Quantum Mechanics Problem Set: Boson Operators and Coherent States, Assignments of Health sciences

Problem set solutions for quantum mechanics, focusing on boson operators and coherent states. It covers the conversion of operators between first-quantized and second-quantized formalisms, commutation relations, and properties of coherent states. Students will learn how to calculate matrix elements and understand the relationship between different formalisms.

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Pre 2010

Uploaded on 08/26/2009

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PHY–396 K. Problem set #3. Due October 2, 2008.
1. An operator acting on identical bosons can be described in terms of N–particle wave
functions (the first-quantized formalism) or in terms of creation and annihilation operators
in the Fock space (the second-quantized formalism). This exercise is about converting the
operators from one formalism to another.
The key to this conversion are the single-particle wave functions φα(x) of states |αiand
the symmetrized N-particle states wave functions
φαβ···ω(x1,x2. . . , xN) = 1
D
distinct permutations
of (α,β,...,ω)
X
α, ˜
β,..., ˜ω)
φ˜α(x1)×φ˜
β(x2)× · ·· × φ˜ω(xN)
=1
TD
all permutations
of (α,β,...,ω)
X
α, ˜
β,..., ˜ω)
φ˜α(x1)×φ˜
β(x2)× · ·· × φ˜ω(xN)
(1)
of N-boson states |α, β , . . . , ωi. In eqs. (1), Dis the number of distinct (i.e., non-trivial)
permutations of single-particle states (α, β, . . . , ω ) and Tis the number of trivial permu-
tations. In terms of the occupation numbers nγ
T=Y
γ
nγ!, D =N!
T.(2)
(a) Consider a generic N-particle quantum state |N;ψ)iwith a totally symmetric wave-
function Ψ(x1,...,xN). Show that the (N+1)–particle state |N+ 1, ψ0i= ˆa
α|N;ψi
has wave function
ψ0(x1,...,xN) = 1
N+ 1
N+1
X
i=1
φα(xi)×ψ(x1,...,6xi,...,xN+1).(3)
Hint: First prove this for wave-functions of the form (1). Then use the fact that
states |α1, . . . , αNiform a complete basis of the N-boson Hilbert space.
1
pf3
pf4

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PHY–396 K. Problem set #3. Due October 2, 2008.

  1. An operator acting on identical bosons can be described in terms of N –particle wave

functions (the first-quantized formalism) or in terms of creation and annihilation operators

in the Fock space (the second-quantized formalism). This exercise is about converting the

operators from one formalism to another.

The key to this conversion are the single-particle wave functions φ α

(x) of states |α〉 and

the symmetrized N -particle states wave functions

φ αβ···ω

(x 1

, x 2

... , x N

D

distinct permutations

of (α,β,...,ω)

(˜α,

˜ β,...,ω˜)

φ α˜

(x 1

) × φ ˜ β

(x 2

) × · · · × φ ω˜

(x N

T

D

all permutations

of (α,β,...,ω) ∑

(˜α,

˜ β,...,ω˜)

φ α˜

(x 1 ) × φ ˜ β

(x 2 ) × · · · × φ ω˜

(x N

of N -boson states |α, β,... , ω〉. In eqs. (1), D is the number of distinct (i.e., non-trivial)

permutations of single-particle states (α, β,... , ω) and T is the number of trivial permu-

tations. In terms of the occupation numbers n γ

T =

γ

n γ

! , D =

N!

T

(a) Consider a generic N -particle quantum state |N ; ψ)〉 with a totally symmetric wave-

function Ψ(x 1

,... , x N

). Show that the (N +1)–particle state |N + 1, ψ

′ 〉 = ˆa

α

|N ; ψ〉

has wave function

ψ

(x 1

,... , x N

N + 1

N + ∑

i=

φ α

(x i

) × ψ(x 1

,... , 6 x i

,... , x N +

Hint: First prove this for wave-functions of the form (1). Then use the fact that

states |α 1

,... , α N

〉 form a complete basis of the N -boson Hilbert space.

(b) Show that the (N − 1)–particle state |N − 1 , ψ

′′ 〉 = ˆa α

|N ; ψ〉 has wave-function

ψ

′′ (x 1

,... , x N − 1

N

d

3 x N

φ

α

(x N

) × ψ(x 1

,... , x N − 1

, x N

Hint: for any |N − 1 ,

ψ〉, 〈N − 1 ,

ψ| ˆa α

|N, ψ〉 = 〈N, ψ| ˆa

α

|N − 1 ,

ψ〉

.

Now consider one-body operators, i.e. additive operators acting on one particle at a time.

In the first-quantized formalism they act on N –particle states according to

A

(1)

net

N ∑

i=

A

1

(i

th

particle) (5)

where

A

1

is some kind of a one-particle operator (such as momentum ˆp, or kinetic energy

1

2 m

2 , or potential V (ˆx), etc., etc.). In the second-quantized formalism such operators

become

A

(2)

net

α,β

〈α|

A 1 |β〉 ˆa

α

ˆa β

(c) Verify that the two operators have the same matrix elements between any two N -

boson states |N, ψ〉 and |N,

ψ〉, 〈N,

ψ|

A

(1)

net

|N, ψ〉 = 〈N,

ψ|

A

(2)

net

|N, ψ〉.

Hint: use

A

1

α,β

|α〉 〈α|

A

1

|β〉 〈β|.

Finally, consider two-body operators, i.e. additive operators acting on two particles at a

time. Given a two-particle operator

B

2

— such as V (ˆx 1

− xˆ 2

) — the net B operator acts

in the first-quantized formalism according to

B

(1)

net

1

2

i 6 =j

B

2

(i

th

and j

th

particles), (7)

and in the second-quantized formalism according to

B

(2)

net

1

2

α,β,γ,δ

(〈α| ⊗ 〈β|)

B 2 (|γ〉 ⊗ |δ〉) ˆa

α

β

ˆa γ

ˆa δ

(d) Again, show these two operators have the same matrix elements between any two

N -boson states, 〈N,

ψ|

A

(1)

net

|N, ψ〉 = 〈N,

ψ|

A

(2)

net

|N, ψ〉 for any 〈N,

ψ| and |N, ψ〉.

(e) Consider time-dependent coherent states |ξ(t)〉. Show that for ξ(t) = ξ 0

e

−iωt , the

state |ξ(t)〉 satisfies the time-dependent Schr¨odinger equation i¯h

d

dt

|ξ(t)〉 =

H |ξ(t)〉.

(f) The coherent states are not quite orthogonal to each other.

Calculate their overlap 〈η|ξ〉.

Now consider coherent states of multi-oscillator systems and hence quantum fields. In

particular, let us focus on the creation and annihilation fields

(x) and

Ψ(x) for non-

relativistic spinless bosons.

(g) Generalize (a) and construct coherent states |Φ〉 which satisfy

Ψ(x) |Φ〉 = Φ(x) |Φ〉 (11)

for any given classical complex field Φ(x).

(h) Show that for any such coherent state, ∆N =

N where

N

def

N |Φ〉 =

dx |Φ(x)|

2

. (12)

(i) Let

H =

dx

¯h

2

2 M

(x) · ∇

Ψ(x) + V (x) ×

(x)

Ψ(x)

and show that for any classical field configuration Φ(x, t) that satisfies the classical

field equation

i¯h

∂t

Φ(x, t) =

¯h

2

2 M

2

  • V (x)

Φ(x, t),

the time-dependent coherent state |Φ〉 satisfies the true Schr¨odinger equation

i¯h

∂t

H |Φ〉. (13)

(j) Finally, show that the quantum overlap | 〈Φ 1

2

2 between two different coherent

states is exponentially small for any macroscopic difference δΦ(x) = Φ 1

(x) − Φ 2

(x)

between the two field configurations.