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The Symmetric Linear Potential [ ]

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<strong>The</strong> <strong>Symmetric</strong> <strong>Linear</strong> <strong>Potential</strong><br />

<strong>The</strong> goal is to find analytical solutions to the TISE eigensystem for a potential of<br />

the form<br />

V ( x)<br />

<br />

<br />

b x x ,<br />

<br />

(1)<br />

where b is a constant specific to the potential in question. <strong>The</strong> first thing to notice is that<br />

the potential is symmetric, which in this case means we can classify solutions in terms of<br />

parity. For x 0 , the TISE is<br />

2 2<br />

d ψ( x)<br />

bx ( x) E ( x)<br />

2<br />

2m<br />

dx<br />

ψ ψ (2)<br />

We change variables with the definitions 1<br />

x as<br />

2<br />

<br />

a <br />

mb <br />

1/3<br />

W<br />

2<br />

<br />

<br />

ma<br />

2<br />

E<br />

( s ) (3)<br />

W<br />

and obtain a differential equation whose solutions are, in general, a linear combination of<br />

3<br />

3<br />

the Airy functions Ai ( 2 ) and Bi ( 2 ) .<br />

ψ''( ) 2 ψ ( )<br />

<br />

ψ ( ) C Ai( 2 ) C Bi( 2 )<br />

(4)<br />

3 3<br />

1 2<br />

However, Bi(ξ) diverges as . This violates the requirement that ψ 0 as<br />

, which does not make physical sense. We therefore restrict the solutions to the<br />

form<br />

ψ (5)<br />

3<br />

n<br />

( ) Cn Ai( 2 n)<br />

where C n are normalization factors. Again, this is for s 0 .<br />

At this point we consider the parity of our solutions. Even and odd eigenstates for<br />

s 0 can be extended to give the solutions for s 0 by<br />

even<br />

even<br />

odd<br />

odd<br />

ψ ( s) ψ ( s)<br />

ψ ( s) ψ ( s)<br />

(6)<br />

1 Another option is to take a <br />

2mb<br />

2 1/3<br />

and<br />

2 2<br />

W 2ma<br />

the Airy equation, but includes a factor of 2 -1/3 in the energy (9).<br />

. This leads to a more common form of


With these properties, it then stands to reason that we need the boundary conditions<br />

ψ<br />

odd<br />

3<br />

k<br />

(0) Ai( 2 <br />

k<br />

) 0<br />

dψ<br />

ds<br />

even<br />

k<br />

3<br />

(0) Ai '( 2 <br />

k<br />

) 0<br />

(7)<br />

for our (non-normalized) solutions. Normalization is done numerically as<br />

1/2<br />

<br />

1/3 2<br />

C 2 Ai( ) d<br />

<br />

n 3<br />

<br />

(8)<br />

2<br />

n n<br />

n <br />

<strong>The</strong> two equations in (7) then give the eigenvalues for odd and even parity states,<br />

respectively. Finally, we come to the conclusion that the bound state energies are given<br />

by<br />

E<br />

2 2<br />

1/3<br />

b<br />

n<br />

<br />

nW<br />

<br />

n<br />

<br />

m <br />

(9)<br />

Fig 1: An example of the symmetric linear potential theoretical eigenfunctions (n = 20). Note that since<br />

ψ is an odd state, ψ 20 (0) 0 . Observe also the decaying behavior of the wavefunction around the<br />

20<br />

classical turning points s <br />

20<br />

.

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