Radiative corrections in K l3 decays
description
Transcript of Radiative corrections in K l3 decays
Radiative corrections in Kl3
decays
Andrea MarroccoPh.D. student, University “Roma Tre”
[Ph.D. thesis supervisor: G. Isidori]
Thesis Decay rate calculation including
radiative corrections
0
0
K
K
Independent determination of |Vus|Improve the theoretical indetermination of this parameter
The rates ratio of the electronic and the muonic channel is |Vus| independent
It is possible to test the accuracy required in the CHPT expansion
Dimensional regularization for both UV & IR divergences
The decay amplitude
Real photon emissionγ,q
K+,p4 π0,p1
νµ,p3
µ+,p2
γ,qK+,p4
π0,p1
νµ,p3µ+,p2
K+,p4 π0,p1
µ+,p2
γ,q
νµ,p3
2
Virtual photon
exchange
K+,p4
µ+,p2
π0,p1
νµ,p3 kq
hνµ,p3
π0,p1K+,p4
µ+,p2
+
π0,p1K+,p4
µ+,p2
νµ,p3
+
q
h
K+,p4 π0,p1
νµ,p3µ+,p2
+
K+,p4
µ+,p2
π0,p1
νµ,p3
+
K+,p4 π0,p1
νµ,p3
µ+,p2
+
K+,p4
µ+,p2
π0,p1
νµ,p3+
K+,p4 π0,p1
νµ,p3
µ+,p2
+
K+,p4π0,p1
νµ,p3µ+,p2+
K+,p4
µ+,p2
π0,p1
νµ,p3
2
1414
25
3*
,,
12
ppvtfppvtf
pvpuVG
A
KK
usF
Self energy
Vertex modification
51 AZ
Wave function renormalization
512
1 AZ
+ 512
1 AZ
A,p A,p
pA
22
2
Amp
AA p
pZ
“A” particle self energy
1
02)1(
1
bzaz
dz
ab
Standard Feynman parameterization
1
2
22
2
2
22
11
224
1
2
12
4
11
2
dn
dn
E
Ed
Ed
dn
dn
E
dE
d
n
dn
d
l
lld
n
dn
l
ld
K+,p4
h
q
K+,p4
K+,p4 K+,p4+K+,p4
h
q
K+,p4
K+,p4 K+,p4+
2
6522
212
2222
2422
9
20
3
8
2
2
2kk
kkk
kd
dd
kK pkkepkkeimppqqiq
qpqdiep
Ki = coefficients of the O(e2p2) mesonic Lagrangian [Urech, ‘95]
652
212
2
22
22
2
22
9
20
3
8,1
2,1,
21
2
2,2
2,3,
22
4
8
,12,2,
22
2
8,2,1,
22
2
2
4
22
kkekkenn
Fn
nnF
nn
nnF
nn
nnF
nm
n
me kn
n
kk
2
2
k
k
m
p
1
0
11 11,,, dxxxxbcb
ccbaF abcb
Hypergeometric functions
65
221
22
22
2
22
12 9
20
3
8
3212
1
4
22
1kkekke
nnn
n
me
mZ n
n
k
K
kK
μ+,p2 μ+,p2+
h
q
μ+,p2μ+,p2
pXe
iqiqpq
mpqqdiep n
nd
62
2242
22
6
22
22
2
22
13
1
4
22
1Xe
n
nn
me
mZ n
n
6222
2
22
2
22 ,1
2,2,
22
4,2,1,
22
2
2
4
22
Xemnn
Fn
nnF
n
nm
n
me n
n
m
p
Xi = coeff. of the O(e2p2) leptonic Lagrangian [Neufeld & Rupertsberger, ’95-96]
vpunn
Fnn
nnF
n
n
m
VGiekn
n
k
usF52
22
2
2*2
1,12,2,
22
2
4,2,1,
22
2
2
4
22
2
vppuvppuvpu kkk 555 12
11
2
11
K+,p4 π0,p1
νµ,p3
µ+,p2
222254
*2
2
12
22 kkk
kn
nnusF
mpqpqiq
vqpuqdVGe
2
2
k
k
m
p
K+,p4π0,p1
νµ,p3µ+,p2
2222
54*2
2
1
22 kn
nnusF
mpqpqiq
vmpquqdVGe
vum
n
nn
m
VGien
n
usF52
22
2
2*2
13
1
4
22
2
vppuvum k 55 11 Contributes only to the f-
function
µ+,p2νµ,p3
π0,p1K+,p4
k
q
h
2425413
42
222
42
21
22
1
22
pvqpmqpqpppu
iqpqiqpqiq
qdVGe
rs
n
nnusF
22153
2
12
pvIIpuVGe rsusF
1
03
1
0 11
12
1
cyxxybxadyxdx
abcFeynman parameterization
251432
251432
2
1,1,2
pvpppuppmHpvpppuppmGVGie rs
Kjrs
KjusF
Full agreement with Cirigliano et al.
24
4log2log
22
mm
M
mm KK
Real photon emission process
pvpuqVieG rusF
5*
*
12
pvqpppu
pq
pVieGk
k
kr
usF5
**
12
pvmqppppu
qp
qVieG
k
r
usF
5
**
1
22
0K
γ,q
K+,p4 π0,p1
νµ,p3
µ+,p2
γ,qK+,p4
π0,p1
νµ,p3µ+,p2
K+,p4 π0,p1
µ+,p2
γ,q
νµ,p3
2
Phase space separation 21
324 2,,;,;,,,; dlqplpdppldqppppd nkk
nlG
ln
mlppld
nnn
nn ,
21
2
,;2 2
1222
342
322
2
This formula is valid in n dimensions and the
result is based on Lorentz-covariance
considerations
In K+ rest frame
qppppdMm
mmd k
n
k
,,,;2 4
2
m
j jn
jnm
iimm
E
pdpPppPd
11
1
41
22,....,;
Decay rate
2
22
1
0
1
022
2
32
3
2
322
32
2
322
22
2
1222
21
1
21
1
,
,
22
21
2
12
222
2
2
M
xEC
mE
xddx
xEC
mE
xx
ECllEA
lEAmEdEdl
nnm
mm
nn
n
nnm
lmm
m
mm
m
nnk
k
k
k
22
22
2222 2,
mEEmEC
mEEmEC
lEmmmlEA
k
k
kk
The infrared divergence is hidden in this
factor
It has no divergent terms and can be
analytically expressed using hypergeometric
functions
522
2
2222
,1
0,2
n
k
k
lEAE
M
lEAm
lmmE
21cos
21
2
, 222
xEC
mE
EC
lEAE
Strategy to isolate the divergences
25222
,,,,,
222
lEnflEAlEnkdEn
m
lmm
m
k
k
result of the integration
on the photon
variables
All other factors are in this function
Coordinate transformation
22
2,
lmm
lEAz
k
1
0 0
221
1
0
21 ,,0,,,, dz
lzjlzjzdzlzjz
0,0,0,0,0,,0,0, 21
0
222
lj
dzz
ljzljlj
• Full analytical agreement with Cirigliano et al. in the virtual corrections
• Differential decay rate calculation with real emission completed -> explicit check of the cancellation of infrared divergences
• The IR-safe observable differential rate depends on z and l2. For each bin of l2 we are numerically calculating the O(α) corrections to the decay rate (numerical results in progress..).
• Calculation performed for both K+ and K0 decays
• For each channel we expect to reach the same accuracy of Cirigliano et al. (counterterms error ~ few x 0.001)
• For the ratio between the decay rates of electronic channel and muonic channel we expect a better accuracy because many counterterms cancel (~ 0.001)
Conclusions & Outlook