PlanetPhysics/Schrodinger Equation Wtih Ramp Potential

Here we will investigate [[../TimeIndependentSchrodingerEquation/|time independent Schr\"odinger equation]] with a ramp potential.

$V(x)=kx$

Starting with the S.E

$-\frac{{\hslash }^2}{2m}\frac{d^2\psi (x)}{d{x}^2}+V(x)\psi (x)=\psi (x)E$

substitute the potential in to get

$-\frac{{\hslash }^2}{2m}\frac{d^2\psi (x)}{d{x}^2}+kx\psi (x)=\psi (x)E$

Not sure off hand how to solve this [[../DifferentialEquations/|differential equation]] analytically, so it may be useful to write it in [[../QuantumOperatorAlgebra4/|operator]] form, using the [[../Momentum/|momentum]] operator

$𝐩=-i\hslash \frac{\partial }{\partial x}=\frac{\hslash }{i}\frac{\partial }{\partial x}$

we get

$\frac{1}{2m}[{\left(\frac{\hslash }{i}\frac{\partial }{\partial x}\right)}^2+kx]\psi (x)=E\psi (x)$

Before we choose a method of attack, let us get a feel for the problem at hand. In Figure 1, we plot a potential [[../Bijective/|function]] that goes from $\pm \mathrm{\infty }$. In this example we see the classical turning point at $E=V$, and we should remember that there will be tunneling.

\includegraphics[scale=.4]{RampPot1.eps}

{\mathbf Figure 1:} Open Ramp Potential

This [[../CategoricalGroupRepresentation/|representation]] where $E$ exceeds $V$ on the left side, demonstrates that the [[../Particle/|particle]] would come in from infinity, slow down because of the increase in potential [[../CosmologicalConstant/|energy]] and then reflect back going off into infinity. This results in the so called Scattering State.

However, if in a similar way to the infinite [[../PiecewiseLinear/|square]] well, we say that $V(0)=\mathrm{\infty }$, then we get the potential depicted in Figure 2.

\includegraphics[scale=.4]{RampPot2.eps}

{\mathbf Figure 2:} Open Ramp Potential

For this example, we see that at $V(-\mathrm{\infty })$ and at $V(+\mathrm{\infty })$, $E$ is less than $V$. Therefore, we would get bound states. One more thing to keep in mind is that the square of the [[../CosmologicalConstant2/|wave]] function for these 1D potentials, leads to the [[../Bijective/|relation]] ${|\psi (x)|}^2\approx \frac{{\left|C\right|}^2}{p(x)}$

This tells us that the probability of finding the particle is higher where the potential energy is higher, i.e. higher up the ramp, because here the [[../KineticEnergy/|kinetic energy]] which is related to momentum is low. This makes sense because if the particle is moving fast on the left side of Figure 2 near the infinite potential, you will be less likely to find it here and more likely to find the particle when it is slowed down up the ramp. Next, we should attempt to solve for $\psi$. The three most common ways to attack this [[../Bijective/|type]] of problem are: to solve the differential equation using a [[../Power/|power]] series, use some [[../CoIntersections/|algebraic]] trick similar to the harmonic oscillator or use the WKB method.

All of these techniques would be excellent exercises for students to solve and make good PlanetPhysics entries. Here we will explore the WKB (Wentzel, Kramers, Brillouin) method, which is used to find approximate solutions to the time-independent Schor\"odinger equation for 1D problems. Before we go on, we can look at solutions to a similar problem to guide us. If we have the exact same setup, except that instead of the ramp in Figure 2, we have a harmonic oscillator ramp, where $V(x)=\frac{1}{2}m{\omega }^2{x}^2$ for positive x, the WKB approximation yields

$E_n=(2n-\frac{1}{2})\hslash \omega$

Finally, from [Griffiths] the allowed energies for a general power-law potential

$V(x)=k{\left|x\right|}^m$

is

$E_n=k{\left[(n-\frac{1}{2})\hslash \sqrt{\frac{\pi }{2mk}}\frac{\mathrm{\Gamma }(\frac{1}{m}+\frac{3}{2})}{\mathrm{\Gamma }(\frac{1}{m}+1)}\right]}^{\frac{2m}{m+2}}$

{\mathbf References}

[1] Griffiths, D. "Introduction to Quantum Mechanics" Prentice Hall, New Jersey, 1995.