Quantum Particles in a box, Lecture notes of Quantum Mechanics

This describes the formulation of quantum particle in a box.

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Tabish Qureshi
Quantum Mechanics: Particle in a box
Energy of a particle in a box
Consider a particle of mass
𝑚
, which is trapped inside a one-dimensional box of length
𝐿
. Inside the box, the particle is free, but the two walls of the box are rigid, and the box
can neither penetrate them, nor go out of the box. Thus the potential experienced by the
particle is zero inside the box and infinite at the two walls and beyond. The Hamiltonian is
given by
ˆ
𝐻=ˆ
𝑝2
2𝑚+𝑉(ˆ
𝑥),(1)
which can be written in the position representation as
ˆ
𝐻=2
2𝑚
𝑑2
𝑑𝑥2+𝑉(𝑥), 𝑉 (𝑥)=0 0 <𝑥<𝐿
𝑥𝐿, 𝑥 0(2)
Notice that since there is only one variable
𝑥
, we use total derivatives instead of partial
derivatives. The time-independent Schrödinger equation can be written as
2
2𝑚
𝑑2𝜓(𝑥)
𝑑𝑥2+𝑉(𝑥)𝜓(𝑥)=𝐸𝜓(𝑥).(3)
This is a 2nd order differential equation, and can be easily solved inside the box, because
the potential energy term is zero there. Inside the box the Schr¨
dinger equation is
𝑑2𝜓(𝑥)
𝑑𝑥2+2𝑚 𝐸
2𝜓(𝑥)=0,
which may be written as
𝑑
𝑑𝑥 +𝑖2𝑚𝐸
𝑑
𝑑𝑥 𝑖2𝑚𝐸
𝜓(𝑥)=0.
The solution of the equation
𝑑
𝑑𝑥 𝑖2𝑚𝐸
𝜓(𝑥)=
0will also be a solution of the above
equation. We could have also written the above equation as
𝑑
𝑑𝑥 𝑖2𝑚𝐸
𝑑
𝑑𝑥 +𝑖2𝑚𝐸
𝜓(𝑥)=0.
In that case, the solution of the equation
𝑑
𝑑𝑥 +𝑖2𝑚𝐸
𝜓(𝑥)=
0will also be a solution of
the above equation. A second order equation can have only two independent solutions.
These two solutions can easily be gotten as
𝜓1(𝑥)=𝑒𝑖𝑘 𝑥 ,𝜓2(𝑥)=𝑒𝑖 𝑘𝑥 ,
where
𝑘=2𝑚𝐸/
. The general solition will be a linear combination of these two solutions,
namely
𝜓(𝑥)=𝑐1𝑒𝑖𝑘 𝑥 +𝑐2𝑒𝑖𝑘 𝑥 ,
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Quantum Mechanics: Particle in a box

Energy of a particle in a box

Consider a particle of mass 푚, which is trapped inside a one-dimensional box of length

퐿. Inside the box, the particle is free, but the two walls of the box are rigid, and the box

can neither penetrate them, nor go out of the box. Thus the potential experienced by the

particle is zero inside the box and infinite at the two walls and beyond. The Hamiltonian is

given by

2

which can be written in the position representation as

−\

2

2

2

(2)

Notice that since there is only one variable 푥, we use total derivatives instead of partial

derivatives. The time-independent Schrödinger equation can be written as

−\

2

2 휓(푥)

2

This is a 2nd order differential equation, and can be easily solved inside the box, because

the potential energy term is zero there. Inside the box the Schr ¨dinger equation is

2

휓(푥)

2

\

2

which may be written as

\

\

The solution of the equation

푑푥

2 푚퐸

\

휓(푥) = 0 will also be a solution of the above

equation. We could have also written the above equation as

\

\

In that case, the solution of the equation

푑푥

2 푚퐸

\

휓(푥) = 0 will also be a solution of

the above equation. A second order equation can have only two independent solutions.

These two solutions can easily be gotten as

푖푘푥

, 휓 2 (푥) = 푒

−푖푘푥

,

where 푘 =

2 푚퐸/. The general solition will be a linear combination of these two solutions,

namely

푖푘푥

  • 푐 2 푒

−푖푘푥

,

where 푐 1

2

are undetermined constants. We have gotten the eigenfunction, but we still

don’t have the energy of the particle. So, what is missing? We have solved the Schrödinger

equation inside the box, but have left out the boundary, and the region of space outside the

box. Instead of putting in infinite potential, which can potentially create problems, we can

simply use the physical condition that the particle cannot penetrate the boundary, and thus

the probability of finding it inside the walls should be zero. From Born’s interpretation of

the wave-function we have learnt that the |휓(푥)|

2

푑푥 is the probability of finding the particle

between 푥 and 푥 + 푑푥. The probability density of finding the particle at a position 푥 is

2

. Since particle cannot penetrate the walls, we have, |휓( 0 )|

2 = 0 and |휓(퐿)|

2 = 0.

This in turn means 휓( 0 ) = 0 and 휓(퐿) = 0. From the first condition we get 푐 2

1

, which

implies

1

sin(푘푥).

The second condition yields

1

sin(푘퐿) = 0 ,

which means 푘퐿 = 푛휋, 푛 = 1 , 2 , 3.... We cannot have 푛 = 0 because that will

make 푘 zero, and the wave-function zero everywhere. The wave-function cannot be zero

everywhere, because that would imply that the probability of finding the particle anywhere

is zero, i.e., the particle does not exist. Thus

and there are many eigenfunctions corresponding to those, which we label by 푛

1

sin(푛휋푥/퐿).

Recalling the relation of 푘 to energy, we get

\

or

2

2

2

We arrive at a very interesting result which says that the particle which is trapped inside a

box, cannot just take any value of energy. There are only fixed, quantized values it can

take. The energy of the particle is quantized. This is something that never happens in

classical mechanics. We shall see later that this quantization of energy is not a special

case here, but happens whenver a particle is confined to a small region.

Normalization of the eigenfunctions

Since |휓(푥)|

2 푑푥 is the probability of finding the particle in a small region around 푥, if we

sum it over all 푥, it should give us the probability of finding the particle in all of space. Since

the particle does exist, the probability of finding it anywhere in all of space should be 1:

−∞

(푥)휓(푥)푑푥 = 1. (4)

This is called the normalization condition, and must be satisfied by all wave-functions

representing a physical system. Using the normalization of all eigenfunctions 휓 푛

(푥), we

can find the unknown constant 푐 1 , and get the final normalized eigenfunctions as

2

sin(푛휋푥/퐿), 푛 = 1 , 2 , 3... (5)