to understand the nature of solutions, compare energy to potential at classically, there are two...

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2 2 2 2 d x E x V x x m dx To understand the nature of solutions, compare energy to potential at •Classically, there are two types of solutions to these equations Bound States are when E < V(). Unbound states are when E > V() •Quantum mechanically, there are bound and unbound states as well, with the same criteria •Bound states are a little easier to understand, so we’ll do these first E > V() E < V() V(x ) Bound and Unbound States

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Page 1: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

22

22

d xE x V x x

m dx

To understand the nature of solutions, compare energy to potential at •Classically, there are two types of solutions to these equations

•Bound States are when E < V().•Unbound states are when E > V()

•Quantum mechanically, thereare bound and unbound states aswell, with the same criteria

•Bound states are a littleeasier to understand, sowe’ll do these first

E > V()

E < V()

V(x)

Bound and Unbound States

Page 2: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

Wave Function Constraints

2 2

22

dE V x

m dx

1. The wave function (x) must be continuous2. Its derivative must exist everywhere3. Its derivative must be continuous*4. Its second derivative must exist everywhere*5. The wave function must be properly normalized†

• Must not blow up at *Except where V(x) is infinite†There are exceptions and ways around this problem

Normalization

21 x dx

2x dx A

What if the wave function is not properly normalized?•If the integral is finite, multiply by a constant to fix it

•Modified wave satisfies Schrödinger•If the integral is infinite, it gets complicated

•For bound states, this is still trouble•For unbound states, it is okay

2

ˆDefine

ˆThen 1

x x A

x dx

Page 3: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The 1D infinite square well (1)

2 2

22

dE V x

m dx

0 if 0

otherwise

x LV x

•Outside of the well, the wave function must vanish•In remaining region, we need to solve differential equation

0 if 0 or x x x L

2 2

22

dE

m dx

•What functions are minus their second derivative?•We prefer real

cos

sinikx

x kx

x kx

x e

Boundary Conditions•Must vanish at x = 0•And at x = L

•Where does sin vanish?•Don’t worry about derivative because V(x) blows up there

0 sinL kL n

kL

V(x)

Page 4: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The 1D infinite square well (2) nk

L

sinx kx 2 2

22

dE

m dx

2 2

2sin sin

2

dE kx kx

m dx

2

cos2

k dkx

m dx

2 2

sin2

kkx

m

2 2

2

kE

m 2 2 2

22 n

nE

mL

1,2,3,n sinnx

xL

mL2E/2

Energy Diagram

n = 1n = 2n = 3n = 4

Page 5: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

1D Infinite Square Well (3)BUT WAIT: What about normalization?

sinnx

xL

2x dx

2

0sin

L nxdx

L

0

2sin

2 2

Lx L nx

n L

1

2

L

To fix it: multiply by (2/L).

2

sin if 0

0 otherwisen

nxx L

x L L

2 2 2

22n

nE

mL

•The most general solution is superposition of this solution

, expn n nn

x t c x iE t

1,2,3,n

Page 6: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Finite Square Well (1)

2 2

22

dE V x

m dx

12

0

0 if

otherwise

x LV x

V

•We need to solve equation in all three regions; this takes work•In region II, we get solutions like before

•No longer necessary that it vanish at the boundaries•In regions I and III, we solve a different equation:

cos

sin

x kx

x kx

2 2

2

kE

m

2 2

022

dE V

m dx

2 2

022

dV E

m dx

•If we are looking at bound state (E < V0), in these regions, we get exponentials xx e 2 2

0 2V E

m

I II III

Page 7: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Finite Square Well (2)

cos sin

x xI

II

x xIII

x Ae Be

x C kx D kx

x Ee Fe

•Wave function must not blow up at •Wave function must be continuous at x = ½L

I II III

0B E

22

2mEk

1 12 2

1 12 2

I II

II III

L L

L L

022

2m V E

2

2

cos 2 sin 2

cos 2 sin 2

L

L

Ae C kL D kL

Fe C kL D kL

1 12 2

1 12 2

I II

II III

L L

L L

2

2

sin 2 cos 2

sin 2 cos 2

L

L

A e Ck kL Dk kL

F e Ck kL Dk kL

•Derivative of wave function must be continuous at x = ½L

Page 8: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Finite Square Well (2)

cos sin

x xI

II

x xIII

x Ae Be

x C kx D kx

x Ee Fe

•Wave function must not blow up at •Wave function must be continuous at x = ½L

I II III

0B E

22

2mEk

1 12 2

1 12 2

I II

II III

L L

L L

022

2m V E

2

2

cos 2 sin 2

cos 2 sin 2

L

L

Ae C kL D kL

Fe C kL D kL

1 12 2

1 12 2

I II

II III

L L

L L

2

2

sin 2 cos 2

sin 2 cos 2

L

L

A e Ck kL Dk kL

F e Ck kL Dk kL

•Derivative of wave function must be continuous at x = ½L

Page 9: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Finite Square Well (3)

•Wave function penetrates into “forbidden” region•Oscillates when E > V(x)•Damps when E < V(x)

•Energies decreased slightly compared to infinite square well•Finite number of bound states

•Due to finite extension and depth of potential well

Energy Diagram

Infinite Well

2

0 2

75V

mL

n = 4n = 3n = 2n = 1

•Solve all these equations simultaneously•Normalize the final wave function

Page 10: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Harmonic Oscillator (1)

2 2

22

dE V x

m dx

212V x kx

•At large x, the behavior is governed (mostly) by the x2 term•Now we guess

2 212 m x

2 2 22

2 2 2

2d mE mx

dx

22

2

d m x

dx

d m x

dx

d mxdx

2

ln2

m x

2

exp2

m x

•Don’t want it blowing up at infinity!

2

exp2

m x

Our strategy:•Check that this works•Find more solutions and check them

Page 11: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

The Harmonic Oscillator (2)2

exp2

m x

2

exp2

d d m x

dx dx

2

exp2

m x m x

2 2

2exp

2

d m d m xx

dx dx

2

exp2

m m x

2 2

exp2

m x m x

2 2 2

2

m m x

12E

2 221

222

dE m

m dx

2 2 2 22 21

222

m m xE m x

m

12

Page 12: To understand the nature of solutions, compare energy to potential at  Classically, there are two types of solutions to these equations Bound States are

n = 3n = 2n = 1n = 0

The Harmonic Oscillator (3)2

exp2

m x

•We still need to normalize it22 m xdx e dx

m

2

40 exp

2

m m xx

•Expect other solutions to have similar behavior, at least at large x

•We will guess the nature of these solutions•Multiply the wave function above by an arbitrary polynomial P(x)

2

11 0

exp2n n

n nn n n

m xx P x

P x a x a x a

•Substitute in and see if it works•This will give you En

12nE n