The Delta-Function Potential - Physics &...

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The Delta-Function Potential As our last example of one-dimensional bound-state solutions, let us re-examine the finite potential well: and take the limit as the width, a, goes to zero, while the depth, V 0 , goes to infinity keeping their product aV 0 to be constant, say U 0 . In that limit, then, the potential becomes: ( ) ( ) x U x V δ 0 = and we can have a sense that if there is at least one bound state of this potential, it should look (as drawn above) like the ground state of the finite square well. Let’s examine the TISE for this potential: x V(x) x = -a/2 x = a/2 V = -V 0 x V(x) x = -a/2 x = a/2 V = -V 0 x V(x) x V(x)

Transcript of The Delta-Function Potential - Physics &...

Page 1: The Delta-Function Potential - Physics & Astronomyphysics.unm.edu/Courses/Fields/Phys491/Notes/TISEDelta.pdfTo be complete, we can find the constant A via the normalization condition:

The Delta-Function Potential As our last example of one-dimensional bound-state solutions, let us re-examine the finite potential well: and take the limit as the width, a, goes to zero, while the depth, V0, goes to infinity keeping their product aV0 to be constant, say U0. In that limit, then, the potential becomes: ( ) ( )xUxV δ

0−=

and we can have a sense that if there is at least one bound state of this potential, it should look (as drawn above) like the ground state of the finite square well. Let’s examine the TISE for this potential:

x

V(x)

x = -a/2 x = a/2

V = -V0

x

V(x)

x = -a/2 x = a/2

V = -V0

x

V(x)

x

V(x)

Page 2: The Delta-Function Potential - Physics & Astronomyphysics.unm.edu/Courses/Fields/Phys491/Notes/TISEDelta.pdfTo be complete, we can find the constant A via the normalization condition:

( )

( )

otherwise2

0at x2

2

2

22

02

22

02

22

ψψ

ψψδψ

ψψδ

ψψ

Exm

ExUxm

ExUxm

EH

=∂∂−

==−∂∂−

⇒=⎥⎦

⎤⎢⎣

⎡−

∂∂−

⇒=

h

h

h

)

Let’s first take a look at the region outside of x = 0. Here, we can rewrite the TISE as:

h

h

h

mE

mEx

Exm

2

22

222

2

2

22

−=

=−

=∂∂

⇒=∂∂−

κ

ψκψψ

ψψ

Here, kappa is real since the energy is negative. This simple differential equation has solutions we know: ( ) xx BeAex κκψ += −

For negative x (left side of the potential), ψ will blow up as x goes to negative infinity, so A must be zero. On the right side the same thing happens and there, the constant B must be zero. So, we have:

( )⎪⎩

⎪⎨⎧

><

= − 00

xAexBe

x x

x

κ

κ

ψ

At x = 0, the wavefunction must be continuous, so A = B and we have:

( )⎪⎩

⎪⎨⎧

≥≤

= − 00

xAexAe

x x

x

κ

κ

ψ

Now, we must use the information at x = 0. In the region near x = 0, the TISE gives us:

( ) ψψδψ ExUxm

=−∂∂−

02

22

2h

we integrate both sides with respect to x over an infinitesimally small region around the delta potential, say from –ε to +ε:

Page 3: The Delta-Function Potential - Physics & Astronomyphysics.unm.edu/Courses/Fields/Phys491/Notes/TISEDelta.pdfTo be complete, we can find the constant A via the normalization condition:

( )

( ) ( ) ( )

( ) ( ) ( ) ( )∫

∫∫∫

−−

−−−

=−⎟⎟⎠

⎞⎜⎜⎝

⎛∂

∂−

∂∂−

⇒=−∂

∂−

ε

εεε

ε

ε

ε

ε

ε

ε

ψψψψ

ψψδψ

dxxEUxx

xx

m

dxxEdxxxUdxx

xm

02

2

0

2

02

22

h

h

Now, let’s let ε go to zero. Then the right hand side of the equation will go to zero since ψ is finite and we integrate it over a zero width. This gives us:

( ) ( ) ( )02

20 ψψψ

εε h

mUxx

xx −

=⎟⎟⎠

⎞⎜⎜⎝

⎛∂

∂−

∂∂

Now, from above (and letting epsilon go to zero):

( )

( )

( )

( ) κψ

κψ

κψ

κψ

κ

κ

Axx

eAxx

Axx

eAxx

x

x

=∂

⇒=∂

∂<

−=∂

⇒−=∂

∂>

0

0

0, for x

0, for x

So that

( ) ( ) ( )02

2 20 ψκκκψψ

εε h

mUAAA

xx

xx −

=−=−−=⎟⎟⎠

⎞⎜⎜⎝

⎛∂

∂−

∂∂

Now, ψ(0) = A, so:

20

20

22

h

hmU

AmU

A

=

⇒−

=−

κ

κ

So that there is one, and only one allowed energy level:

2

20

20

2

2

h

hh

mUE

mEmU

−=

⇒−

==κ

Page 4: The Delta-Function Potential - Physics & Astronomyphysics.unm.edu/Courses/Fields/Phys491/Notes/TISEDelta.pdfTo be complete, we can find the constant A via the normalization condition:

To be complete, we can find the constant A via the normalization condition:

( )

h

0

2

0

222 12

mUA

AdxeAdxx x

==

⇒=== ∫∫∞

−∞

∞−

κ

κψ κ

Then there is one and only one bound state, and one energy eigenvalue:

( ) 2

200

22

0

hhh

mUEe

mUx x

mU

−==− ,ψ