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Homework 1-4 PDF

This document is the homework assignment for Physics 513: Quantum Field Theory. It contains: 1) Definitions and proofs regarding coherent states and their properties including commutation relations. 2) Calculations of the normalization constant N, expectation value of the field φ(x), expected particle number, and mean square dispersion for a coherent state. 3) The homework contains proofs and calculations involving coherent states, field operators, and their commutation relations to determine properties of coherent states.
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0% found this document useful (0 votes)
88 views5 pages

Homework 1-4 PDF

This document is the homework assignment for Physics 513: Quantum Field Theory. It contains: 1) Definitions and proofs regarding coherent states and their properties including commutation relations. 2) Calculations of the normalization constant N, expectation value of the field φ(x), expected particle number, and mean square dispersion for a coherent state. 3) The homework contains proofs and calculations involving coherent states, field operators, and their commutation relations to determine properties of coherent states.
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
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Download as PDF, TXT or read online on Scribd
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PHYSICS 513: QUANTUM FIELD THEORY HOMEWORK 4 1

Physics 513, Quantum Field Theory


Homework 4
Due Tuesday, 30th September 2003
Jacob Lewis Bourjaily

1. We have defined the coherent state by the relation


(Z )
d3 k ηk a†k
|{ηk }i ≡ N exp √ |0i.
(2π)3 2Ek
For my own personal convenience throughout this solution, I will let
Z
d3 k ηk a†k
A≡ √ .
(2π)3 2Ek
£ ¤ η
a) Lemma: ap , eA = √ p eA .
2Ep
proof: First we note that from simple Taylor expansion (which is justified here),
A2 A3
eA = 1 + A + + + ...
2 3!
Clearly ap commutes with 1 so we may write,
£ ¤ 1 1
ap , eA = [ap , A] + [ap , A2 ] + [ap , A3 ] + . . . ,
2 3!
1 1 ¡ ¢
= [ap , A] + ([ap , A]A + A[ap , A]) + [ap , A]A2 + A[ap , A]A + A[ap , A]A + . . . ,
µ 2 2 3 4
3! ¶
∗ A A A
= [ap , A] 1 + A + + + + ... ,
2 3! 4!
= [ap , A]eA .
Note that the step labelled ‘*’ is unjustified. To allow the use of ‘*’ we must show that
[ap , A] is an invariant scalar and therefore commutes with all the A’s. This is shown by
direct calculation.
Z
d3 k ηk
[ap , A] = √ [ap , a†k ],
(2π)3 2Ek
Z
d3 k ηk
= √ p − ~k),
(2π)3 δ (3) (~
(2π)3 2Ek
ηp
=p .
2Ep
η
This proves what was required for ‘*.’ √ p is clearly a scalar because η and Ep are real
2Ep
numbers only. But by demonstrating the value of [ap , A] we can complete the proof of the
required lemma. Clearly,
£ ¤ ηp
ap , eA = [ap , A]eA = p eA .
2Ep
‘ ’
£ ¤ óπ²ρ ²́δ²ι δ²Äιξαι
A A A
It is clear from the definition of the commutator that ap e = ap , e + e ap . Therefore it
is intuitively obvious, and also proven that
ap |{ηk }i = N ap eA |0i,
¡£ ¤ ¢
= N ap , eA + eA ap |0i,
ηp
=Np |0i + N eA ap |0i,
2Ep
ηp
∴ ap |{ηk }i = p ap |{ηk }i. (1.1)
2Ep
‘ ’
óπ²ρ ²́δ²ι δ²Äιξαι
2 JACOB LEWIS BOURJAILY

b) We are to compute the normalization constant N so that h{ηk }|{ηk }i = 1. I will proceed
by direct calculation.
1 = h{ηk }|{ηk }i,
R d3 k √
ηk ak

= N ∗ h0|e (2π)3 2Ek


|{ηk }i,
R d3 k ηk

= N ∗ h0|e (2π)3 2Ek
|{ηk }i
because we know that ak |{ηk }i = √ηk |{ηk }i. So clearly
2Ek
R d3 k
2
ηk

1 = |N |2 e (2π)3 2Ek ,
R d3 k
2
ηk
− 12
∴N =e (2π)3 2Ek .
c) We will find the expectation value of the field φ(x) by direct calculation as before.
Z
d3 p 1 ¡ i~p·~x ¢
φ(x) = h{ηk }|φ(x)|{ηk }i = h{ηk }| 3
p ap e + a†p e−i~p·~x |{ηk }i,
(2π) 2Ep
 
Z
d3 p 1  
 h{ηk }|ap ei~p·~x |{ηk }i + h{ηk }|a†p e−i~p·~x |{ηk }i,
= p 
(2π) 3
2Ep | {z } | {z }
act with ap to the right act with a†p to the left
Z Ã !
d3 p 1 ηp i~
p·~
x ηp −i~
p·~
x
= p p e +p e ,
(2π)3 2Ep 2Ep 2Ep
Z
d3 p ηp
= cos(~
p · ~x).
(2π)3 Ep
d) We will compute the expected particle number directly.
Z
d3 p †
N = h{ηk }|N |{ηk }i = h{ηk }| a ap |{ηk }i,
(2π)3 p
Z µ ¶
d3 p †
= h{η k }|a a
p p |{η k }i ,
(2π)3 ←−−−− −−−−→
Z
d3 p ηp2
= .
(2π)3 2Ep
e) To compute the mean square dispersion, let us recall the theorem of elementary probability
theory that
2
h(∆N )2 i = N 2 − N .
We have already calculated N so it is trivial to note that
Z 3 3
2 d kd p ηk2 ηp2
N = .
(2π)6 4Ek Ep
Let us then calculate N 2 .
Z 3 3
d kd p †
N 2 = h{ηk }|N 2 |{ηk }i = h{ηk }| a ak a†p ap |{ηk }i,
(2π)6 k
Z 3 3
d kd p ηk ηp
= p h{ηk }|ak a†p |{ηk }i,
(2π)6 2 Ek Ep
Z 3 3
d kd p ηk ηp ³ 3 (3) ~ †
´
= p (2π) δ (k − p
~) + h{η k }|ap a k |{ηk }i ,
(2π)6 2 Ek Ep
Z Z 3 3
d3 k ηk2 d kd p ηk2 ηp2
= + .
(2π)3 2Ek (2π)6 4Ek Ep
It is therefore quite easy to see that
Z
2 2 d3 k ηk2
h(∆N ) i = N2 −N = .
(2π)3 2Ek
PHYSICS 513: QUANTUM FIELD THEORY HOMEWORK 4 3

2. We are given the Lorentz commutation relations,


[J µν , J ρσ ] = i(g νρ J µσ − g µρ J νσ − g νσ J µρ + g µσ J νρ ).
a) Given the generators of rotations and boosts defined by,
1
Li = ²ijk J jk K i = J 0i ,
2
we are to explicitly calculate all the commutation relations. We are given trivially that
[Li , Lj ] = i²ijk Lk .
Let us begin with the K’s. By direct calculation,
[K i , K j ] = [J 0i , J 0j ] = i(g 0i J 0j − g 00 J ij − g ij J 00 + g 0j J i0 ),
= −iJ ij ;
= −2i²ijk Lk .
Likewise, we can directly compute the commutator between the L and K’s. This also will
follow by direct calculation.
1
[Li , K j ] = ²lk [J ilk , J 0j ],
2
1
= ²ilk i(g l0 J ij − g i0 J lj − g lj J i0 + g ij J l0 ),
2
= i²ijk J 0k ;
= i²ijk K k .
We were also to show that the operators
i 1 1
J+ = (Li + iK i ) J−i
= (Li − iK i ),
2 2
could be seen to satisfy the commutation relations of angular momentum. First let us
compute,
1£ i ¤
[J+ , J− ] = (L + iK i ), (Lj − iK i ) ,
4
1¡ i j ¢
= [L , L ] + i[K i , Lj ] − i[Li , K j ] + [K i , K j ] ,
4
= 0.
In the last line it was clear that I used the commutator [Li , K j ] derived above. The next
two calculations are very similar and there is a lot of ‘justification’ algebra in each step.
There is essentially no way for me to include all of the details of every step, but each can be
verified (e.g. i[K i , Lj ] = −i[Lj , K i ] = (−i)i²jik K k = −²ijk K k ...etc). They are as follows:
i j 1£ i ¤
[J+ , J+ ]= (L + iK i ), (Lj + iK j ) ,
4
1¡ i j ¢
= [L , L ] + i[K i , Lj ] + i[Li , K j ] + i[Li , K i ] − [K i , K j ] ,
4
1 ¡ ijk k ¢
= i² L − ²ijk K k − ²ijk K k + i²ijk Lk ,
4
1
= i²ijk (Lk + iK k ) = i²ijk J+ k
.
2
Likewise,
i j 1£ i ¤
[J− , J− ]= (L − iK i ), (Lj − iK j ) ,
4
1¡ i j ¢
= [L , L ] − i[K i , Lj ] − i[Li , K j ] + i[Li , K i ] − [K i , K j ] ,
4
1 ¡ ijk k ¢
= i² L + ²ijk K k + ²ijk K k + i²ijk Lk ,
4
1
= i²ijk (Lk − iK k ) = i²ijk J− k
.
2
‘ ’
óπ²ρ ²́δ²ι δ²Äιξαι
4 JACOB LEWIS BOURJAILY

b) Let us consider first the (0, 12 ) representation. For this representation we will need to satisfy
i 1 i 1 i σi
J+ = (L + iK i ) = 0 i
J− = (L − iK k ) = .
2 2 2
σi iσ i
This is obtained by taking Li = 2 and K i = 2 . The transformation law then of the (0, 12 )
representation is
µν
Φ(0, 12 ) −→ e−iωµν J Φ(0, 12 ) ,
i
Li +β j K j )
= e−i(θ Φ(0, 21 ) ,
i i j j
− iθ 2σ + β 2K
=e Φ(0, 12 ) .
σi i
The calculation for the ( 12 , 0) representation is very similar. Taking Li = 2 and K i = − σ2 ,
we get
i 1 σi 1
J+ = (Li + iK i ) = J−i
= (Li − iK k ) = 0.
2 2 2
Then the transformation law of the representation is
µν
Φ( 12 ,0) −→ e−iωµν J Φ( 12 ,0) ,
i
Li +β j K j )
= e−i(θ Φ( 21 ,0) ,
i i j j
− iθ 2σ − β 2K
=e Φ( 12 ,0) .
Comparing these transformation laws with Peskin and Schroeder’s (3.37), we see that
ψL = Φ( 12 ,0) ψR = Φ(0, 12 ) .
3. a) We are given that Ta is a representation of some Lie group. This means that
[Ta , Tb ] = if abc Tc
by definition. Allow me to take the complex conjugate of both sides. Note that [Ta , Tb ] =
[(−Ta ), (−Tb )] in general and recall that f abc are real.
[Ta , Tb ]∗ = (if abc Tc )∗ ,
[Ta∗ , Tb∗ ] = −if abc Tc∗ ,
∴ [(−Ta∗ ), (−Tb∗ )] = if abc (−Tc∗ ).
So by the definition of a representation, it is clear that (−Ta∗ ) is also a representation of the
algebra.
b) As before, we are given that Ta is a representation of some Lie group. We will take the
Hermitian adjoint of both sides.
[Ta , Tb ]† = (if abc Tc )† ,
(Ta Tb )† − (Tb Ta )† = −if abc Tc† ,
Tb† Ta† − Ta† Tb† = −if abc Tc† ,
[Tb† , Ta† ] = −if abc Tc† ,
∴ [Ta† , Tb† ] = if abc Tc† .
So by the definition of a representation, it is clear that Ta† is a representation of the algebra.
a
c) We define the spinor representation of SU (2) by Ta = σ2 so that
µ ¶ µ ¶ µ ¶
1 0 1 1 0 −i 1 1 0
T1 ≡ T2 ≡ T3 ≡ .
2 1 0 2 i 0 2 0 −1
We will consider the matrix S = iσ 2 . Clearly S is unitary because (iσ 2 )(iσ 2 )† = 1. Now,
one could proceed by direct calculation to demonstrate that
µ ¶ µ ¶ µ ¶
1 0 −1 1 0 −i 1 −1 0
ST1 S † = = −T1∗ ST2 S † = = −T2∗ ST3 S † = = −T3∗ .
2 −1 0 2 i 0 2 0 1
This clearly demonstrates that the representation −Ta∗ is equivalent to that of Ta .
PHYSICS 513: QUANTUM FIELD THEORY HOMEWORK 4 5

i i
d) From our definitions of our representation of SO(3, 1) using J+ and J− , it is clear that
i † i
(J+ ) = J− .
This could be expressed as if ( 21 , 0)† = (0, 12 ), or, rather L† = R. So what we must ask
ourselves is, does there exist a unitary matrix S such that
SLS † = L but SKS † = −K ?
If there did exist such a unitary transformation, then we could conclude that L and R
are equivalent representations. However, this is not possible in our SO(3, 1) representation
because both L and K are represented strictly by the Pauli spin matrices so that iK = L =
σ
2 . It is therefore clear that there cannot exist a transformation that will change the sign
of K yet leave L alone. So the representations are inequivalent.
‘ ’
óπ²ρ ²́δ²ι δ²Äιξαι

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