Spinor Tech Summary
Kiyoshi Shiraishi June 15, 2014
Abstract
We summarize some definitions and identities on the spinorial tech- nique in writing the scattering amplitudes.
1 Two-spinors and Basic definitions
Here
k 2 ≡ k µ k µ ≡ η µν k µ k ν ≡ (k 0 ) 2 − (k 1 ) 2 − (k 2 ) 2 − (k 3 ) 2 = 0 (1) k 0 = k 0 , k i = − k i (i = 1, 2, 3) (2)
|j ± ≡ u ± (k j ) , j ± | ≡ u ± (k j ) (3) ij ≡ i − |j + = u − (k i )u + (k j ) (4) [ij] ≡ i + | j − = u + (k i )u − (k j ) (5) u + (k) = k +
k − e iφ
k, u − (k) = k − e − iφ
k− k +
(6) where
e ±iφ
k= k 1 ± ik 2
(k 1 ) 2 + (k 2 ) 2 = k 1 ± ik 2
k + k − , k ± = k 0 ± k 3 (7) u + (k) = u † + (k) =
k + ,
k − e − iφ
k, u − (k) = u † − (k) =
k − e iφ
k, − k +
(8) ij =
k i− k j+ e iφ
ki−
k i+ k j− e iφ
kj(9)
[ij] =
k i+ k j − e − iφ
kj−
k i − k j+ e −iφ
ki(10) ij[ji] = 2k i · k j (11)
|ij| = |[ij]| =
2k i · k j (12)
ji = −ij , [ji] = −[ij] (13) especially,
ii = i − |i + = u − (k i )u + (k i ) = 0 (14) [ii] = i + | i − = u + (k i )u − (k i ) = 0 (15)
u + (k)u + (k) = k +
k − e iφ
kk + ,
k − e − iφ
k=
k +
k + k − e −iφ
kk + k − e iφ
kk −
=
k 0 + k 3 k 1 − ik 2 k 1 + ik 2 k 0 − k 3
= k 0 σ 0 + k i σ i = k 0 σ 0 − k i σ i (16)
u − (k)u − (k) = k − e − iφ
k−
k + k − e iφ
k, − k +
=
k − −
k + k − e − iφ
k−
k + k − e iφ
kk +
=
k 0 − k 3 − k 1 + ik 2
− k 1 − ik 2 k 0 + k 3
= k 0 σ 0 − k i σ i = k 0 σ 0 + k i σ i (17) where
σ 0 =
1 0 0 1
, σ 1 =
0 1 1 0
, σ 2 =
0 −i i 0
, σ 3 =
1 0 0 −1
(18) (k 0 σ 0 ± k i σ i )u ± (k) = 0 (‘Dirac equation ) (19) u − (k) = iσ 2 u ∗ + (k) , u − (k) = u T + (k)( − i)σ 2 (20) u − (k i )u − (k j ) = u T + (k i )(−i)σ 2 iσ 2 u ∗ + (k j ) = u T + (k i )u ∗ + (k j ) = u + (k j )u + (k i ) (21)
u − (k i )σ i u − (k j ) = u T + (k i )(−i)σ 2 σ i iσ 2 u ∗ + (k j ) = −u T + (k i )(σ i ) T u ∗ + (k j ) = −u + (k j )σ i u + (k i ) (22)
Fierz identity
σ µ = (1, σ i ) (23)
(σ µ ) ab (σ µ ) cd = δ ab δ cd − (σ i ) ab (σ i ) cd = −2(σ 2 ) ac (σ 2 ) bd (24) i + | σ µ | j + p + | σ µ | q + = u † + (k i )σ µ u + (k j )u † + (k p )σ µ u + (k q )
= − 2u † + (k i )u − (k p )u † − (k j )u + (k q )
= −2jq[ip] (25)
Schouten identity
ab cd = δ ac δ bd − δ ad δ bc (26) ac db = δ ad δ cb − δ ab δ cd (27) ad bc = δ ab δ dc − δ ac δ db (28) Thus
ab cd + ac db + ad bc = 0 (29) Then
ijk + ijk + ikj = 0 (30)
“eikonal” identity
k − 1
i=j
i (i + 1)
iqq (i + 1) = jk
jqqk (31)
which can be proved by jk
jqqk + k (k + 1)
kqq (k + 1) = jk q (k + 1) − jq k (k + 1) jqqkq (k + 1)
= − kj q (k + 1) − jq k (k + 1) jqqkq (k + 1)
= qkj (k + 1) jq qk q (k + 1)
= j (k + 1)
jq q (k + 1) (32)
where Schouten identity is used.
2 Four-component spinors
gamma matrices
Bjorken-Drell rep.
γ 0 =
1 0 0 − 1
, γ i =
0 σ i
− σ i 0
, γ 5 =
0 1 1 0
(33) {γ µ , γ ν } = 2η µν , γ 5 γ µ + γ µ γ 5 = 0 , (γ 5 ) 2 = 1 (34) four component spinor
U + (k) = 1
√ 2
u + (k) u + (k)
, U − (k) = 1
√ 2
u − (k)
− u − (k)
(35)
γ 5 U ± (k) = ±U ± (k) (36)
U + (k) = U + † (k)γ 0 = 1
√ 2 (u + (k) , −u + (k)) (37) U − (k) = U − † (k)γ 0 = 1
√ 2 (u − (k) , u − (k)) (38) U ± (k)γ 5 = ∓U ± (k) (39) U ± (k i )γ 0 U ± (k j ) = u ± (k i )u ± (k j ) (40) U ± (k i )γ i U ± (k j ) = ±u ± (k i )σ i u ± (k j ) (41) U ∓ (k i )γ µ U ± (k j ) = ±U ∓ (k i )γ µ γ 5 U ± (k j ) = ∓U ∓ (k i )γ 5 γ µ U ± (k j )
= −U ∓ (k i )γ µ U ± (k j ) = 0 (42)
|j ± ≡ U ± (k j ) , j ± | ≡ U ± (k j ) N ote! the same notation as 2spinors (43) i ± | j ± = U ± (k i ) U ± (k j ) = 0 (44) i − |j + = U − (k i )U + (k j ) = ij , i + |j − = U + (k i )U − (k j ) = [ij] (45) i ± | γ µ | i ± = U ± (k i )γ µ U ± (k i ) = 2k µ i (46) i − |γ µ |j − = U − (k i )γ µ U − (k j ) = U + (k j )γ µ U + (k i ) = j + |γ µ |i + (47) i ∓ |γ µ |j ± = U ∓ (k i )γ µ U ± (k j ) = 0 (48) Fierz identity
i − |γ µ |j − p + |γ µ |q + = j + |γ µ |i + p + |γ µ |q + = −2iq[jp] (49)
i − |γ µ |j − γ µ = 2(|j − i − | + |i + j + |) (50) i + | γ µ | j + γ µ = 2( | j + i + | + | i − j − | ) (51)
‘Dirac equation’
k/ U ± (k) = k/ | k ± = 0 (52) Projector
U ± (k)U ± (k) = 1 2
u ± (k)u ± (k) ∓u ± (k)u ± (k)
±u ± (k)u ± (k) −u ± (k)u ± (k)
= 1
2 (1 ± γ 5 )k/ (53)
re-discover:
ij[ji] = i − |j + j + |i − = tr U − (k i )U + (k j )U + (k j )U − (k i )
= tr
1 − γ 5 2 k/ i k/ j
= 2k i · k j (54)
3 QED (QCD) Examples (I)
First of all, remember that
s ij = (k i + k j ) 2 = 2k i · k j = ij [ji] (55)
3.1 e − e + → µ − µ +
(Of course, the amplitude for e − e + → q q ¯ can be obtained similarly) A 4 = ie 2 A 4 δ(
i
k i ) (56)
3.1.1 e − L (1)e + R (2) → µ − R (3)µ + L (4)
A 4 = 2 − | γ µ | 1 − 3 + | γ µ | 4 + s 12
= −2 24 [13]
s 12
(57) here we used (49).
| A 4 | = 2 |s 13 |
s 12 ∝ 1 − cos θ (CMF ) (58) helicity suppressed as 1 3 or 2 4
A 4 = − 2 24 [13]
s 12
= − 2 24 [13] 13
12[21]13 = 2 24 [24] 24
12[24]43 = − 2 24 2
1234 (59) here we used
4 j=1
ij [jk] = 0 (derived f rom (16)) , s 12 = s 34 , s 13 = s 24 (60) Exercise: Show
A 4 = −2 [13] 2
[12][34] (61)
3.1.2 e − R (1)e + L (2) → µ − R (3)µ + L (4) Using (47), we obtain
A 4 = +2 14 2
1234 (62)
3.1.3 e − L (1)e + R (2) → µ − L (3)µ + R (4)
A 4 = +2 23 2
12 34 (63)
3.1.4 e − R (1)e + L (2) → µ − L (3)µ + R (4)
A 4 = −2 13 2
1234 (64)
3.1.5 Unpolarized, helicity-summed cross sections
dσ(e
−e
+→µ
−µ
+)
d cos θ ∝ 1
2
helicity
|A 4 | 2 = 4 24 2 1234
2 + 14 2
1234 2
= 4 s 2 13 + s 2 14
s 2 12 ∝ (1 − cos θ) 2 + (1 + cos θ) 2 ∝ 1 + cos 2 θ(65) e − e + → µ − µ +
s 12 = s, s 13 = t, s 14 = u dσ dΩ = α 2
2s t 2 + u 2
s 2 (66)
(In the limit of t → 0, dΩ dσ → α 2s
2) e − µ − → e − µ −
s 12 = t, s 13 = s, s 14 = u dσ dΩ = α 2
2s
s 2 + u 2
t 2 (67)
(In the limit of t → 0, dΩ dσ → α t
22s )
3.2 e − e − , e − e + scattering
e(1)e(2) → e(3)e(4)
A + −− + = 3 − |γ µ |1 − 4 + |γ µ |2 + s 13
= +2 23[14]
s 13
(68)
A + − + − = − 4 − |γ µ |1 − 3 + |γ µ |2 + s 14
= −2 24[13]
s 14
(note the sign f rom exchange 3 ↔ 4) (69)
A ++−− = 3 − | γ µ | 1 − 4 − | γ µ | 2 −
s 13 − 4 − | γ µ | 1 − 3 − | γ µ | 2 − s 14
= − 2 34 [12]
1 s 13
+ 1 s 14
= +2 34 [12]
s 12 s 13 s 14
(70)
since s 12 + s 13 + s 14 = 0.
Unpolarized, helicity-summed cross sections
|A| 2 ∝ s 2 14 s 2 13 + s 2 13
s 2 14 + s 4 12
s 2 13 s 2 14 = s 4 12 + s 4 13 + s 4 14
s 2 13 s 2 14 (71) For e − e − → e − e − or e + e + → e + e + (Møller scattering),
s 12 = s, s 13 = t, s 14 = u
|A| 2 ∝ s 4 + t 4 + u 4
t 2 u 2 (72)
dσ
dΩ = α 2 2s
s 4 + t 4 + u 4
t 2 u 2 (73)
= α 2 2s
s 2 + u 2
t 2 + s 2 + t 2 u 2 + 2 s 2
ut
(74)
= α 2 4s
s − u
t + s − t u
2
(75) (In the limit of t → 0, dΩ dσ → α t
22s )
For e − e + → e − e + (Bhabha scattering), s 13 = s, s 14 = t, s 12 = u
| A | 2 ∝ s 4 + t 4 + u 4
s 2 t 2 (76)
dσ
dΩ = α 2 2s
s 4 + t 4 + u 4
s 2 t 2 (77)
= α 2 2s
s 2 + u 2
t 2 + u 2 + t 2 s 2 + 2 u 2
st
(78)
= α 2 4s
s − u
t + t − u s
2
(79)
(In the limit of t → 0, dΩ dσ → α t
22s )
4 Spinor-helicity rep. for polarization
4.1 Polarization vectors
+ µ (k, q) = q − √ |γ µ |k −
2qk , − µ (k, q) = q + √ |γ µ |k +
2[kq] (80)
where q · k does not vanish.
k · ± (k, q) = 0 (T ransverse) (f rom Dirac eq.) (81) + · − = q − |γ µ |k − q + |γ µ |k +
2 qk [kq] = −2qk[kq]
2 qk [kq] = −1 (82) + · + = q − |γ µ |k − q − |γ µ |k −
2 qk 2 = q − |γ µ |k − k + |γ µ |q +
2 qk 2 = 0 (83) + µ − ν + − µ + ν = − η µν + k µ q ν + k ν q µ
k · q (84)
where we used (47), (53), (46) and γ µ q/γ ν + γ ν q/γ µ = 2(q ν γ µ + q µ γ ν − q/η µν ). It is easy to confirm k · + − ν + k · − + ν = q · + − ν + q · − + ν = 0.
From (53),
U ± (p)U ± (p) = 1
2 (1 ± γ 5 )p / (85)
then for arbitrary p p · + (k, q) = q √ − |p /|k −
2qk = qp[pk] √
2qk , p · − (k, q) = q √ + |p /|k +
2[kq] = [qp]pk √ 2[kq] (86) Thus we find
q · ± = 0 (and rediscover k · ± = 0) (87) Exercise. Show
+ (k 1 , q) · + (k 2 , q) = − (k 1 , q) · − (k 2 , q) = 0 (88) + (k 1 , q) · − (k 2 , k 1 ) = 0 (89) Actually, you must show
+ (k, q) · + (k , q ) = − qq [kk ]
qk q k (90) + (k, q) · − (k , q ) = − qk [kq ]
qk [k q ] (91) Using (51), we find
/ + (k, q) =
√ 2
qk (|k − q − | + |q + k + |) , / − (k, q) =
√ 2
[kq] (|k + q + | + |q − k − |) (92) Then
/ ± (k, q) | q ± = 0 , q ∓ | / ± (k, q) = 0 (93)
4.2 Significance of q
+ µ (k, q ) = q √ − | γ µ | k −
2 q k = q − √ | γ µ | k − k − | q +
2 q k kq = √ q − | γ µ k/ | q + 2 q k kq
= − q √ − |k/γ µ |q + 2q kkq +
√ 2q q q k kq k µ
= + µ (k, q) +
√ 2q q
q k kq k µ (94)
It’s a gauge degree of freedom!
5 QED (QCD) example (II)
5.1 two fermions and two photons
A +−λ
3λ
4= 2 − | / λ
4(k 4 , q 4 )(p / 1 + k/ 3 ) / λ
3(k 3 , q 3 ) | 1 − s 13
+ 2 − | / λ
3(k 3 , q 3 )(p / 1 + k/ 4 ) / λ
4(k 4 , q 4 ) | 1 − s 14
(95) For λ 3 = λ 4 = −, this vanishes if we take q 3 = q 4 = p 1 .
For λ 3 = λ 4 = +, this vanishes if we take q 3 = q 4 = p 2 .
A +−+− = 2 − | / − (k 4 , q 4 )(p / 1 + k/ 3 ) / + (k 3 , p 2 )|1 − s 13
=
√ 2
[4q 4 ] 24 q 4 + | (p / 1 + k/ 3 ) | 2 + [31]
√ 2 23
1
s 13 (96)
The choice q 4 = k 3 leads to A + − + − =
√ 2
[43] 24 3 + | p / 1 | 2 + [31]
√ 2 23
1
s 13 = 2 24[31]12[31]
[43] 23 s 13
= 2 24 [31] 12 [31]
[43]2313[31] = 2 24 [34] 42
[34]2313 = − 2 24 2
1323 (97) or
A + − + − = 2 24[31]12[31]
[43] 23 s 13 = −2 [13] 2 2412 23 [34]s 24
= +2 [13] 2 2412
21 [14] 24 [42] = 2 [13] 2
[14][24] (98)
By exchanging 3 ↔ 4, we obtain
A +−−+ = − 2 23 2
1424 (99)
Unpolarized, helicity-summed cross sections
|A| 2 ∝ |s 14 |
| s 13 | + |s 13 |
| s 14 | (100)
For e − γ → e − γ or e + γ → e + γ,
s 13 = s, s 12 = t, s 14 = u
|A| 2 ∝ s 2 + u 2
|su| (101)
For e − e + → γγ,
s 12 = s, s 13 = t, s 14 = u
| A | 2 ∝ t 2 + u 2
|tu| (102)
5.2 e − e + → qg¯ q
Using Fierz identity, we find A 5 = 25
s 12
1 + | (k/ 3 + k/ √ 4 )/ + (k 4 , q) | 3 −
2s 34 + [13]
s 12
2 − | (k/ 4 + k/ √ 5 )/ + (k 4 , q) | 5 +
2s 45 (103)
Using (92), we can rewrite A 5 as A 5 = 25
s 12
1 + | (k/ 3 + k/ 4 ) | q + [43]
s 34 q4 + [13]
s 12
2 − | (k/ 4 + k/ 5 ) | 4 − q5
s 45 q4 (104)
Choosing q = k 5 , we remove the second term and get A 5 = − 25
s 12
1 + | (k/ 3 + k/ 4 ) | 5 + [43]
s 34 45
= 25 1 + | (k/ 1 + k/ 2 + k/ 5 ) | 5 + [43]
12[21]34[43]45
= 25[12]25[43]
12 [21] 34 [43] 45
= − 25 2
12 34 45 (105)
where we used 5
i=1 k i = 0, Dirac eqs. and (53).
Note that
25 2
123445 = 35 3445
25 2
1235 (106)
6 Gluon amplitudes
• “Color” factors are separated (and ordered).
• Gluon vertices include · .
• Since + (k 1 , q) · + (k 2 , q) = 0, A(+ + · · · +) = 0 can be shown.
• Using − (k 1 , q) · + (k 2 , k 1 ) = 0, A( − + · · · +) = 0 is also shown.
6.1 4-point amplitude
6.1.1 an amplitude
• Calculate A 4 (1 − 2 − 3 + 4 + ).
• Choose q 1 = q 2 = k 3 , q 3 = q 4 = k 2 , only nonvanishing · is − (k 1 , k 3 ) · + (k 4 , k 2 ) = 24 [31] 21 [43] .
• only s 12 channel contributes
A 4 (1 − 2 − 3 + 4 + )
= i
√ 2 2
[ − 2k 1 · − (k 2 , k 3 ) − µ (k 1 , k 3 )] − ig µν s 12
[2k 4 · + (k 3 , k 2 ) + ν (k 4 , k 2 )]
= − 2i s 12
k 1 · − (k 2 , k 3 ) k 4 · + (k 3 , k 2 ) − (k 1 , k 3 ) · + (k 4 , k 2 )
= − 2i s 12
[31] √ 12 2[23]
24 [43]
√ 2 23
21 [43]
24 [31] = − i 12 2 [34] 2 s 12 s 23
= i 12 4
12 23 34 41 (107)
Using cyclic symmetry, we get
A 4 (1 + 2 − 3 − 4 + ) = i 23 4
12233441 (108) 6.1.2 decoupling identity
We consider SU (N) gauge theory, not U (N) gauge theory. The vertices come
from the commutater in the field strength, thus if one of the generator T a is
replaced by unity, the amplitude (possibly thought as in U (N) theory) must
vanish.
The full amplitude looks like
A = g 2
noncyclic perms
Tr(T a
1T a
2T a
3T a
4)A(1234) (109) (which can be generalized to n-point amplitudes)
Noncyclic means that, roughly speaking, 1 is fixed (or permutation σ ∈ S n /Z n ), because of the cyclicity A(1234) = A(4123).
Turning to the discussion, the following holds:
0 = T r(T a
1T a
2T a
3)[A(1234) + A(1243) + A(1423)]
+ T r(T a
1T a
3T a
2)[A(1324) + A(1342) + A(1432)] (110) Therefore we find
A(1234) + A(1243) + A(1423) = A(1324) + A(1342) + A(1432) = 0 (111) and then
A(1 − 2 + 3 − 4 + ) = − A(1 − 2 + 4 + 3 − ) − A(1 − 4 + 2 + 3 − ) (112)
A(1 − 2 + 3 − 4 + ) = −A(1 − 2 + 4 + 3 − ) − A(1 − 4 + 2 + 3 − )
= − A(3 − 1 − 2 + 4 + ) − A(3 − 1 − 4 + 2 + )
= − i
31 4
31122443 + 31 4 31144223
= −i 13 3 24
1
12 34 + 1 14 23
= i 13 3 24
14 23 + 12 34 12233441
= i 13 3 24
− 13 42
12233441 = i 13 4
12233441 (113) where we used Schouten identity (30).
6.1.3 cross section
colors
|A| 2 = 2N 2 (N 2 − 1)g 4 (|A(1234)| 2 + |A(1342)| 2 + |A(1423)| 2 ) (114) because of (6.1.2) and the reflection symmetry 1 A(1234) = A(4321). Then
colors
|A| 2 (1 − 2 − 3 + 4 + ) = 2N 2 (N 2 − 1)g 4 s 4 1
s 2 u 2 + 1 t 2 s 2 + 1
u 2 t 2
(115)
1
A(12 · · · n) = ( − 1)
nA(n · · · 21) in general
and summing over helicities, we find
colors