Using the separation of variables technique, derive the time-independent Schrodinger equation (T.I.S.E.) in three dimensions.
3-D Time-Independent Schrodinger Equation
(−ℏ2/2m)∇2ψ(r)+V(r)ψ(r)=Eψ(r)
Since we are dealing with a 3-dimensional figure, we need to add the 3 different axes into the Schrondinger equation:
−ℏ2/2m(d2ψ(r)/dx2+d2ψ(r)/dy2+d2ψ(r)/dz2)=Eψ(r)
The easiest way in solving this partial differential equation is by having the wavefunction equal to a product of individual function for each independent variable (e.g., the Separation of Variables technique):
ψ(x,y,z)=X(x)Y(y)Z(z)
Now each function has its own variable:
X(x) is a function for variable x only
Y(y) function of variable y only
Z(z) function of variable z only
Now substitute Equation 4 into Equation 3 and divide it by the product: xyz:
d2ψ/dx2=(YZ)d2X/dx2⇒(1/X)d2X/dx2
d2ψ/dy2=(XZ)d2Y/dy2⇒(1/Y)d2Y/dy2
d2ψ/dz2=(XY)d2Z/dz2⇒(1/Z)d2Z/dz2
E is an energy constant, and is the sum of x, y, and z. For this to work, each term must equal its own constant. For example,
(d2X/dx2(+(2m/ℏ2)εxX=0
Now separate each term in Equation to equal zero:
(d2X/dx2)+(2m/ℏ2)εxX=0
(d2Y/dy2)+(2m/ℏ2)εyY=0
(d2Z/dz2)+(2m/ℏ2)εzZ=0
Now we can add all the energies together to get the total energy:
Ex+Ey+Ez =E
Now the equations are very similar to a 1-D box and the boundary conditions are identical, i.e.,
n=1,2,..∞
Use the normalization wavefunction equation for each variable:
ψ(x)={(√2/Lx)sinnπxLx } if 0≤x≤L0if L<x<0
Normalization wavefunction equation for each variable
X(x)=(√2/Lx)sin(nxπx/Lx)
Y(y)=(√2/Ly)sin(nyπy/Ly)
Z(z)=(√2/Lz)sin(nzπz/Lz)
The limits of the three quantum numbers
nx=1,2,3,...∞
ny=1,2,3,...∞
nz=1,2,3,...∞
For each constant use the de Broglie Energy equation:
εx=nx2h2/8mLx2
with nx=1,2,3...∞
Do the same for variables ny and nz. Combine wave functions for all axis , So overall wavefunctions inside a 3D box is
ψ(r)=(√8/L)sin(nxπx/Lx)sin(nyπy/Ly)sin(nzπz/Lz)
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