[Quantum mechanics] Step barrier |R|^2 and |T|^2

Aaron7
Messages
12
Reaction score
0

Homework Statement



There is a step barrier at x=0, V_0 > E
I am given:
ψi = e^i(kx−ωt) --->
ψr = R e^i(−kx−ωt) <---

ψt = T e^(−αx−iωt) --->

Part of question I am confused about: State the two boundary conditions satisfied by the wave function at x = 0 and hence find expressions for |R|^2 and |T|^2

Homework Equations


N/A


The Attempt at a Solution


I have already worked out an equation for alpha in the previous part.

ψ1 = ψi + ψr
ψ2 = ψt

I started to apply the conditions ψ1(0) = ψ2(0) to get 1 + R = T
and d/dx ψ1(0) = d/dx ψ2(0) to get ik - iRk = -αT

I solved the above to get R = (ik +αT) / ik with T = 1 + R etc
I understand that |R|^2 = R x R* and |T|^2 = T x T*
However I am told that T = 1 - R since these are probability coefficients. Do I solve with T = 1-R (probability coefficients) or T = 1+R (using ψ1(0) = ψ2(0))? I am confused which one to use and why.

Many thanks.
 
Physics news on Phys.org
Aaron7 said:
ψi = e^i(kx−ωt) --->
ψr = R e^i(−kx−ωt) <---

ψt = T e^(−αx−iωt) --->

ψ1 = ψi + ψr
ψ2 = ψt

I started to apply the conditions ψ1(0) = ψ2(0) to get 1 + R = T
and d/dx ψ1(0) = d/dx ψ2(0) to get ik - iRk = -αT

However I am told that T = 1 - R since these are probability coefficients.
Well, ask yourself: should you expect the wavefunction to violate the Schrodinger equation at x=0, and if so, why?

The probability interpretation only makes since with respect to a normalization, usually the L2 norm for wavefunctions. Unfortunately, the friendly plane wave that makes naive calculations so simple wreaks havoc on the L2 norm. (Plane waves for free particles actually live in a different kind of quantum space than normalizable/quantized wavefunctions.) I don't know what you mean by calling R and T "probability coefficients", but I believe that your equations for R and T (the ones that you derived) are correct (assuming that the wavefunction obeys the Schrodinger equation, which T = 1 - R would actually violate at x = 0).

I think it doesn't even make sense to compare |R|2 to |T|2 as probabilities, because I think that the probability of transmission is zero, but I will have to think back to my QM (and that is a long way back).
 
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
The value of H equals ## 10^{3}## in natural units, According to : https://en.wikipedia.org/wiki/Natural_units, ## t \sim 10^{-21} sec = 10^{21} Hz ##, and since ## \text{GeV} \sim 10^{24} \text{Hz } ##, ## GeV \sim 10^{24} \times 10^{-21} = 10^3 ## in natural units. So is this conversion correct? Also in the above formula, can I convert H to that natural units , since it’s a constant, while keeping k in Hz ?
Back
Top