2) Consider a 2D infinite potential well with the potential U(x, y) = 0 for 0 ≤ x ≤ a & 0 ≤ y ≤ B, and U(x, y) = ∞, otherwise. Solve the time-independent Schrodinger equation, and find the normalized wavefunction and the corresponding energies.
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Expert's answer
2021-05-17T13:32:12-0400
Let us now consider the Schrödinger Equation for an electron confined to a two dimensional box, 0≤x≤a and 0≤y≤b . That is to say, within this rectangle the electron wavefunction behaves as a free particle U(x,y)=0 , but the walls are impenetrable so the wavefunction ψ(x,y,t)=0 at the walls
Extending the (time-independent) Schrödinger equation for a one-dimensional system
Equation 2 can be simplified for the particle in a 2D box since we know that U(x,y)=0
is within the box and U(x,y)=∞ is outside the box.
−2mℏ2(∂x2∂2ψ(x,y)+∂2ψ(x,y)∂y2)=Eψ(x,y)(3)
Since the Hamiltonian (i.e. left side of Equation 3) is the sum of two terms with independent (separate) variables, we try a product wavefunction like in the Separation of Variables approach used to separate time-dependence from the spatial dependence previously. Within this approach we express the 2-D wavefunction as a product of two independent 1-D components
ψ(x,y)=X(x)Y(y)(4)
This ansatz separates Equation 3 into two independent one-dimensional Schrödinger equations
−2mℏ2(∂x2∂2X(x))=εxX(x)(5)
−2mℏ2(∂y2∂2Y(y))=εyY(y)(6)
where the total energy of the particle is the sum of the energies from each one-dimensional Schrödinger equation
E=εx+εy(7)
The differential equations in Equations 5 and 6 are familiar as they were found for the particle in a 1-D box. They have the general solution
X(x)=Axsin(kxx)+Bxcos(kxx)(8)
Y(y)=Aysin(kyy)+Bycos(kyy)(9)
Applying Boundary Conditions
The general solutions in Equations 8 and 9 can be simplified to address boundary conditions dictated by the potential, i.e ψ(0,y)=0 and ψ(x,0)=0. Therefore, Bx=0 and By=0.
Thus, we can combine Equations 8, 9, and 4 to construct the wavefunction ψ(x,y) for a particle in a 2D box of the form
ψ(x,y)=Nsin(ℏ22mεxx)sin(ℏ22mεyy)(10)
We still need to satisfy the remaining boundary conditions ψ(L,y)=0ψ(L,y)=0andψ(x,L)=0
ψ(x,y)=Nsin(ℏ22mεxL)sin(ℏ22mεyy)(11)
and
ψ(x,y)=Nsin(ℏ22mεxx)sin(ℏ22mεyL)(12)
Equation 11 can be satisfied if
sin(ℏ22mεxL)=0(13)
independent of the value of y, while equation 12 can be satisfied if
sin(ℏ22mεyL)=0(14)
independent of the value of x. These are the same conditions that we encountered for the one-dimensional box, hence we already know the sin function in each case can be zero in many places. In fact, these two conditions are satisfied if
ℏ22mεxL=nxπ(15)
and
ℏ22mεyL=nyπ(16)
which yield the allowed values of εx and εy as
εnx=2mL2ℏ2π2nx2(17)
and
εny=2mL2ℏ2π2ny2(18)
We need two different integers nx and ny because the conditions are completely independent and can be satisfied by any two different (or similar) values of these integers. The allowed values of the total energy are now given by
Enx,ny=2mL2ℏ2π2(n2x+n2y)(19)
Once the conditions on εnx and εny are substituted into Equation 10, the wavefunctions become
ψnx,ny(x,y)=Nsin(Lnxπx)sin(Lnyπy)(20)
The constant N is now determined by the normalization condition
∫0L∫0L∣ψnx,ny(x,y)∣2dxdy=1
N2∫0Lsin2(Lnxπx)dx∫0Lsin2(Lnyπy)dy=1
N22L⋅2L=1
N=L2
so that the complete normalized 2D wavefunction is
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