) → \frac{1}{|a|}\partial s .## Of course, g ∈ ℤ and is constant.
 
  • Like
Likes BvU
Hello,

I have made some more additions to my list of equations in my efforts for obtaining a transcendental in κ.

Given the wavefunction 'pieces' for the even solutions, we also have: $$ \psi_e = \begin{cases}
κe^{κs} & s < -1\\
κBe^{κs} - κCe^{-κs} & -1 < s < 0\\
-κBe^{-κs} + κCe^{κs} & 0 < s < 1 \\
-κe^{-κs} & 1 <s \\
\end{cases}. $$
Applying the continuity equation about the discontinuity in ## \frac{d\psi}{ds} ## at ## s=0 ## gives:

$$ \begin{cases}
\frac{d\psi}{ds}|_+ =& -κB + κC \\
\frac{d\psi}{ds}|_- =& κB - κC\\

\end{cases} \\ Δ\frac{d\psi}{ds} = (-κB + κC) - (κB - κC) = -2κB + 2κC; \\ \text{or, using } B = 1 - Ce^{2k}: \\ -2κ + 2κCe^{2κ} + 2κC.$$
This implies that $$ -2κ + 2κCe^{2κ} + 2κC = -g(1 - Ce^{2κ} + 2κC), $$
which I obtain as leading to: $$ \frac{2κ}{g} = \frac{1-C(e^{2κ}+1)}{1-C(e^{2κ}-1)}. $$
This is close to an equation involving a ## \tanh 2k ,## but I haven't been able to produce such an equation.

Any tips?

EDIT: I also decided to exploit the continuity of the derivatives of ##\psi## at finite potentials, as well as the symmetry in the wavefunctions about ##s=0:## $$ κBe^{-k/2} - κCe^{k/2} = -(-κBe^{-k/2} + κCe^{κ/2}) → 0 = 0,$$
with an equivalent result for ##\frac{d\psi_I(s<-1)}{ds}## and ##\frac{\psi_{IV}(s>1)}{ds}. ##
 
Last edited:
Hello,

For those who are interested, I finally pieced together something which seems okay for ##\kappa.## Recall from post # 1 that ## g = 2C\kappa e^{2\kappa}; ## using this fact we can also obtain a value for ##C## upon inspection: ## C=\frac{g}{2\kappa}e^{-2\kappa} ##. I have already proven that $$ \frac{2\kappa}{g} = \frac{1-C(e^{2\kappa}+1)}{1-C(e^{2\kappa}-1)}, $$ so implementing our new expression for ##C## into our equation of ##\frac{2\kappa}{g}## yields $$ 2\kappa [1-\frac{g}{2\kappa}(1+e^{-2\kappa})] = g[1-\frac{g}{2\kappa}(1-e^{-2\kappa})].$$

Now, for ##g=5##, Wolfram returns three roots for this transcendental in ##\kappa##:## \begin{align}
\kappa &≈ -2.42392 \\
\kappa &≈ 2.0756 \\
\kappa &≈2.73481
\end{align}.##

We know that ## \kappa = \frac{\sqrt{-2mE}}{\hbar};## so for our case in epsilon (## \epsilon=\frac{2mEa^2}{\hbar^2} ##): ## \kappa = \frac{\sqrt{\frac{-2m \hbar^2 \epsilon}{2ma^2}}}{a} \rightarrow \kappa = \frac{\sqrt{- \epsilon}}{a}.##

The only restriction for ##\kappa## is ##\kappa ∈ ℝ.## Our ##\epsilon ## is assumed to be ## < 0.## It is trivial to show that ## - \epsilon = a^2\kappa^2 \rightarrow \epsilon = -a^2\kappa^2.## The negative sign ensures we always recover a negative value for ## \epsilon ## notwithstanding the sign of ## \kappa.## So, it looks like our three ##\kappa##'s are in favor of three bound states at ##g=5.##
 
Last edited:
Thread 'Need help understanding this figure on energy levels'
This figure is from "Introduction to Quantum Mechanics" by Griffiths (3rd edition). It is available to download. It is from page 142. I am hoping the usual people on this site will give me a hand understanding what is going on in the figure. After the equation (4.50) it says "It is customary to introduce the principal quantum number, ##n##, which simply orders the allowed energies, starting with 1 for the ground state. (see the figure)" I still don't understand the figure :( Here is...
Thread 'Understanding how to "tack on" the time wiggle factor'
The last problem I posted on QM made it into advanced homework help, that is why I am putting it here. I am sorry for any hassle imposed on the moderators by myself. Part (a) is quite easy. We get $$\sigma_1 = 2\lambda, \mathbf{v}_1 = \begin{pmatrix} 0 \\ 0 \\ 1 \end{pmatrix} \sigma_2 = \lambda, \mathbf{v}_2 = \begin{pmatrix} 1/\sqrt{2} \\ 1/\sqrt{2} \\ 0 \end{pmatrix} \sigma_3 = -\lambda, \mathbf{v}_3 = \begin{pmatrix} 1/\sqrt{2} \\ -1/\sqrt{2} \\ 0 \end{pmatrix} $$ There are two ways...
Back
Top