Transmission and Reflection Coefficients

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SUMMARY

The discussion focuses on the computation of reflection and transmission coefficients for a quantum particle encountering a step potential defined by V(x) = 0 for x < 0 and Vb > 0 for x ≥ 0. The participants derive the wave functions for both regions using the Schrödinger equation and apply boundary conditions to calculate the probability current densities. The transmission coefficient (T) and reflection coefficient (R) are defined in terms of these currents. Additionally, a user seeks clarification on imposing boundary conditions to eliminate incoming waves in numerical simulations.

PREREQUISITES
  • Understanding of the Schrödinger equation and its applications in quantum mechanics
  • Familiarity with wave functions and boundary conditions in quantum systems
  • Knowledge of reflection and transmission coefficients in quantum mechanics
  • Basic concepts of Fourier analysis for wave decomposition
NEXT STEPS
  • Study the derivation of reflection and transmission coefficients in quantum mechanics
  • Learn about boundary conditions in quantum systems and their implications
  • Explore numerical methods for solving the Schrödinger equation, particularly in potential barriers
  • Investigate the use of Fourier analysis in quantum mechanics for wavefunction manipulation
USEFUL FOR

Quantum physicists, students of quantum mechanics, and researchers working on numerical simulations of quantum systems will benefit from this discussion.

stunner5000pt
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Consider the step potential defined by
V(x) = 0 if x < 0
Vb > 0 if x=> 0

a) Compute te relfection and tranmission coefficients for a particle of energy E > Vb approaching from th left

For x < 0
Schrödinger equaion since V = 0
-\frac{\hbar^2}{2m} \frac{\partial^2 \psi}{\partial x^2} = E \psi(x)

\frac{\partial^2 \psi}{\partial x^2} = -\frac{2mE}{\hbar^2} \psi(x)

define k_{1}^2 = \frac{2mE}{\hbar^2}

\frac{\partial^2 \psi}{\partial x^2} = -k^2 \psi(x)

\psi(x) = A \cos(k_{1}x) + B \sin(k_{1} x)

for x=> 0
-\frac{\hbar^2}{2m} \frac{\partial^2 \psi}{\partial x^2} = (E-V_{B}) \psi(x)
k_{2}^2 = \frac{2m}{\hbar^2} (E - V_{B})
\frac{\partial^2 \psi}{\partial x^2} = k_{2}^2 \psi(x)
\psi_(x) = C \exp(ik_{2} x) + D\exp(-ik_{2}x)
but we only care about the one with the negative exponential
hence C = 0
\psi_(x) = D\exp(-ik_{2}x)

are these solutions correct? I am just afraid i may have made a stupid mistake by switching the negative sign somewhere :(

ok to proceed i apply the boundary conditions s.t.

\psi_{I}(0) = \psi_{T}(0)
\psi_{I}&#039;(0) = \psi_{T}&#039;(0)

we calculate probability current density j

j_{trans} = \frac{\hbar k_{2}}{m} |D|^2
j _{inc} = \frac{\hbar k_{1}}{m} |A|^2
j_{refl} = \frac{\hbar k_{1}}{m} |B|^2

and transmission coefficient is calculated like this

T = \left| \frac{j_{trans}}{j_{inc}} \right|
R = \left| \frac{j_{refl}}{j_{inc}} \right|

thank you for your input
 
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stunner5000pt said:
Consider the step potential defined by
V(x) = 0 if x < 0
Vb > 0 if x=> 0

a) Compute te relfection and tranmission coefficients for a particle of energy E > Vb approaching from th left

For x < 0
Schrödinger equaion since V = 0
-\frac{\hbar^2}{2m} \frac{\partial^2 \psi}{\partial x^2} = E \psi(x)

\frac{\partial^2 \psi}{\partial x^2} = -\frac{2mE}{\hbar^2} \psi(x)

define k_{1}^2 = \frac{2mE}{\hbar^2}

\frac{\partial^2 \psi}{\partial x^2} = -k^2 \psi(x)

\psi(x) = A \cos(k_{1}x) + B \sin(k_{1} x)

for x=> 0
-\frac{\hbar^2}{2m} \frac{\partial^2 \psi}{\partial x^2} = (E-V_{B}) \psi(x)
k_{2}^2 = \frac{2m}{\hbar^2} (E - V_{B})
\frac{\partial^2 \psi}{\partial x^2} = k_{2}^2 \psi(x)
\psi_(x) = C \exp(ik_{2} x) + D\exp(-ik_{2}x)
but we only care about the one with the negative exponential
hence C = 0
\psi_(x) = D\exp(-ik_{2}x)

are these solutions correct? I am just afraid i may have made a stupid mistake by switching the negative sign somewhere :(
You want a wave traveling to the right so you must keep the C wavefunction and set D =0.

Patrick
 
Sorry to resurrect a long dead thread, but if i wanted to impose the condition D = 0, ie incoming waves only from one direction on standing wave computed numerically, how would i go about doing that? I know Fourier analysis can give me the momentum components, but that's about it. Would i have to do it in the time dependent case?
 
Say you have a wave incident from the left. The wavefunction would be

ψI = A*Exp(ik1x)+B*Exp(-ik1x) in region I (x ≤ 0)
ψII = C*Exp(ik2x) in region II (x ≥ 0)

You have an incident and reflected wave in region I (constants A and B respectively) and a transmitted wave in region II. Of course, you have to impose the proper boundary conditions at x=0.

For a lovely simulation of this and potential barriers in general, you may wish to go to
http://phet.colorado.edu/en/simulation/quantum-tunneling
 
I understand that perfectly from an analytic point of view, but what I've got is the equation (actually want to do the KG equation but good to start with Schrod) with a set of boundary conditions, mass of the particle and potential and that's it. I then solve numerically and get a standing wave. It is in this process that i am unsure as to how to impose the correct condition to kill the other incoming wave. In fact, I'm really lost because essentially mathematica will spit out what are essentially shifted cos waves in either regime, which when you take a Fourier transform will have momentum components in both directions, both with equal magnitude (as you expect from a cosine/sine wave). I thought perhaps a Fourier decomposotion would pull out the momentum components and i could kill them off accordingly but it didnt work really :(

thanks!
-G
 

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