(a) Classically (i.e, from Maxwell’s equations), change in charge density, ρ, is related to divergence of current density, J. Use this fact and the time-dependent Schrödinger wave equation for particles of mass m and charge e to derive the current density
J=-\frac{ie\hbar }{2m} \left(\psi ^{*} \nabla \psi -\psi \nabla \psi ^{*} \right)
(b) If a wave function can be expressed as \psi \left(x,t\right) =Ae^{i(kx-\omega t)} +Be^{i(-kx-\omega t)}, show that particle flux is proportional to A²−B².
(c) For current to flow through a tunnel barrier, the wave function must contain both left- and right-propagating exponentially decaying solutions with a phase difference. If \psi \left(x,t\right) =Ae^{kx-i\omega t} +Be^{-kx-i\omega t}, show that particle flux is proportional to Im(AB^{*}). Hence, show that if \psi \left(x,t\right) = Be^{-kx-i\omega t} particle flux is zero.
(d) Show that a particle of energy E and mass m moving from left to right in a onedimensional potential in such a way that V(x)=0 for x\lt 0 and V(x)=V_{0} for x\geq 0 has unity reflection probability if E\lt V_{0}.
(a) We will use the classical expression relating the divergence of charge density to current density to obtain an expression for the quantum mechanical current. The change in charge density ρ is related to the divergence of current density J through
\frac{\partial }{\partial t} \rho (r, t)=-\nabla \cdot J(r, t)In quantum mechanics, we assume that the charge density of a particle with charge e and wave function \psi can be written \rho =e\left|\psi \right| ^{2}, so that
\frac{\partial \rho }{\partial t} =e\frac{\partial }{\partial t} (\psi ^{*}\psi )=e\left(\psi ^{*}\frac{\partial \psi }{\partial t}+\psi \frac{\partial \psi ^{*} }{\partial t} \right)We now make use of the fact that the time-dependent Schrödinger equation for a particle of mass m moving in a real potential is
i\hbar \frac{\partial }{\partial t} \psi (r,t)=\left(-\frac{\hbar ^{2} }{2m}\nabla ^{2} +V(r) \right)\psi (r, t) =\hat{H}\psi (r,t)Multiplying both sides by \psi^{*} (r,t) gives
i\hbar \psi ^{*} (r, t)\frac{\partial }{\partial t} \psi (r, t)=-\frac{\hbar ^{2} }{2m} \psi ^{*} (r, t)\nabla ^{2} \psi (r, t)+\psi ^{*} (r, t)V(r)\psi (r, t)which, when multiplied by e/i\hbar, is the first term on the right-hand side in our expression for \partial \rho /\partial t. To find the second term, one takes the complex conjugate of the time-dependent Schrödinger equation and multiplies both sides by \psi (r, t). Because V(r) is taken to be real, we have \psi ^{*} (r, t)V(r)\psi (r, t)=\psi (r, t)V(r)\psi ^{*} (r, t), giving the rate of change of charge density
\frac{\partial \rho }{\partial t} =-\psi ^{*} \frac{e\hbar }{i2m} \nabla^2 \psi +\psi \frac{e\hbar }{i2m} \nabla^2 \psi ^{*} +\frac{e\psi ^{*}\psi }{i\hbar } (V(r)-V(r))\frac{\partial \rho }{\partial t}=\frac{ie\hbar }{2m} (\psi ^{*}\nabla^2 \psi -\psi \nabla^2 \psi ^{*} )
\frac{\partial \rho }{\partial t} =\frac{ie\hbar }{2m} \nabla \cdot (\psi ^{*}\nabla \psi -\psi \nabla \psi ^{*} )=-\nabla .J
Hence, an expression for the current density for a particle charge e described by state \psi is
J=-\frac{ie\hbar }{2m} (\psi ^{*}\nabla \psi -\psi \nabla \psi ^{*} )This expression has an obvious symmetry, some consequences of which we will now explore.
(b) In this exercise we will work with a particle of mass m and charge e that is described by a wave function \psi \left(x,t\right) =Ae^{i(kx-\omega t)} +Be^{i(-kx-\omega t)} , where k is real. The aim is to show that particle flux is proportional to A²−B².
Starting with the current density in one dimension and substituting in the expression for the wave function gives
J_{x} =-\frac{ie\hbar }{2m}\left(\psi ^{*} \frac{\partial }{\partial x}\psi -\psi \frac{\partial \psi ^{*} }{\partial x} \right)\psi ^{*} \frac{\partial \psi }{\partial x} =(A^{*}e^{-ikx}+B^{*} e^{ikx} )(ikAe^{ikx}-ikBe^{-ikx} )
\psi ^{*} \frac{\partial \psi }{\partial x} =ik\left|A\right| ^{2} -ikA^{*} Be^{-2ike} +ikB^{*}Ae^{2ikx} -ik\left|B\right|^{2}
and
\psi \frac{\partial \psi ^{*} }{\partial x} =(Ae^{ikx} +Be^{-ikx} ) (-ikA^{*}e^{-ikx} +ikB^{*} e^{ikx} )\psi \frac{\partial \psi ^{*} }{\partial x} = -ik\left|A\right|^{2} -ikBA^{*} e^{-2ikx} +ikAB^{*}e^{2ikx} +ik\left|B\right| ^{2}
so that, finally,
J_{x} =-\frac{ie\hbar }{2m}(ik2(\left|A\right|^{2} -\left|B\right|^{2} )) =\frac{e\hbar k}{m} (\left|A\right|^{2} -\left|B\right|^{2} )This is not an unexpected result, since the wave function \psi \left(x,t\right) is made up of two traveling waves. The first traveling wave Ae^{ikx} might consist of an electron probability density \rho =\left|A\right| ^{2} moving from left to right at velocity v=\hbar k/m carrying current density j_{+} =ev_{+} \rho =e\hbar k\left|A\right| ^{2} /m. The second traveling wave Be^{-ikx} consists of an electron probability \rho =\left|B\right| ^{2} moving from right-to-left at velocity v=-\hbar k/m carrying current density j_{-} =ev_{-} \rho =-e\hbar k\left|B\right| ^{2} /m. The net current density is just the sum of the currents J_{x}=j_{+} +j_{-} =e\hbar k(\left|A\right|^{2} -\left|B\right|^{2} )/m.
(c) A particle of mass m and charge e is described by the wave function \psi \left(x,t\right) =Ae^{kx-i\omega t} +Be^{-kx-i\omega t}, where \kappa is real. We wish to show that for current to flow through a tunnel barrier the wave function must contain both left- and right-propagating exponentially decaying solutions with a phase difference.
As in part (b) we start with the current density in one dimension and substitute in the expression for the wave function. This gives
J_{x} =-\frac{ie\hbar }{2m}\left(\psi ^{*} \frac{\partial }{\partial x}\psi -\psi \frac{\partial \psi ^{*} }{\partial x} \right)\psi ^{*} \frac{\partial \psi }{\partial x} = (A^{*}e^{\kappa x} +B^{*}e^{-\kappa x} )(A\kappa e^{\kappa x} -B\kappa e^{-\kappa x} )
\psi^{*} \frac{\partial \psi }{\partial x} =\kappa \left|A\right|^{2} e^{2\kappa x} +\kappa B^{*}A -\kappa A^{*}B -\kappa \left|B\right|^{2} e^{-2\kappa x}
and
\psi \frac{\partial \psi^{*} }{\partial x} =(Ae^{\kappa x}+Be^{-\kappa x} )(A^{*}\kappa e^{\kappa x} -B^{*} \kappa e^{-\kappa x})\psi \frac{\partial \psi^{*} }{\partial x} =\kappa \left|A\right|^{2} e^{2\kappa x} -\kappa AB^{*} +\kappa BA^{*} -\kappa \left|B\right|^{2}e^{-2\kappa x}
so that
J_{x} =-\frac{ie\hbar }{2m} 2\kappa (A^{*}B-B^{*} A )=-\frac{2e\hbar \kappa }{m} (Im(AB^{*} ))To show this last equality, one starts by explicitly writing the real and imaginary parts of the terms in the brackets
(A^{*} B-B^{*} A)=(A_{Re}-iA_{Im} )(B_{Re} +iB_{Im} )-(B_{Re} -iB_{Im})(A_{Re}+iA_{Im})Multiplying out the terms on the right-hand side gives
(A^{*} B-B^{*} A)=A_{Re}B_{Re} +iA_{Re} B_{Im} -iA_{Im} B_{Re} +A_{Im} B_{Im} -A_{Re} B_{Re} -iB_{Re} A_{Im} +iB_{Im} A_{Re} -A_{Im} B_{Im}This simplifies to
(A^{*} B-B^{*} A)=2iA_{Re} B_{Im} -2iA_{Im} B_{Re}=2i(A_{Re}B_{Im} -A_{Im} B_{Re} )Taking the imaginary part of the terms on the right-hand side allows one to add the real terms A_{Re}B_{Re} and A_{Im}B_{Im}, so that the expression may be factored
(A^{*}B-B^{*}A)=-2i(Im(A_{Re}B_{Re}-iA_{Re} B_{Im}+ iA_{Im}B_{Re} +A_{Im} B_{Im} ))(A^{*}B-B^{*}A)=-2i(Im((A_{Re}+iA_{Im} )(B_{Re}-iB_{Im} )))=-2i(Im(AB^{*} ))
J_{x} =-\frac{ie\hbar }{2m} 2\kappa (A^{*} B-B^{*}A )=-\frac{2e\hbar \kappa }{m} (Im(AB^{*} ))
The significance of this result is that current can only flow through a one dimensional tunnel barrier in the presence of both exponentially decaying terms in the wave function \psi \left(x,t\right) =Ae^{\kappa x} +Be^{-\kappa x}. In addition, the complex coefficients A and B must differ in phase. The right-propagating term Ae^{\kappa x} can only carry current if the left-propagating term Be^{-\kappa x} exists. This second term indicates that the tunnel barrier is not opaque and that transmission of current via tunneling is possible.
Suppose a particle of mass m and charge e is described by wave function \psi \left(x,t\right) = Be^{-\kappa x-i\omega t}. Substitution into the expression for the one-dimensional current density gives
J_{x} =-\frac{ie\hbar }{2m}\left(\psi ^{*}\frac{\partial }{\partial x} \psi -\psi \frac{\partial \psi ^{*} }{\partial x} \right) =-\frac{ie\hbar }{2m} (B^{*}e^{-\kappa x}(-B\kappa e^{-\kappa x} )-Be^{-\kappa x}(-B^{*}\kappa e^{-\kappa x} ) )J_{x} =-\frac{ie\hbar }{2m}(-B^{*}B\kappa e^{-2\kappa x} +BB^{*}\kappa e^{-2\kappa x} )=0
(d) To show that a particle of energy E and mass m moving in a one-dimensional potential in such a way that V(x) = 0 for x < 0 in region 1 and V(x) = V_{0} for x ≥ 0 in region 2 has unity reflection probability if E < V_{0}, we write down solutions of the time-independent Schrödinger equation \left(\frac{-\hbar ^{2} }{2m} \frac{d^{2} }{dx^{2} }+V(x) \right) \psi (x)=E\psi (x). The solutions that describe left- and right-traveling waves in the two regions are
\psi _{1} (x)=Ae^{ik_{1}x } +Be^{-ik_{1}x } for x < 0
and
\psi _{2} (x) =Ce^{ik_{2}x}+De^{-ik_{2}x} for x ≥ 0
When E < V_{0} , the value of k_{2} is imaginary, and so k_{2} → ik_{2} . The value of D is zero to avoid a wave function with infinite value as x\rightarrow \infty. The value of C is finite, but the contribution to the wave function \psi _{2} (x\rightarrow \infty )=Ce^{-k_{2}x}\mid _{x\rightarrow \infty } =0. Hence, we may conclude that the transmission probability in the limit x\rightarrow \infty must be zero, since \left|\psi _{2} (x\rightarrow \infty )\right| ^{2} = 0.
From this it follows that \left|A\right| ^{2} = \left|B\right| ^{2} = 1, which has the physical meaning that the particle is completely reflected at the potential step when E < V_{0}.
Alternatively, one could calculate the reflection probability from the square of the amplitude coefficient for a particle of energy E and mass m incident on a one-dimension potential step
B=\left(\frac{1 – k_{2}/k_{1} }{1 + k_{2}/k_{1} } \right)When particle energy E < V_{0}, the value of k_{2} is imaginary, so that k_{2} → ik_{2}, which gives
\left|B\right| ^{2} =B^{*}B=\left(\frac{1 + ik_{2}/k_{1} }{1 – ik_{2}/k_{1} }\right)\left(\frac{1 – ik_{2}/k_{1} }{1 + ik_{2}/k_{1} }\right) =1From this one may conclude that the particle has a unity reflection probability.