S
eminaire
P
oinar
e
2
(2002)
93
{
125
S
eminaire
P
oina
r
e
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
Mar
Kne
h
t
Cen
tre
de
Ph
ysique
Th
eorique
CNRS-Lumin
y
,
Case
907
F-13288
Marseille
Cedex
9,
F
rane
1
In
tro
dution
In
F
ebruary
2001,
the
Muon
(g-2)
Collab
oration
of
the
E821
exp
erimen
t
at
the
Bro
okha
v
en
A
GS
released
a
new
v
alue
of
the
anomalous
magneti
momen
t
of
the
m
uon,
measured
with
an
unpree-
den
ted
auray
of
1.3
ppm.
This
announemen
t
has
aused
quite
some
exitemen
t
in
the
partile
ph
ysis
omm
unit
y
.
Indeed,
this
exp
erimen
tal
v
alue
w
as
laimed
to
sho
w
a
deviation
of
2.6
with
one
of
the
most
aurate
ev
aluation
of
the
anomalous
magneti
momen
t
of
the
m
uon
within
the
standard
mo
del.
It
w
as
subsequen
tly
sho
wn
that
a
sign
error
in
one
of
the
theoretial
on
tributions
w
as
resp
onsible
for
a
sizable
part
of
this
disrepany
,
whi
h
ev
en
tually
only
amoun
ted
to
1.6
.
Ho
w
ev
er,
this
ev
en
t
had
the
merit
to
dra
w
the
atten
tion
to
the
fat
that
lo
w
energy
but
high
preision
exp
erimen
ts
represen
t
real
p
oten
tialities,
omplemen
tary
to
the
high
energy
aelerator
programs,
for
evidening
p
ossible
new
degrees
of
freedom,
sup
ersymmetry
or
whatev
er
else,
b
ey
ond
those
desrib
ed
b
y
the
standard
mo
del
of
eletromagneti,
w
eak,
and
strong
in
terations.
Clearly
,
in
order
for
theory
to
mat
h
su
h
an
aurate
measuremen
t
[in
the
mean
time,
the
relativ
e
error
has
ev
en
b
een
further
redued,
to
0.7
ppmâ„„,
alulations
in
the
standard
mo
del
ha
v
e
to
b
e
pushed
to
their
v
ery
limits.
The
diÆult
y
is
not
only
one
of
ha
ving
to
ompute
higher
orders
in
p
erturbation
theory
,
but
also
to
orretly
tak
e
in
to
aoun
t
strong
in
teration
on
tributions
in
v
olving
lo
w-energy
sales,
where
non
p
erturbativ
e
eets
are
imp
ortan
t,
and
whi
h
therefore
represen
t
a
real
theoretial
hallenge.
The
purp
ose
of
this
aoun
t
is
to
giv
e
an
o
v
erview
of
the
main
features
of
the
theoretial
alulations
that
ha
v
e
b
een
done
in
order
to
obtain
aurate
preditions
for
the
anomalous
magneti
momen
ts
of
the
eletron
and
of
the
m
uon
within
the
standard
mo
del.
There
exist
sev
eral
exellen
t
reviews
of
the
sub
jet,
whi
h
the
in
terested
reader
ma
y
onsult.
As
far
as
the
situation
up
to
1990
is
onerned,
the
olletion
of
artiles
published
in
Ref.
[1â„„
oers
a
w
ealth
of
information,
on
b
oth
theory
and
exp
erimen
t.
A
v
ery
useful
aoun
t
of
earlier
theoretial
w
ork
is
presen
ted
in
Ref.
[2â„„.
Among
the
more
reen
t
reviews,
Refs.
[3
,
4,
5,
6
â„„
are
most
informativ
e.
I
shall
not
tou
h
on
the
sub
jet
of
the
study
of
new
ph
ysis
senarios
whi
h
migh
t
oer
an
explanation
for
a
p
ossible
deviation
b
et
w
een
the
standard
mo
del
predition
of
the
magneti
momen
t
of
the
m
uon
and
its
exp
erimen
tal
v
alue.
F
or
this
asp
et,
I
refer
the
reader
to
[7
â„„
and
to
the
artiles
quoted
therein,
or
to
[8
â„„.
2
General
onsiderations
In
the
on
text
of
relativisti
quan
tum
me
hanis,
the
in
teration
of
a
p
oin
tlik
e
spin
one-half
partile
of
harge
e
`
and
mass
m
`
with
an
external
eletromagneti
eld
A
(x)
is
desrib
ed
b
y
the
Dira
equation
with
the
minimal
oupling
presription,
i
h
t
=
h
i
h
r
e
`
A
+
m
`
2
+
e
`
A
0
i
:
(2.1)
94
M.
Kne
h
t
S
eminaire
P
oinar
e
In
the
non
relativisti
limit,
this
redues
to
the
P
auli
equation
for
the
t
w
o-omp
onen
t
spinor
'
desribing
the
large
omp
onen
ts
of
the
Dira
spinor
,
i
h
'
t
=
(
i
h
r
(e
`
=)A)
2
2m
`
e
`
h
2m
`
B
+
e
`
A
0
'
:
(2.2)
As
is
w
ell
kno
wn,
this
equation
amoun
ts
to
asso
iate
with
the
partile's
spin
a
magneti
momen
t
M
s
=
g
`
e
`
2m
`
S
;
S
=
h
2
;
(2.3)
with
a
gyromagneti
ratio
predited
to
b
e
g
`
=
2.
In
the
on
text
of
quan
tum
eld
theory
,
the
resp
onse
to
an
external
eletromagneti
eld
is
desrib
ed
b
y
the
matrix
elemen
t
of
the
eletromagneti
urren
t
1
J
[spin
pro
jetions
and
Dira
indies
are
not
written
expliitlyâ„„
h`
(p
0
)jJ
(0)j`
(p)i
=
u(p
0
)
(p
0
;
p)u(p)
;
(2.4)
with
[k
p
0
p
â„„
(p
0
;
p)
=
F
1
(k
2
)
+
i
2m
`
F
2
(k
2
)
k
F
3
(k
2
)
5
k
:
(2.5)
This
expression
of
the
matrix
elemen
t
h`
(p
0
)jJ
(0)j`
(p)i
is
the
most
general
that
follo
ws
from
Loren
tz
in
v
ariane,
the
Dira
equation
for
the
t
w
o
spinors,
(6
p
m)u (p)
=
0,
u(p
0
)(6
p
0
m)
=
0,
and
the
onserv
ation
of
the
eletromagneti
urren
t,
(
J
)
(x)
=
0.
The
t
w
o
rst
form
fators,
F
1
(k
2
)
and
F
2
(k
2
),
are
kno
wn
as
the
Dira
(or
eletri)
form
fator
and
the
P
auli
(or
magneti)
form
fator,
resp
etiv
ely
.
Sine
the
eletri
harge
op
erator
Q
is
giv
en,
in
units
of
the
harge
e
`
,
b
y
Q
=
Z
dx
J
0
(x
0
;
x)
;
(2.6)
the
form
fator
F
1
(k
2
)
satises
the
normalization
ondition
F
1
(0)
=
1.
The
presene
of
the
form
fator
F
3
(k
2
)
requires
b
oth
parit
y
and
time
rev
ersal
in
v
ariane
to
b
e
brok
en.
It
is
therefore
absen
t
if
only
eletromagneti
in
terations
are
onsidered.
On
the
other
hand,
in
the
standard
mo
del,
the
w
eak
in
terations
violate
b
oth
parit
y
and
time
rev
ersal
symmetry
,
so
that
they
ma
y
indue
su
h
a
form
fator.
The
analyti
struture
of
these
form
fators
is
ditated
b
y
general
prop
erties
of
quan
tum
eld
theory
[ausalit
y
,
analytiit
y
,
and
rossing
symmetryâ„„.
They
are
real
funtions
of
k
2
in
the
spaelik
e
region
k
2
<
0.
In
the
timelik
e
region,
they
b
eome
omplex,
with
a
ut
starting
at
k
2
>
4m
2
`
.
A
t
k
2
=
0,
they
desrib
e
the
residue
of
the
s-
hannel
p
ole
in
the
S-matrix
elemen
t
for
elasti
`
+
`
sattering.
A
t
tree
lev
el,
i.e.
in
the
lassial
limit,
one
nds
F
tree
1
(k
2
)
=
1
;
F
tree
2
(k
2
)
=
0
;
F
tree
3
(k
2
)
=
0
:
(2.7)
In
order
to
obtain
non
zero
v
alues
for
F
2
(k
2
)
and
F
3
(k
2
)
already
at
tree
lev
el,
the
in
teration
of
the
Dira
eld
with
the
photon
eld
A
w
ould
ha
v
e
to
depart
from
the
minimal
oupling
presription.
F
or
instane,
the
mo
diation
[F
=
A
A
,
J
=
â„„
Z
d
4
xL
in
t
=
e
`
Z
d
4
xJ
A
!
!
Z
d
4
x
b
L
in
t
=
e
`
Z
J
A
+
h
4m
`
a
`
F
+
h
2e
`
d
`
i
5
F
=
e
`
Z
d
4
x
b
J
A
;
(2.8)
1
In
the
standard
mo
del,
J
denotes
the
total
eletromagneti
urren
t,
with
the
on
tributions
of
all
the
harged
elemen
tary
elds
in
presene,
leptons,
quarks,
eletro
w
eak
gauge
b
osons,...
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
95
with
2
b
J
=
J
h
2m
`
a
`
h
d
`
e
`
i
5
;
(2.9)
leads
to
b
F
tree
1
(k
2
)
=
1
;
b
F
tree
2
(k
2
)
=
a
`
;
b
F
tree
3
(k
2
)
=
d
`
=e
`
:
(2.10)
The
equation
satised
b
y
the
Dira
spinor
then
reads
i
h
t
=
i
hr
e
`
A
+
m
`
2
+
e
`
A
0
+
e
`
h
2m
`
a
`
(i
E
B)
hd
`
(
E
+
i
B)
;
(2.11)
and
the
orresp
onding
non
relativisti
limit
b
eomes
3
i
h
'
t
=
(
i
h
r
(e
`
=)A)
2
2m
`
e
`
h
2m
`
(1
+
a
`
)
B
E
+
e
`
A
0
+
'
:
(2.12)
Th
us
the
oupling
onstan
t
a
`
indues
a
shift
in
the
gyromagneti
fator,
g
`
=
2(1
+
a
`
),
while
d
`
giv
es
rise
to
an
eletri
dip
ole
momen
t.
The
mo
diation
(2.8)
of
the
in
teration
with
the
photon
eld
in
tro
dues
t
w
o
arbitrary
onstan
ts,
and
b
oth
terms
pro
dues
a
non
r
enormalizable
in
teration.
Non
onstan
t
v
alues
of
the
form
fators
ould
b
e
generated
at
tree
lev
el
up
on
in
tro
duing
[9
â„„
additional
non
renormalizable
ouplings,
in
v
olving
deriv
ativ
es
of
the
external
eld
of
the
t
yp
e
2
n
A
,
whi
h
preserv
e
the
gauge
in
v
ariane
of
the
orresp
onding
eld
equation
satised
b
y
.
In
a
renormalizable
framew
ork,
lik
e
QED
or
the
standard
mo
del,
alulable
non
v
anishing
v
alues
for
F
2
(k
2
)
and
F
3
(k
2
)
are
generated
b
y
the
lo
op
orretions.
In
partiular,
the
latter
will
lik
ewise
indue
an
anomalous
magneti
moment
a
`
=
1
2
(g
`
2)
=
F
2
(0)
(2.13)
and
an
eletri
dip
ole
momen
t
d
`
=
e
`
F
3
(0).
If
w
e
onsider
only
the
eletromagneti
and
the
strong
in
terations,
the
urren
t
J
is
gauge
in
v
ari-
an
t,
and
the
t
w
o
form
fators
symmetry
F
1
(k
2
)
and
F
2
(k
2
)
do
not
dep
end
on
the
gauges
hosen
in
order
to
quan
tize
the
photon
and
the
gluon
gauge
elds.
This
is
no
longer
the
ase
if
the
w
eak
in
ter-
ations
are
inluded
as
w
ell,
sine
J
no
w
transforms
under
a
w
eak
gauge
transformation,
and
the
orresp
onding
form
fators
in
general
dep
end
on
the
gauge
hoies.
As
w
e
ha
v
e
already
men
tioned
ab
o
v
e,
the
zero
momen
tum
transfer
v
alues
F
i
(0),
i
=
1;
2;
3
desrib
e
a
ph
ysial
S-matrix
elemen
t.
T
o
the
exten
t
that
the
p
erturbativ
e
S-matrix
of
the
standard
mo
del
do
es
not
dep
end
on
the
gauge
parameters
to
an
y
order
of
the
renormalized
p
erturbation
expansion,
the
quan
tities
F
i
(0)
should
dene
b
ona
de
gauge-xing
indep
enden
t
observ
ables.
The
omputation
of
(p
0
;
p)
is
often
a
tedious
task,
esp
eially
if
higher
lo
op
on
tributions
are
onsidered.
It
is
therefore
useful
to
onen
trate
the
eorts
on
omputing
the
form
fator
of
in
terest,
e.g.
F
2
(k
2
)
in
the
ase
of
the
anomalous
magneti
momen
t.
This
an
b
e
a
hiev
ed
up
on
pro
jeting
out
the
dieren
t
form
fators
[10
,
11
â„„
using
the
follo
wing
general
expression
4
F
i
(k
2
)
=
tr
[
i
(p
0
;
p)(6
p
0
+
m
`
)
(p
0
;
p)(6
p
+
m
`
)â„„
;
(2.14)
with
1
(p
0
;
p)
=
1
4
1
k
2
4m
2
`
+
3m
`
2
1
(k
2
4m
2
`
)
2
(p
0
+
p)
2
The
urren
t
b
J
is
still
a
onserv
ed
four-v
etor,
therefore
the
matrix
elemen
t
h`
(p
0
)j
b
J
(0)j`
(p)i
also
tak
es
the
form
(2.4),
(2.5),
with
appropriate
form
fators
b
F
i
(k
2
).
3
T
erms
in
v
olving
the
gradien
ts
of
the
external
elds
E
and
B
or
terms
nonlinear
in
these
elds
are
not
sho
wn.
4
F
rom
no
w
on,
I
most
of
the
time
use
the
system
of
units
where
h
=
1,
=
1.
96
M.
Kne
h
t
S
eminaire
P
oinar
e
2
(p
0
;
p)
=
m
2
`
k
2
1
k
2
4m
2
`
m
`
k
2
k
2
+
2m
2
`
(k
2
4m
2
`
)
2
(p
0
+
p)
r
ho
3
(p
0
;
p)
=
i
2k
2
1
k
2
4m
2
`
5
(p
0
+
p)
:
(2.15)
F
or
k
!
0,
one
has
2
(p;
p
0
)
=
1
4k
2
h
1
m
`
1
+
k
2
m
2
`
(p
+
1
2
k
)
+
i
;
(2.16)
and
(6
p
+
m
`
)
2
(p;
p
0
)(6
p
0
+
m
`
)
=
1
4
(6
p
+
m
`
)
h
k
k
2
+
(
p
m
`
)
6
k
k
2
+
i
:
(2.17)
The
last
expression
b
eha
v
es
as
1=k
as
the
external
photon
four
momen
tum
k
v
anishes,
so
that
one
ma
y
w
orry
ab
out
the
niteness
of
F
2
(0)
obtained
up
on
using
Eq.
(2.14).
This
problem
is
solv
ed
b
y
the
fat
that
(p
0
;
p)
satises
the
W
ard
iden
tit
y
(p
0
p)
(p
0
;
p)
=
0
;
(2.18)
follo
wing
from
the
onserv
ation
of
the
eletromagneti
urren
t.
Therefore,
the
iden
tit
y
(p
0
;
p)
=
k
k
(p
0
;
p)
(2.19)
pro
vides
the
additional
p
o
w
er
of
k
whi
h
ensures
a
nite
result
as
k
!
0.
The
presene
of
three
dieren
t
in
terations
in
the
standard
mo
del
naturally
leads
one
to
onsider
the
follo
wing
deomp
osition
of
the
anomalous
magneti
momen
t
a
`
:
a
`
=
a
QED
`
+
a
had
`
+
a
w
eak
`
:
(2.20)
By
a
QED
`
,
I
denote
all
the
on
tributions
whi
h
arise
from
lo
ops
in
v
olving
only
virtual
photons
and
leptons.
Among
these,
it
is
useful
to
distinguish
those
whi
h
in
v
olv
e
only
the
same
lepton
a
v
our
`
for
whi
h
w
e
wish
to
ompute
the
anomalous
magneti
momen
t,
and
those
whi
h
in
v
olv
e
lo
ops
with
leptons
of
dieren
t
a
v
ours,
denoted
olletiv
ely
as
`
0
[
e
2
=4
â„„,
a
QED
`
=
X
n1
A
n
n
+
X
n2
B
n
(`;
`
0
)
n
:
(2.21)
The
seond
t
yp
e
of
on
tribution,
a
had
`
in
v
olv
es
also
quark
lo
ops.
Their
on
tribution
is
far
from
b
eing
limited
to
the
short
distane
sales,
and
a
had
`
is
an
in
trinsially
non
p
erturbativ
e
quan
tit
y
.
F
rom
a
theoretial
p
oin
t
of
view,
this
represen
ts
a
serious
diÆult
y
.
Finally
,
at
some
lev
el
of
preision,
the
w
eak
in
terations
an
no
longer
b
e
ignored,
and
on
tributions
of
virtual
Higgs
or
massiv
e
gauge
b
oson
degrees
of
freedom
indue
the
third
omp
onen
t
a
w
eak
`
.
Of
ourse,
starting
from
the
t
w
o
lo
op
lev
el,
a
hadroni
on
tribution
to
a
w
eak
`
will
also
b
e
presen
t.
The
remaining
of
this
presen
tation
is
dev
oted
to
a
detailed
disussion
of
these
v
arious
on
tributions.
Before
starting
this
guided
tour
of
the
anomalous
magneti
momen
ts
of
the
massiv
e
harged
leptons
of
the
standard
mo
del,
it
is
useful
to
k
eep
in
mind
a
few
simple
and
elemen
tary
onsiderations:
The
anomalous
magneti
momen
t
is
a
dimensionless
quan
tit
y
.
Therefore,
the
o
eÆien
ts
A
n
ab
o
v
e
are
universal,
i.e.
they
do
not
dep
end
on
the
a
v
our
of
the
lepton
whose
anomalous
magneti
momen
t
w
e
wish
to
ev
aluate.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
97
The
on
tributions
to
a
`
of
degrees
of
freedom
orresp
onding
to
a
t
ypial
sale
M
m
`
deouple
[12
â„„,
i.e.
they
are
suppr
esse
d
b
y
p
o
w
ers
of
m
`
=
M
.
5
The
on
tributions
to
a
`
originating
from
ligh
t
degrees
of
freedom,
haraterized
b
y
a
t
ypial
sale
m
m
`
are
enhan
e
d
b
y
p
o
w
ers
of
ln(m
`
=m).
A
t
a
giv
en
order,
the
logarithmi
terms
that
do
not
v
anish
as
m
`
=m
!
0
an
often
b
e
omputed
from
the
kno
wledge
of
the
lesser
order
terms
and
of
the
funtion
through
the
renormalization
group
equations
[15
,
16
,
17
,
18
â„„.
These
general
prop
erties
already
allo
w
to
dra
w
a
few
elemen
tary
onlusions.
The
eletron
b
eing
the
ligh
test
harged
lepton,
its
anomalous
magneti
momen
t
is
dominan
tly
determined
b
y
the
v
alues
of
the
o
eÆien
ts
A
n
.
The
rst
on
tribution
of
other
degrees
of
freedom
omes
from
graphs
in
v
olving,
sa
y
,
at
least
one
m
uon
lo
op,
whi
h
o
urs
rst
at
the
t
w
o-lo
op
lev
el,
and
is
of
the
order
of
(m
2
e
=m
)
2
(=
)
2
10
10
.
The
hadroni
eets,
i.e.
\quark
and
gluon
lo
ops",
haraterized
b
y
a
sale
of
1
GeV,
or
eets
of
degrees
of
freedom
b
ey
ond
the
standard
mo
del,
whi
h
ma
y
app
ear
at
some
high
sale
M
,
will
b
e
felt
more
strongly
,
b
y
a
onsiderable
fator
(m
=m
e
)
2
40
000,
in
a
than
in
a
e
.
Th
us,
a
e
is
w
ell
suited
for
testing
the
v
alidit
y
of
QED
at
higher
orders,
whereas
a
is
more
appropriate
for
deteting
new
ph
ysis.
If
w
e
follo
w
this
line
reasoning,
a
w
ould
ev
en
b
e
b
etter
suited
for
nding
evidene
of
degrees
of
freedom
b
ey
ond
the
standard
mo
del.
Unfortunately
,
the
v
ery
short
lifetime
of
the
lepton
[
3
10
13
sâ„„
mak
es
a
suÆien
tly
aurate
measuremen
t
of
a
imp
ossible
at
presen
t.
3
Brief
o
v
erview
of
the
exp
erimen
tal
situation
3.1
Measuremen
ts
of
the
magneti
momen
t
of
the
eletron
The
rst
indiation
that
the
gyromagneti
fator
of
the
eletron
is
dieren
t
from
the
v
alue
g
e
=
2
predited
b
y
the
Dira
theory
ame
from
the
preision
measuremen
t
of
h
yp
erne
splitting
in
h
ydrogen
and
deuterium
[19
â„„.
The
rst
measuremen
t
of
the
gyromagneti
fator
of
free
eletrons
w
as
p
erformed
in
1958
[20
â„„,
with
a
preision
of
3.6%.
The
situation
b
egan
to
impro
v
e
with
the
in
tro
dution
of
exp
erimen
tal
setups
based
on
the
P
enning
trap.
Some
of
the
suessiv
e
v
alues
obtained
o
v
er
a
p
erio
d
of
fort
y
y
ears
are
sho
wn
in
T
able
1.
T
e
hnial
impro
v
emen
ts,
ev
en
tually
allo
wing
for
the
trapping
of
a
single
eletron
or
p
ositron,
pro
dued,
in
the
ourse
of
time,
an
enormous
inrease
in
preision
whi
h,
starting
from
a
few
p
eren
ts,
w
en
t
through
the
ppm
[parts
p
er
millionâ„„
lev
els,
b
efore
ulminating
at
4
ppb
[parts
p
er
billionâ„„
[21
â„„
in
the
last
of
a
series
of
exp
erimen
ts
p
erformed
at
the
Univ
ersit
y
of
W
ashington
in
Seattle.
The
same
exp
erimen
t
has
also
pro
dued
a
measuremen
t
of
the
magneti
momen
t
of
the
p
ositron
with
the
same
auray
,
th
us
pro
viding
a
test
of
C
P
T
in
v
ariane
at
the
lev
el
of
10
12
,
g
e
=g
e
+
=
1
+
(0:5
2:1)
10
12
:
(3.1)
An
extensiv
e
surv
ey
of
the
literature
and
a
detailed
desription
of
the
v
arious
exp
erimen
tal
asp
ets
an
b
e
found
in
[22
â„„.
The
earlier
exp
erimen
ts
are
review
ed
in
[23
â„„.
3.2
Measuremen
ts
of
the
magneti
momen
t
of
the
m
uon
The
anomalous
magneti
momen
t
of
the
m
uon
has
also
b
een
the
sub
jet
of
quite
a
few
exp
erimen
ts.
The
v
ery
short
lifetime
of
the
m
uon,
=
(2:19703
0:00004
)
10
6
s,
mak
es
it
neessary
to
pro
eed
in
a
ompletely
dieren
t
w
a
y
in
order
to
attain
a
high
preision.
The
exp
erimen
ts
onduted
at
CERN
during
the
y
ears
1968-1977
used
a
m
uon
storage
ring
[for
details,
see
[31
â„„
and
referenes
quoted
thereinâ„„.
The
more
reen
t
exp
erimen
ts
at
the
A
GS
in
Bro
okha
v
en
are
based
on
the
same
5
In
the
presene
of
the
w
eak
in
terations,
this
statemen
t
has
to
b
e
reonsidered,
sine
the
neessit
y
for
the
anellation
of
the
S
U
(2)
U
(1)
gauge
anomalies
transforms
the
deoupling
of,
sa
y
,
a
single
hea
vy
fermion
in
a
giv
en
generation,
in
to
a
somewhat
subtle
issue
[13,
14 â„„.
98
M.
Kne
h
t
S
eminaire
P
oinar
e
T
able
1:
Some
exp
erimen
tal
determinations
of
the
eletron's
anomalous
magneti
momen
t
a
e
with
the
orresp
onding
relativ
e
preision.
0.001
19(5)
4.2%
[24
â„„
0.001
165(11)
1%
[25
â„„
0.001
116(40)
3.6%
[20
â„„
0.001
160
9(2
4)
2
100
ppm
[26
â„„
0.001
159
622(27)
23
ppm
[27
â„„
0.001
159
660(300)
258
ppm
[28
â„„
0.001
159
657
7(3
5)
3
ppm
[29
â„„
0.001
159
652
41(20)
172
ppb
[30
â„„
0.001
159
652
188
4(4
3)
4
ppb
[21
â„„
onept.
Pions
are
pro
dued
b
y
sending
a
proton
b
eam
on
a
target.
The
pions
subsequen
tly
dea
y
in
to
longitudinally
p
olarized
m
uons,
whi
h
are
aptured
inside
a
storage
ring,
where
they
follo
w
a
irular
orbit
in
the
presene
of
b
oth
a
uniform
magneti
eld
and
a
quadrup
ole
eletri
eld,
the
latter
serving
the
purp
ose
of
fo
using
the
m
uon
b
eam.
The
dierene
b
et
w
een
the
spin
preession
frequeny
and
the
orbit,
or
syn
hrotron,
frequeny
is
giv
en
b
y
!
s
!
=
e
m
a
B
a
1
1
2
^
E
:
(3.2)
Therefore,
if
the
Loren
tz
fator
is
tuned
to
its
\magi"
v
alue
=
p
1
+
1=a
=
29:3,
the
measuremen
t
of
!
s
!
and
of
the
magneti
eld
B
allo
ws
to
determine
a
.
The
spin
diretion
of
the
m
uon
is
determined
b
y
deteting
the
eletrons
or
p
ositrons
pro
dued
in
the
dea
y
of
the
m
uons
with
an
energy
greater
than
some
threshold
energy
E
t
.
The
n
um
b
er
of
eletrons
deteted
dereases
exp
onen
tially
in
time,
with
a
time
onstan
t
set
b
y
the
m
uon's
lifetime,
and
is
mo
dulated
b
y
the
frequeny
!
s
!
,
N
e
(t)
=
N
0
e
t=
f1
+
A
os
[(!
s
!
)t
+
â„„g
:
(3.3)
T
able
2:
Determinations
of
the
anomalous
magneti
momen
t
of
the
p
ositiv
ely
harged
m
uon
from
the
storage
ring
exp
erimen
ts
onduted
at
the
CERN
PS
and
at
the
BNL
A
GS.
0.001
166
16(31)
265
ppm
[32
â„„
0.001
165
895(27)
23
ppm
[33
â„„
0.001
165
911(11)
10
ppm
[34
â„„
0.001
165
925(15)
13
ppm
[35
â„„
0.001
165
9191(59)
5
ppm
[36
â„„
0.001
165
920
2(16)
1.3
ppm
[37
â„„
0.001
165
920
3(8)
0.7
ppm
[38
â„„
Sev
eral
exp
erimen
tal
results
for
the
anomalous
magneti
momen
t
of
the
p
ositiv
ely
harged
m
uon,
obtained
at
the
CERN
PS
or,
more
reen
tly
,
at
the
BNL
A
GS,
are
reorded
in
T
able
2.
Notie
that
the
relativ
e
errors
are
measured
in
ppm
units,
to
b
e
on
trasted
with
the
ppb
lev
el
of
auray
a
hiev
ed
in
the
eletron
ase.
The
four
last
v
alues
in
T
able
2
w
ere
obtained
b
y
the
E821
exp
erimen
t
at
BNL.
They
sho
w
a
remark
able
stabilit
y
and
a
steady
inrease
in
preision,
and
no
w
ompletely
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
99
dominate
the
w
orld
a
v
erage
v
alue.
F
urther
data,
for
negativ
ely
harged
m
uons
6
are
presen
tly
b
eing
analyzed.
The
aim
of
the
Bro
okha
v
en
Muon
(g
-
2)
Collab
oration
is
to
rea
h
a
preision
of
0.35
ppm,
but
this
will
dep
end
on
whether
the
exp
erimen
t
will
reeiv
e
nanial
supp
ort
to
ollet
more
data
or
not.
3.3
Exp
erimen
tal
b
ounds
on
the
anomalous
magneti
momen
t
of
the
lepton
As
already
men
tioned,
the
v
ery
short
lifetime
of
the
preludes
a
measuremen
t
of
its
anomalous
magneti
momen
t
follo
wing
an
y
of
the
te
hniques
desrib
ed
ab
o
v
e.
Indiret
aess
to
a
is
pro
vided
b
y
the
reation
e
+
e
!
+
.
The
results
obtained
b
y
OP
AL
[39
â„„
and
L3
[40
â„„
at
LEP
only
pro
vide
v
ery
lo
ose
b
ounds,
0:052
<
a
<
0:058
(95%C :L:)
0:068
<
a
<
0:065
(95%C :L:)
;
(3.4)
resp
etiv
ely
.
W
e
shall
no
w
turn
to
w
ards
theory
,
in
order
to
see
ho
w
the
standard
mo
del
preditions
ompare
with
these
exp
erimen
tal
v
alues.
Only
the
ases
of
the
eletron
and
of
the
m
uon
will
b
e
treated
in
some
detail.
The
theoretial
asp
ets
as
far
as
the
anomalous
magneti
momen
t
of
the
are
onerned
are
disussed
in
[41
â„„.
4
The
anomalous
magneti
momen
t
of
the
eletron
W
e
start
with
the
anomalous
magneti
momen
t
of
the
ligh
test
harged
lepton,
the
eletron.
Sine
the
eletron
mass
m
e
is
m
u
h
smaller
than
an
y
other
mass
sale
presen
t
in
the
standard
mo
del,
the
mass
indep
enden
t
part
of
a
QED
e
dominates
its
v
alue.
As
men
tioned
b
efore,
non
v
anishing
on
tributions
app
ear
at
the
lev
el
of
the
lo
op
diagrams
sho
wn
in
Fig.
1.
=
+
+
+ ...
QED
Figure
1:
The
p
erturbativ
e
expansion
of
(p
0
;
p)
in
single
a
v
our
QED.
The
tree
graph
giv
es
F
1
=
1,
F
2
=
F
3
=
0.
The
one
lo
op
v
ertex
orretion
graph
giv
es
the
o
eÆien
t
A
1
in
Eq.
(2.21).
The
ross
denotes
the
insertion
of
the
external
eld.
4.1
The
lo
w
est
order
on
tribution
The
one
lo
op
diagram
giv
es
(p
0
;
p)
1
lo
op
=
(
ie)
2
Z
d
4
q
(2
)
4
(6
p
0
+
6
q
+
m
e
)
(6
p+
6
q
+
m
e
)
i
(p
0
+
q
)
2
m
2
e
i
(p
+
q
)
2
m
2
e
(
i)
q
2
:
(4.1)
6
The
CERN
exp
erimen
t
had
also
measured
a
=
0:001
165
937(12)
with
a
10
ppm
auray
,
giving
the
a
v
erage
v
alue
a
=
0:001
165
924(8:5),
with
an
auray
of
7
ppm.
100
M.
Kne
h
t
S
eminaire
P
oinar
e
The
form
fator
F
2
(k
2
)
is
obtained
b
y
using
Eqs.
(2.14)
and
(2.15)
and,
up
on
ev
aluating
the
orresp
onding
trae
of
Dira
matries,
one
nds
F
2
(k
2
)
1
lo
op
=
ie
2
32m
2
e
k
2
(k
2
4m
2
e
)
2
Z
d
4
q
(2
)
4
1
(p
0
+
q
)
2
m
2
e
1
(p
+
q
)
2
m
2
e
1
q
2
3k
2
(p
q
)
2
+
2k
2
m
2
e
(p
q
)
+
k
2
m
2
e
q
2
m
2
e
(k
q
)
2
:
(4.2)
Then
follo
w
the
usual
steps
of
in
tro
duing
t
w
o
F
eynman
parameters,
of
p
erforming
a
trivial
hange
of
v
ariables
and
a
symmetri
in
tegration
o
v
er
the
lo
op
momen
tum
q
,
so
that
one
arriv
es
at
F
2
(k
2
)
1
lo
op
=
ie
2
64m
2
e
(k
2
4m
2
e
)
2
Z
1
0
dxx
Z
1
0
dy
Z
d
4
q
(2
)
4
1
(q
2
R
2
)
3
2x(1
x)m
4
e
3
4
x
2
y
2
(k
2
)
2
+
m
2
e
k
2
x
3xy
y
+
1
2
x
=
e
2
2
2m
2
e
(k
2
4m
2
e
)
2
Z
1
0
dxx
Z
1
0
dy
1
R
2
2x(1
x)m
4
e
3
4
x
2
y
2
(k
2
)
2
+
m
2
e
k
2
x
3xy
y
+
1
2
x
;
(4.3)
with
R
2
=
x
2
y
(1
y
)(2m
2
e
k
2
)
+
x
2
y
2
m
2
e
+
x
2
(1
y
)
2
m
2
e
:
(4.4)
As
exp
eted,
the
limit
k
2
!
0
an
b
e
tak
en
without
problem,
and
giv
es
a
e
j
1
lo
op
F
2
(0)
1
lo
op
=
1
2
:
(4.5)
Let
us
stress
that
although
the
in
tegral
(4.1)
div
erges,
w
e
ha
v
e
obtained
a
nite
result
for
F
2
(k
2
),
and
hene
for
a
e
,
without
in
tro
duing
an
y
regularization.
This
is
of
ourse
exp
eted,
sine
a
di-
v
ergene
in,
sa
y
,
F
2
(0)
w
ould
require
that
a
oun
terterm
of
the
form
giv
en
b
y
the
seond
term
in
b
L
in
t
,
see
Eq.
(2.8),
b
e
in
tro
dued.
This
w
ould
in
turn
sp
oil
the
renormalizabilit
y
of
the
theory
.
In
fat,
as
is
w
ell
kno
wn,
the
div
ergene
lies
in
F
1
(0),
and
is
absorb
ed
in
to
the
renormalization
of
the
eletron's
harge.
+
sym
+
sym
Figure
2:
The
F
eynman
diagrams
whi
h
on
tribute
to
the
o
eÆien
t
A
2
in
Eq.
(2.21).
4.2
Higher
order
mass
indep
enden
t
orretions
The
previous
alulation
is
rather
straigh
tforw
ard
and
amoun
ts
to
the
result
A
1
=
1
2
(4.6)
rst
obtained
b
y
S
h
winger
[42
â„„.
S
h
winger's
alulation
w
as
so
on
follo
w
ed
b
y
a
omputation
of
A
2
[43
â„„,
whi
h
requires
the
ev
aluation
of
7
graphs,
represen
ting
v
e
distint
top
ologies,
and
sho
wn
in
Fig.
2.
Historially
,
the
result
of
Ref.
[43
â„„
w
as
imp
ortan
t,
b
eause
it
pro
vided
the
rst
expliit
example
of
the
realization
of
the
renormalization
program
of
QED
at
t
w
o
lo
ops.
Ho
w
ev
er,
the
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
101
v
alue
for
A
2
w
as
not
giv
en
orretly
.
The
orret
expression
of
the
seond
order
mass
indep
enden
t
on
tribution
w
as
deriv
ed
in
[44
,
45
,
46
â„„
(see
also
[47
,
48
â„„)
and
reads
7
A
2
=
197
144
+
1
2
3
ln
2
(2)
+
3
4
(3)
=
0:328
478
965:::
(4.7)
with
(p)
=
1
X
n=1
1=n
p
,
(2)
=
2
=6.
The
o
urrene
of
transenden
tal
n
um
b
ers
lik
e
zeta
funtions
or
p
olylogarithms
is
a
general
feature
of
higher
order
alulations
in
p
erturbativ
e
quan
tum
eld
theory
.
The
pattern
of
these
transenden
tals
in
p
erturbation
theory
has
also
b
een
put
in
relationship
with
other
mathematial
strutures,
lik
e
knot
theory
.
The
analyti
ev
aluation
of
the
three-lo
op
mass
indep
enden
t
on
tribution
to
the
anomalous
magneti
momen
t
required
quite
some
time,
and
is
mainly
due
to
the
dediation
of
E.
Remiddi
and
his
o
w
ork
ers
during
the
p
erio
d
1969-1996.
There
are
no
w
72
diagrams
to
onsider,
in
v
olving
man
y
dieren
t
top
ologies,
see
Fig.
3.
6
20
12
24
4
6
Figure
3:
The
72
F
eynman
diagrams
whi
h
mak
e
up
the
o
eÆien
t
A
3
in
Eq.
(2.21).
The
alulation
w
as
ompleted
[49
â„„
in
1996,
with
the
analytial
ev
aluation
of
a
last
lass
of
diagrams,
the
non
planar
\triple
ross"
top
ologies.
The
result
reads
8
A
3
=
87
72
2
(3)
215
24
(5)
+
100
3
a
4
+
1
24
ln
4
2
1
24
2
ln
2
2
239
2160
4
+
139
18
(3)
298
9
2
ln
2
+
17101
810
2
+
28259
5184
=
1:181
241
456:::
(4.8)
7
Atually
,
the
exp
erimen
tal
result
of
Ref.
[25â„„
disagreed
with
the
v
alue
A
2
=
2:973
obtained
in
[43â„„,
and
prompted
theoretiians
to
reonsider
the
alulation.
The
result
obtained
b
y
the
authors
of
Refs.
[44,
45,
46 â„„
reoniled
theory
with
exp
erimen
t.
8
The
ompletion
of
this
three-lo
op
program
an
b
e
follo
w
ed
through
Refs.
[50â„„-[55â„„
and
[49 â„„.
A
desription
of
the
te
hnial
asp
ets
related
to
this
w
ork
and
an
aoun
t
of
its
status
up
to
1990,
with
referenes
to
the
orresp
onding
literature,
are
giv
en
in
Ref.
[56â„„.
102
M.
Kne
h
t
S
eminaire
P
oinar
e
where
9
a
p
=
1
X
n=1
1
2
n
n
p
.
The
n
umerial
v
alue
extrated
from
the
exat
analytial
expression
giv
en
ab
o
v
e
an
b
e
impro
v
ed
to
an
y
desired
order
of
preision.
In
parallel
to
these
analytial
alulations,
n
umerial
metho
ds
for
the
ev
aluation
of
the
higher
order
on
tributions
w
ere
also
dev
elop
ed,
in
partiular
b
y
Kinoshita
and
his
ollab
orators
(for
details,
see
[57
â„„).
The
n
umerial
ev
aluation
of
the
full
set
of
three
lo
op
diagrams
w
as
a
hiev
ed
in
sev
eral
steps
[58
â„„-[64
â„„.
The
v
alue
quoted
in
[64
â„„
is
A
3
=
1:195(26),
where
the
error
omes
from
the
n
umerial
pro
edure.
In
omparison,
let
us
quote
the
v
alue
[65
,
57
â„„
A
3
=
1:176
11
(42)
obtained
if
only
a
subset
of
21
three
lo
op
diagrams
out
of
the
original
set
of
72
is
ev
aluated
n
umerially
,
relying
on
the
analytial
results
for
the
remaining
51
ones,
and
reall
the
v
alue
A
3
=
1:181
241
456:::
obtained
from
the
full
analytial
ev
aluation.
The
error
indued
on
a
e
due
to
the
n
umerial
unertain
t
y
in
the
seond,
more
aurate,
v
alue
is
still
(a
e
)
=
5:3
10
12
,
whereas
the
exp
erimen
tal
error
is
only
(a
e
)j
exp
=
4:3
10
12
.
This
disussion
sho
ws
that
the
analytial
ev
aluations
of
higher
lo
op
on
tributions
to
the
anomalous
magneti
momen
t
of
the
eletron
ha
v
e
a
strong
pratial
in
terest
as
far
as
the
preision
of
the
theoretial
predition
is
onerned,
and
whi
h
go
es
w
ell
b
ey
ond
the
mere
in
telletual
satisfation
and
te
hnial
skills
in
v
olv
ed
in
these
alulations.
10
A
t
the
four
lo
op
lev
el,
there
are
891
diagrams
to
onsider.
Clearly
,
only
a
few
of
them
ha
v
e
b
een
ev
aluated
analytially
[66
,
67
â„„.
The
omplete
n
umerial
ev
aluation
of
the
whole
set
ga
v
e
[65
â„„
A
4
=
1:434(138).
The
dev
elopmen
t
of
omputers
allo
w
ed
subsequen
t
reanalyzes
to
b
e
more
aurate,
i.e.
A
4
=
1:557(70)
[68
â„„,
while
the
\latest
of
[theseâ„„
onstan
tly
impro
ving
v
alues"
is
[4â„„
A
4
=
1:509
8(38
4)
:
(4.9)
Needless
to
sa
y
,
so
far
the
v
e
lo
op
on
tribution
A
5
is
unkno
wn
territory
.
On
the
other
hand,
(=
)
5
7
10
14
,
so
that
one
ma
y
reasonably
exp
et
that,
in
view
of
the
presen
t
exp
erimen
tal
situation,
its
kno
wledge
is
not
y
et
required.
4.3
Mass
dep
enden
t
QED
orretions
W
e
no
w
turn
to
the
QED
lo
op
on
tributions
to
the
eletron's
anomalous
magneti
momen
t
in-
v
olving
the
hea
vier
leptons,
and
.
The
lo
w
est
order
on
tribution
of
this
t
yp
e
o
urs
at
the
t
w
o
lo
op
lev
el,
O
(
2
),
and
orresp
onds
to
a
hea
vy
lepton
v
auum
p
olarization
insertion
in
the
one
lo
op
v
ertex
graph,
f.
Fig.
4.
Quite
generally
,
the
on
tribution
to
a
`
arising
from
the
insertion,
in
to
the
one
lo
op
v
ertex
orretion,
of
a
v
auum
p
olarization
graph
due
to
a
lo
op
of
lepton
`
0
,
reads
[69
,
70
â„„
11
B
2
(`;
`
0
)
=
1
3
Z
1
4m
2
`
0
dt
r
1
4m
2
`
0
t
t
+
2m
2
`
0
t
2
Z
1
0
dx
x
2
(1
x)
x
2
+
(1
x)
t
m
2
`
:
(4.10)
If
m
`
0
m
`
,
the
seond
in
tegrand
an
b
e
appro
ximated
b
y
x
2
m
2
`
=t,
and
one
obtains
[72
â„„
B
2
(`;
`
0
)
=
1
45
m
`
m
`
0
2
+
O
"
m
`
m
`
0
3
#
;
m
`
0
m
`
:
(4.11)
9
The
rst
three
v
alues
are
kno
wn
to
b
e
a
1
=
ln
2,
a
2
=
Li
2
(1=2)
=
(
(2)
ln
2
2)=2,
a
3
=
7
8
(3)
1
2
(2)
ln
2
+
1
6
ln
3
2
[56â„„.
10
It
is
only
fair
to
p
oin
t
out
that
the
n
umerial
v
alues
that
are
quoted
here
orresp
ond
to
those
giv
en
in
the
original
referenes.
It
is
to
b
e
exp
eted
that
they
w
ould
impro
v
e
if
to
da
y's
n
umerial
p
ossibilities
w
ere
used.
11
A
trivial
hange
of
v
ariable
on
t
brings
the
expression
(4.10)
in
to
the
form
giv
en
in
[69,
70â„„.
F
urthermore,
the
analytial
result
obtained
up
on
p
erforming
the
double
in
tegration
is
a
v
ailable
in
[71 â„„.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
103
e
e
µ
e
µ
µ
Figure
4:
The
insertion
of
a
m
uon
v
auum
p
olarization
lo
op
in
to
the
eletron
v
ertex
orretion
(left)
or
of
an
eletron
v
auum
p
olarization
lo
op
in
to
the
m
uon
v
ertex
orretion
(righ
t).
Numerially
,
this
translates
in
to
[3
â„„
[m
e
=
0:51099907(15)
MeV,
m
=m
e
=
206:768273(24),
m
=
1
777:05(26)â„„
B
2
(e;
)
=
5:197
10
7
B
2
(e;
)
=
1:838
10
9
:
(4.12)
F
or
later
use,
it
is
in
teresting
to
briey
disuss
the
struture
of
Eq.
(4.10).
The
quan
tit
y
whi
h
app
ears
under
the
in
tegral
is
related
to
the
ross
setion
for
the
sattering
of
a
`
+
`
pair
in
to
a
pair
(`
0
)
+
(`
0
)
at
lowest
or
der
in
QED,
(`
+
`
!(`
0
)
+
(`
0
)
)
QE
D
(s)
=
4
2
3s
2
r
1
4m
2
`
0
s
(s
+
2m
2
`
0
)
;
(4.13)
so
that
B
2
(`;
`
0
)
=
1
3
Z
1
4m
2
`
0
dtK
(t)R
(`
0
)
(t)
;
(4.14)
where
K
(t)
=
Z
1
0
dx
x
2
(1
x)
x
2
+
(1
x)
t
m
2
`
;
(4.15)
and
R
(`
0
)
(t)
is
the
lowest
or
der
QED
ross
setion
(`
+
`
!(`
0
)
+
(`
0
)
)
Q E
D
(s)
divided
b
y
the
asymptoti
form
of
the
ross
setion
of
the
reation
e
+
e
!
+
for
s
m
2
,
(e
+
e
!
+
)
1
(s)
=
4
2
3s
.
The
three
lo
op
on
tributions
with
dieren
t
lepton
a
v
ours
in
the
lo
ops
are
also
kno
wn
analytially
[73
,
74
â„„.
It
is
on
v
enien
t
to
distinguish
three
lasses
of
diagrams.
The
rst
group
on
tains
all
the
diagrams
with
one
or
t
w
o
v
auum
p
olarization
insertion
in
v
olving
the
same
lepton,
or
,
of
the
t
yp
e
sho
wn
in
Fig.
5.
The
seond
group
onsists
of
the
leptoni
ligh
t-b
y-ligh
t
sattering
insertion
diagrams,
Fig.
6.
Finally
,
sine
there
are
three
a
v
ours
of
massiv
e
leptons
in
the
standard
mo
del,
one
has
also
the
p
ossibilit
y
of
ha
ving
graphs
with
t
w
o
hea
vy
lepton
v
auum
p
olarization
insertions,
one
made
of
a
m
uon
lo
op,
the
other
of
a
lo
op.
This
giv
es
B
3
(e;
`)
=
B
(v.p.
)
3
(e;
)
+
B
(v.p.)
3
(e;
)
+
B
(LL)
3
(e;
)
+
B
(LL)
3
(e;
)
+
B
(v.p.)
3
(e;
;
)
:
(4.16)
The
analytial
expression
for
B
(v.p.)
3
(e;
)
an
b
e
found
in
Ref.
[73
â„„,
whereas
[74
â„„
giv
es
the
orre-
sp
onding
result
for
B
(LL)
3
(e;
).
F
or
pratial
purp
oses,
it
is
b
oth
suÆien
t
and
more
on
v
enien
t
to
use
their
expansions
in
p
o
w
ers
of
m
e
=m
,
B
(v.p.)
3
(e;
)
=
m
e
m
2
23
135
ln
m
m
e
2
45
2
+
10117
24300
104
M.
Kne
h
t
S
eminaire
P
oinar
e
+
m
e
m
4
19
2520
ln
2
m
m
e
14233
132300
ln
m
m
e
+
49
768
(3)
11
945
2
+
2976691
296352000
+
O
"
m
e
m
6
#
=
0:000
021
768:::
(4.17)
12
6
Figure
5:
Three
lo
op
QED
orretions
with
insertion
of
a
hea
vy
lepton
v
auum
p
olarization
whi
h
mak
e
up
the
o
eÆien
t
B
(v.p.)
3
(e;
).
and
[74â„„
B
(LL)
3
(e;
)
=
m
e
m
2
3
2
(3)
19
16
+
m
e
m
4
161
810
ln
2
m
m
e
16189
48600
ln
m
m
e
+
13
18
(3)
161
9720
2
831931
972000
+
O
"
m
e
m
6
#
=
0:000
014
394
5:::
(4.18)
6
Figure
6:
The
three
lo
op
QED
orretion
with
the
insertion
of
a
hea
vy
lepton
ligh
t-b
y-ligh
t
sat-
tering
subgraph,
orresp
onding
to
the
o
eÆien
t
B
(LL)
3
(e;
).
The
expressions
for
B
(v.p.)
3
(e;
)
and
B
(LL)
3
(e;
)
follo
w
up
on
replaing
the
m
uon
mass
m
b
y
m
.
This
again
giv
es
a
suppression
fator
(m
=m
)
2
,
whi
h
mak
es
these
on
tributions
negligible
at
the
presen
t
lev
el
of
preision.
F
or
the
same
reason,
B
(v.p.)
3
(e;
;
)
an
also
b
e
disarded.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
105
4.4
Other
on
tributions
to
a
e
In
order
to
mak
e
the
disussion
of
the
standard
mo
del
on
tributions
to
a
e
omplete,
there
remains
to
men
tion
the
hadroni
and
w
eak
omp
onen
ts,
a
had
e
and
a
w
eak
e
,
resp
etiv
ely
.
Their
features
will
b
e
disussed
in
detail
b
elo
w,
in
the
on
text
of
the
anomalous
magneti
momen
t
of
the
m
uon.
I
therefore
only
quote
the
n
umerial
v
alues
12
a
had
e
=
1:67(3)
10
12
;
(4.19)
and
[75â„„
a
w
eak
e
=
0:030
10
12
(4.20)
4.5
Comparison
with
exp
erimen
t
and
determination
of
Summing
up
the
v
arious
on
tributions
disussed
so
far
giv
es
the
standard
mo
del
predition
[3
,
4,
7
â„„
a
SM
e
=
0:5
0:328
478
444
00
2
+
1:181
234
017
3
1:509
8(38
4)
4
+
1:70
10
12
:
(4.21)
In
order
to
obtain
a
n
um
b
er
that
an
b
e
ompared
to
the
exp
erimen
tal
result,
a
suÆien
tly
aurate
determination
of
the
ne
struture
onstan
t
is
required.
The
b
est
a
v
ailable
measuremen
t
of
the
latter
omes
from
the
quan
tum
Hall
eet
[76
â„„,
1
(q
H
)
=
137:036
003
00(2
70
)
(4.22)
and
leads
to
a
SM
e
(q
H
)
=
0:001
159
652
153
5(24
0
)
;
(4.23)
ab
out
six
times
less
aurate
than
the
latest
exp
erimen
tal
v
alue
[21
â„„
a
exp
e
=
0:001
159
652
188
4
(4
3)
:
(4.24)
On
the
other
hand,
if
one
exludes
other
on
tributions
to
a
e
than
those
from
the
standard
mo
del
onsidered
so
far,
and
b
eliev
es
that
all
theoretial
errors
are
under
on
trol,
then
the
ab
o
v
e
v
alue
of
a
exp
e
pro
vides
the
b
est
determination
of
to
date,
1
(a
e
)
=
137:035
999
58(52)
:
(4.25)
5
The
anomalous
magneti
momen
t
of
the
m
uon
In
this
setion,
w
e
disuss
the
theoretial
asp
ets
onerning
the
anomalous
magneti
momen
t
of
the
m
uon.
Sine
the
m
uon
is
m
u
h
hea
vier
than
the
eletron,
a
will
b
e
more
sensitiv
e
to
higher
mass
sales.
In
partiular,
it
is
a
b
etter
prob
e
for
p
ossible
degrees
of
freedom
b
ey
ond
the
standard
mo
del,
lik
e
sup
ersymmetry
.
The
dra
wba
k,
ho
w
ev
er,
is
that
a
will
also
b
e
more
sensitiv
e
to
the
non
p
erturbativ
e
strong
in
teration
dynamis
at
the
1
GeV
sale.
12
I
repro
due
here
the
v
alues
giv
en
in
[3,
4â„„,
exept
for
the
fat
that
I
ha
v
e
tak
en
in
to
aoun
t
the
hanges
in
the
v
alue
of
the
hadroni
ligh
t-b
y-ligh
t
on
tribution
to
a
,
see
b
elo
w,
for
whi
h
I
tak
e
a
(LL )
=
+8(4)
10
10
,
and
whi
h
translates
in
to
a
(LL )
e
a
(LL )
(m
e
=m
)
2
=
0:02
10
12
.
106
M.
Kne
h
t
S
eminaire
P
oinar
e
5.1
QED
on
tributions
to
a
As
already
men
tioned
b
efore,
the
mass
indep
enden
t
QED
on
tributions
to
a
are
desrib
ed
b
y
the
same
o
eÆien
ts
A
n
as
in
the
ase
of
the
eletron.
W
e
therefore
need
only
to
disuss
the
o
eÆien
ts
B
n
(;
`
0
)
asso
iated
with
the
mass
dep
enden
t
orretions.
F
or
m
`
0
m
`
,
Eq.
(4.10)
giv
es
[69
,
70
,
71
â„„
B
2
(`;
`
0
)
=
1
3
ln
m
`
m
`
0
25
36
+
3
2
m
`
m
`
0
(2)
4
m
`
m
`
0
2
ln
m
`
m
`
0
+
3
m
`
m
`
0
2
+
O
"
m
`
m
`
0
3
#
;
(5.1)
whi
h
translates
in
to
the
n
umerial
v
alues
[3â„„
B
2
(;
e)
=
1:094
258
294(37)
(5.2)
B
2
(;
)
=
0:00
078
059(23)
:
(5.3)
Although
these
n
um
b
ers
follo
w
from
an
analytial
expression,
there
are
unertain
ties
atta
hed
to
them,
indued
b
y
those
on
the
orresp
onding
v
alues
of
the
ratios
of
the
lepton
masses.
The
three
lo
op
QED
orretions
deomp
ose
as
B
3
(;
`)
=
B
(v.p.
)
3
(;
e)
+
B
(v.p.)
3
(;
)
+
B
(LL)
3
(;
e)
+
B
(LL)
3
(;
)
+
B
(v.p.)
3
(;
e;
)
:
(5.4)
with
[73
,
74
â„„
B
(v.p.
)
3
(;
e)
=
2
9
ln
2
m
m
e
+
(3)
2
3
2
ln
2
+
1
9
2
+
31
27
ln
m
m
e
+
11
216
4
2
9
2
ln
2
2
8
3
a
4
1
9
ln
4
2
3
(3)
+
5
3
2
ln
2
25
18
2
+
1075
216
+
m
e
m
13
18
3
16
9
2
ln
2
+
3199
1080
2
+
m
e
m
2
10
3
ln
2
m
m
e
11
9
ln
m
m
e
14
3
2
ln
2
2
(3)
+
49
12
2
131
54
+
m
e
m
3
4
3
2
ln
m
m
e
+
35
12
3
16
3
2
ln
2
5771
1080
2
+
m
e
m
4
25
9
ln
3
m
m
e
1369
180
ln
2
m
m
e
+[
2
(3)
+
4
2
ln
2
269
144
2
7496
675
â„„
ln
m
m
e
43
108
4
+
8
9
2
ln
2
2
+
80
3
a
4
+
10
9
ln
4
2
411
32
(3)
+
89
48
2
ln
2
1061
864
2
274511
54000
+
O
m
e
m
5
;
(5.5)
B
(LL)
3
(;
e)
=
2
3
2
ln
m
m
e
+
59
270
4
3
(3)
10
3
2
+
2
3
+
m
e
m
4
3
2
ln
m
m
e
196
3
2
ln
2
+
424
9
2
+
m
e
m
2
2
3
ln
3
m
m
e
+
(
2
9
20
3
)
ln
2
m
m
e
[
16
135
4
+
4
(3)
32
9
2
+
61
3
â„„
ln
m
m
e
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
107
+
4
3
(3)
2
61
270
4
+
3
(3)
+
25
18
2
283
12
+
m
e
m
3
10
9
2
ln
m
m
e
11
9
2
+
m
e
m
4
7
9
ln
3
m
m
e
+
41
18
ln
2
m
m
e
+
13
9
2
ln
m
m
e
+
517
108
ln
m
m
e
+
1
2
(3)
+
191
216
2
+
13283
2592
+
O
m
e
m
5
;
(5.6)
while
B
(v.p.
)
3
(;
)
and
B
(LL)
3
(;
)
are
deriv
ed
from
B
(v.p.)
3
(;
)
and
from
B
(LL)
3
(;
),
resp
e-
tiv
ely
,
b
y
trivial
substitutions
of
the
masses.
F
urthermore,
the
graphs
with
mixed
v
auum
p
olar-
ization
insertions,
one
eletron
lo
op,
and
one
lo
op,
are
ev
aluated
n
umerially
using
a
disp
ersiv
e
in
tegral
[51
,
73
,
77
â„„.
Numerially
,
one
obtains
(w
e
quote
here
the
n
umerial
v
alues
up
dated
in
[3â„„)
B
(v.p.)
3
(;
e)
=
1:920
455
1(2)
B
(LL)
3
(;
e)
=
20:947
924
6(7)
B
(v.p.)
3
(;
)
=
0:001
782
2(4)
B
(LL)
3
(;
)
=
0:002
142
8(7)
B
(v.p.)
3
(;
e;
)
=
0:000
527
6(2)
:
(5.7)
Notie
the
large
v
alue
of
B
(LL)
3
(;
e),
due
to
the
o
urrene
of
terms
in
v
olving
fators
lik
e
ln(m
=m
e
)
5
and
p
o
w
ers
of
.
5.2
Hadroni
on
tributions
to
a
On
the
lev
el
of
F
eynman
diagrams,
hadroni
on
tributions
arise
through
lo
ops
of
virtual
quarks
and
gluons.
These
lo
ops
also
in
v
olv
e
the
soft
sales,
and
therefore
annot
b
e
omputed
reliably
in
p
erturbativ
e
QCD.
W
e
shall
deomp
ose
the
hadroni
on
tributions
in
to
three
subsets:
hadroni
v
auum
p
olarization
insertions
at
order
2
,
at
order
3
,
and
hadroni
ligh
t-b
y-ligh
t
sattering,
a
had
=
a
(h.v.p.
1)
+
a
(h.v.p.
2)
+
a
(h.
LL)
(5.8)
5.2.1
Hadroni
v
auum
p
olarization
W
e
rst
disuss
a
(h.v.p.
1)
,
whi
h
arises
at
order
O
(
2
)
from
the
insertion
of
a
single
hadroni
v
auum
p
olarization
in
to
the
lo
w
est
order
v
ertex
orretion
graph,
see
Fig.
7.
The
imp
ortane
of
this
on
tribution
to
a
is
kno
wn
sine
long
time
[78
,
79
â„„.
There
is
a
v
ery
on
v
enien
t
disp
ersiv
e
represen
tation
of
this
diagram,
similar
to
Eq.
(4.10)
a
(h.v.p.
1)
=
Z
1
4M
2
dt
t
K
(t)
1
Im(t)
=
1
3
2
Z
1
4M
2
dt
t
K
(t)R
had
(t)
;
(5.9)
Here,
(t)
denotes
the
hadr
oni
omp
onen
t
of
the
v
auum
p
olarization
funtion,
dened
as
13
(q
q
q
2
)(Q
2
)
=
i
Z
d
4
xe
iq
x
hjTfj
(x)j
(0)gji
;
(5.10)
13
Atually
,
(t)
dened
this
w
a
y
has
an
ultra
violet
div
ergene,
pro
dued
b
y
the
QCD
short
distane
singularit
y
of
the
hronologial
pro
dut
of
the
t
w
o
urren
ts.
Ho
w
ev
er,
it
only
aets
the
real
part
of
(t).
A
renormalized,
nite
quan
tit
y
is
obtained
b
y
a
single
subtration,
(t)
(0).
108
M.
Kne
h
t
S
eminaire
P
oinar
e
H
Figure
7:
The
insertion
of
the
hadroni
v
auum
p
olarization
in
to
the
one
lo
op
v
ertex
orretion,
orresp
onding
to
a
(h.v.p.
1)
.
with
j
the
hadroni
omp
onen
t
of
the
eletromagneti
urren
t,
Q
2
=
q
2
0
for
q
spaelik
e,
and
ji
the
QCD
v
auum.
The
funtion
K
(t)
w
as
dened
in
Eq.
(4.15),
and
R
had
(t)
stands
no
w
for
the
ross
setion
of
e
+
e
!
hadrons
,
at
lowest
or
der
in
,
divided
b
y
(e
+
e
!
+
)
1
(s)
=
4
2
3s
.
A
rst
priniple
omputation
of
this
strong
in
teration
on
tribution
is
far
b
ey
ond
our
presen
t
abilities
to
deal
with
the
non
p
erturbativ
e
asp
ets
of
onning
gauge
theories.
This
last
relation
is
ho
w
ev
er
v
ery
in
teresting
b
eause
it
expresses
a
(h.v.p.
1)
through
a
quan
tit
y
that
an
b
e
measured
exp
erimen
tally
.
In
this
resp
et,
t
w
o
imp
ortan
t
prop
erties
of
the
funtion
K
(t)
deserv
e
to
b
e
men
tioned.
First,
it
app
ears
from
the
in
tegral
represen
tation
(4.15)
that
K
(t)
is
p
ositiv
e
denite.
Sine
R
e
+
e
is
also
p
ositiv
e,
one
dedues
that
a
(h.v.p.
1 )
itself
is
p
ositiv
e.
Seond,
the
funtion
K
(t)
dereases
as
m
2
=3t
as
t
gro
ws,
so
that
it
is
indeed
the
lo
w
energy
region
whi
h
dominates
the
in
tegral.
Expliit
ev
aluation
of
a
(h.v.p.
1)
using
a
v
ailable
data
atually
rev
eals
that
more
than
80%
of
its
v
alue
omes
from
energies
b
elo
w
1.4
GeV.
Finally
,
the
v
alues
obtained
this
w
a
y
for
a
(h.v.p.
1)
ha
v
e
ev
olv
ed
in
time,
as
sho
wn
in
T
able
3.
This
ev
olution
is
mainly
driv
en
b
y
the
a
v
ailabilit
y
of
more
data,
and
is
still
going
on,
as
the
last
en
tries
of
T
able
3
sho
w.
In
order
to
mat
h
the
preision
rea
hed
b
y
the
latest
exp
erimen
tal
measuremen
t
of
a
,
a
(h.v.p.
1)
needs
to
b
e
kno
wn
at
1%.
Besides
the
v
ery
reen
t
high
qualit
y
e
+
e
data
obtained
b
y
the
BES
Collab
oration
[80
â„„
in
the
region
b
et
w
een
2
to
5
GeV,
and
b
y
the
CMD-2
ollab
oration
[81
â„„
in
the
region
dominated
b
y
the
resonane,
the
latest
analyses
sometimes
also
inlude
or
use,
in
the
lo
w-energy
region,
data
obtained
from
hadroni
dea
ys
of
the
b
y
ALEPH
[82
â„„,
and,
more
reen
tly
,
b
y
CLEO
[83
â„„.
W
e
ma
y
notie
from
T
able
3
that
the
preision
obtained
b
y
using
e
+
e
data
alone
has
b
eome
omparable
to
the
one
a
hiev
ed
up
on
inluding
the
data.
Ho
w
ev
er,
one
of
the
latest
analyses
rev
eals
a
troubling
disrepany
b
et
w
een
the
e
+
e
and
ev
aluations.
Additional
w
ork
is
ertainly
needed
in
order
to
resolv
e
these
problems.
F
urther
data
are
also
exp
eted
in
the
future,
from
the
KLOE
exp
erimen
t
at
the
D
APHNE
e
+
e
ma
hine,
or
from
the
B
fatories
BaBar
and
Belle.
F
or
additional
omparativ
e
disussions
and
details
of
the
v
arious
analyses,
w
e
refer
the
reader
to
the
literature
quoted
in
T
able
3.
Let
us
briey
men
tion
here
that
it
is
quite
easy
to
estimate
the
order
of
magnitude
of
a
(h.v.p.
1)
.
F
or
this
purp
ose,
it
is
on
v
enien
t
to
in
tro
due
still
another
represen
tation
[93
â„„,
whi
h
relates
a
(h.v.p.
1)
to
the
hadroni
Adler
funtion
A(Q
2
),
dened
as
14
A(Q
2
)
=
Q
2
(Q
2
)
Q
2
=
Z
1
0
dt
Q
2
(t
+
Q
2
)
2
1
Im (t)
;
(5.11)
b
y
a
(h.v.p.
1)
=
2
2
2
Z
1
0
dx
x
(1
x)(2
x)A
x
2
1
x
m
2
:
(5.12)
14
Unlik
e
(t)
itself,
A(Q
2
)
if
free
from
ultra
violet
div
ergenes.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
109
T
able
3:
Some
of
the
reen
t
ev
aluations
of
a
(h.v.p.
1)
10
11
from
e
+
e
and/or
-dea
y
data.
7024(153)
[84
â„„
e
+
e
7026(160)
[85
â„„
e
+
e
6950(150)
[86
â„„
e
+
e
7011(94)
[86
â„„
,
e
+
e
,
6951(75)
[87
â„„
,
e
+
e
,
QCD
6924(62)
[88
â„„
,
e
+
e
,
QCD
[89
â„„
QCD
sum
rules
7036(76)
[41
â„„
,
e
+
e
,
QCD
7002(73)
[90
â„„
e
+
e
,
F
6974(105)
[91
â„„
e
+
e
,
inl.
BES-I
I
data
6847(70)
[92
â„„
e
+
e
,
inl.
BES-I
I
and
CMD-2
data
7019(62)
[92
â„„
,
e
+
e
6831(62)
[94
â„„
e
+
e
A
simple
represen
tation
of
the
hadroni
Adler
funtion
an
b
e
obtained
if
one
assumes
that
Im(t)
is
giv
en
b
y
a
single,
zero
width,
v
etor
meson
p
ole,
and,
ab
o
v
e
a
ertain
threshold
s
0
,
b
y
the
QCD
p
erturbativ
e
on
tin
uum
on
tribution,
1
Im(t)
=
2
3
f
2
V
M
2
V
Æ
(t
M
2
V
)
+
2
3
N
C
12
2
[1
+
O
(
s
)â„„
(t
s
0
)
(5.13)
The
justiation
[95
â„„
for
this
t
yp
e
of
minimal
hadroni
ansatz
an
b
e
found
within
the
framew
ork
of
the
large-N
C
limit
[96
,
97
â„„
of
QCD,
see
Ref.
[95
â„„
for
a
general
disussion
and
a
detailed
study
of
this
represen
tation
of
the
Adler
funtion.
The
threshold
s
0
for
the
onset
of
the
on
tin
uum
an
b
e
xed
from
the
prop
ert
y
that
there
is
no
on
tribution
in
1=Q
2
in
the
short
distane
expansion
of
A(Q
2
),
whi
h
requires
[95
â„„
2f
2
V
M
2
V
=
N
C
12
2
s
0
1
+
3
8
s
(s
0
)
+
O
(
2
s
)
:
(5.14)
This
then
giv
es
[98
â„„
a
(h.v.p.
1)
(570
170)
10
10
,
whi
h
ompares
w
ell
with
the
more
elab
orate
data
based
ev
aluations
in
T
able
3,
ev
en
though
this
simple
estimate
annot
laim
to
pro
vide
the
required
auray
of
ab
out
1%.
H
H
H
+...
+
Figure
8:
Higher
order
orretions
on
taining
the
hadroni
v
auum
p
olarization
on
tribution,
or-
resp
onding
to
a
(h.v.p.
2)
.
110
M.
Kne
h
t
S
eminaire
P
oinar
e
W
e
no
w
ome
to
the
O
(
3
)
orretions
in
v
olving
hadroni
v
auum
p
olarization
subgraphs.
Besides
the
on
tributions
sho
wn
in
Fig.
8,
another
one
is
obtained
up
on
inserting
a
lepton
lo
op
in
one
of
the
t
w
o
photon
lines
of
the
graph
sho
wn
in
Fig.
7.
These
an
again
b
e
expressed
in
terms
of
R
had
[99
,
2
,
77
â„„
a
(h.v.p.
2)
=
1
3
3
Z
1
4M
2
dt
t
K
(2)
(t)R
had
(t)
:
(5.15)
Unlik
e
K
(t),
the
funtion
K
(2)
(t)
is
not
p
ositiv
e
denite,
so
that
the
sign
of
a
(h.v.p.
2)
is
not
xed
on
the
basis
of
general
onsiderations.
The
v
alue
obtained
for
this
quan
tit
y
is
[77
â„„
a
(h.v.p.
2)
10
11
=
101
6.
5.2.2
Hadroni
ligh
t-b
y-ligh
t
sattering
W
e
no
w
disuss
the
so
alled
hadroni
ligh
t-b
y-ligh
t
sattering
graphs
of
Fig.
9.
Atually
,
there
is
another
O
(
3
)
orretion
in
v
olving
the
amplitude
for
virtual
ligh
t-b
y-ligh
t
sattering,
namely
the
one
obtained
b
y
adding
an
additional
photon
line
atta
hed
to
the
hadroni
blob
in
Fig.
7.
This
on
tribution
is
usually
inluded
in
the
ev
aluations
rep
orted
on
in
T
able
3
[see
the
disussion
in
[92
â„„â„„,
otherwise,
it
has
b
een
added.
The
reason
for
that
is
due
to
the
fat
that
the
measured
e
+
e
data
on
tain
QED
eets,
and
do
not
orresp
ond
to
the
ross
setion
of
e
+
e
!
hadrons
restrited
to
the
lowest
or
der
in
.
It
is
p
ossible
to
ompute
and
subtrat
a
w
a
y
QED
orretions
in
v
olving
the
leptoni
v
ertex,
but
there
still
remain
radiativ
e
orretions
b
et
w
een
the
nal
state
hadrons,
or
whi
h
aet
b
oth
the
initial
and
the
nal
states.
These
annot
b
e
ev
aluated
in
a
mo
del
indep
enden
t
w
a
y
,
and
are
not
ompletely
desrib
ed
b
y
atta
hing
a
photon
lo
op
to
the
hadroni
blob
in
Fig.
7.
H
+
permutations
Figure
9:
The
hadroni
ligh
t-b
y-ligh
t
sattering
graphs
on
tributing
to
a
(h.
LL)
.
Coming
ba
k
to
the
diagram
of
Fig.
9,
the
on
tribution
to
(p
0
;
p)
of
relev
ane
here
is
the
ma-
trix
elemen
t,
at
lo
w
est
non
v
anishing
order
in
the
ne
struture
onstan
t
,
of
the
ligh
t
quark
eletromagneti
urren
t
j
(x)
=
2
3
(
u
u)(x)
1
3
(
d
d)(x)
1
3
(
s
s)(x)
(5.16)
b
et
w
een
states,
(
ie)
u(p
0
)
(h.
LL)
(p
0
;
p)u(p)
h
(p
0
)j(ie)j
(0)j
(p)i
=
Z
d
4
q
1
(2
)
4
Z
d
4
q
2
(2
)
4
(
i)
3
q
2
1
q
2
2
(q
1
+
q
2
k
)
2
i
(p
0
q
1
)
2
m
2
i
(p
0
q
1
q
2
)
2
m
2
(
ie)
3
u(p
0
)
(6
p
0
6
q
1
+
m)
(6
p
0
6
q
1
6
q
2
+
m)
u(p)
(ie)
4
(q
1
;
q
2
;
k
q
1
q
2
)
;
(5.17)
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
111
with
k
=
(p
0
p)
and
(q
1
;
q
2
;
q
3
)
=
Z
d
4
x
1
Z
d
4
x
2
Z
d
4
x
3
e
i(q
1
x
1
+q
2
x
2
+q
3
x
3
)
h
j
T
fj
(x
1
)j
(x
2
)j
(x
3
)j
(0)g
j
i
(5.18)
the
fourth-rank
ligh
t
quark
hadroni
v
auum-p
olarization
tensor,
j
i
denoting
the
QCD
v
auum.
Sine
the
a
v
our
diagonal
urren
t
j
(x)
is
onserv
ed,
the
tensor
(q
1
;
q
2
;
q
3
)
satises
the
W
ard
iden
tities
fq
1
;
q
2
;
q
3
;
(q
1
+
q
2
+
q
3
)
g
(q
1
;
q
2
;
q
3
)
=
0
:
(5.19)
This
en
tails
that
15
u(p
0
)
(h.
LL)
(p
0
;
p)u(p)
=
u (p
0
)
F
(h.
LL)
1
(k
2
)
+
i
2m
k
F
(h.
LL)
2
(k
2
)
u(p)
;
(5.20)
as
w
ell
as
(h.
LL)
(p
0
;
p)
=
k
(h.
LL)
(p
0
;
p)
with
u(p
0
)
(h.
LL)
(p
0
;
p)u(p)
=
ie
6
Z
d
4
q
1
(2
)
4
Z
d
4
q
2
(2
)
4
1
q
2
1
q
2
2
(q
1
+
q
2
k
)
2
1
(p
0
q
1
)
2
m
2
1
(p
0
q
1
q
2
)
2
m
2
u(p
0
)
(6
p
0
6
q
1
+
m)
(6
p
0
6
q
1
6
q
2
+
m)
u(p)
k
(q
1
;
q
2
;
k
q
1
q
2
)
:
(5.21)
F
ollo
wing
Ref.
[58
â„„
and
using
the
prop
ert
y
k
k
u (p
0
)
(h.
LL)
(p
0
;
p)u(p)
=
0,
one
dedues
that
F
(h.
LL)
1
(0)
=
0
and
that
the
hadroni
ligh
t-b
y-ligh
t
on
tribution
to
the
m
uon
anomalous
magneti
momen
t
is
equal
to
a
(h.
LL)
F
(h.
LL )
2
(0)
=
1
48m
tr
n
(6
p
+
m)[
;
â„„(6
p
+
m)
(h.
LL)
(p;
p)
o
:
(5.22)
This
is
ab
out
all
w
e
an
sa
y
ab
out
the
QCD
four-p
oin
t
funtion
(q
1
;
q
2
;
q
3
).
Unlik
e
the
hadroni
v
auum
p
olarization
funtion,
there
is
no
exp
erimen
tal
data
whi
h
w
ould
allo
w
for
an
ev
aluation
of
a
(h.
LL)
.
The
existing
estimates
regarding
this
quan
tit
y
therefore
rely
on
sp
ei
mo
dels
in
order
to
aoun
t
for
the
non
p
erturbativ
e
QCD
asp
ets.
A
few
partiular
on
tributions
an
b
e
iden
tied,
see
Fig.
10.
F
or
instane,
there
is
a
on
tribution
where
the
four
photon
lines
are
atta
hed
to
a
losed
lo
op
of
harged
mesons.
The
ase
of
the
harged
pion
lo
op
with
p
oin
tlik
e
ouplings
is
atually
nite
and
on
tributes
4
10
10
to
a
[100
â„„.
If
the
oupling
of
harged
pions
to
photons
is
mo
died
b
y
taking
in
to
aoun
t
the
eets
of
resonanes
lik
e
the
,
this
on
tribution
is
redued
b
y
a
fator
v
arying
b
et
w
een
3
[100
,
102
â„„
and
10
[101
â„„,
dep
ending
on
the
resonane
mo
del
used.
Another
lass
of
on
tributions
onsists
of
those
in
v
olving
resonane
ex
hanges
b
et
w
een
photon
pairs
[100
,
101
,
102
,
103
â„„.
Although
here
also
the
results
dep
end
on
the
mo
dels
used,
there
is
a
onstan
t
feature
that
emerges
from
all
the
analyses
that
ha
v
e
b
een
done:
the
on
tribution
oming
from
the
ex
hange
of
the
pseudosalars,
0
,
and
0
giv
es
pratially
the
nal
result.
Other
on
tributions
[
harged
pion
lo
ops,
v
etor,
salar,
and
axial
resonanes,...â„„
tend
to
anel
among
themselv
es.
Some
of
the
results
obtained
for
a
(h.
LL)
10
11
ha
v
e
b
een
gathered
in
T
able
4.
Lea
ving
aside
the
rst
result
[99
,
2â„„
sho
wn
there,
whi
h
is
aeted
b
y
a
bad
n
umerial
on
v
ergene
[100
â„„,
one
noties
that
the
sign
of
this
on
tribution
has
hanged
t
wie.
The
rst
hange
resulted
from
a
mistak
e
15
W
e
use
the
follo
wing
on
v
en
tions
for
Dira's
-matries:
f
;
g
=
2
,
with
the
at
Mink
o
wski
spae
metri
of
signature
(+
),
=
(i=2)[
;
â„„,
5
=
i
0
1
2
3
,
whereas
the
totally
an
tisymmetri
tensor
"
is
hosen
su
h
that
"
0123
=
+1.
112
M.
Kne
h
t
S
eminaire
P
oinar
e
H
H
=
Ï€
0
Ï€
3
+
+...
+
Figure
10:
Some
individual
on
tributions
to
hadroni
ligh
t-b
y-ligh
t
sattering:
the
neutral
pion
p
ole
and
the
harged
pion
lo
op.
There
are
other
on
tributions,
not
sho
wn
here.
in
Ref.
[100
â„„,
that
w
as
orreted
for
in
[101
â„„.
The
min
us
sign
that
resulted
w
as
onrmed
b
y
an
indep
enden
t
alulation,
using
the
ENJL
mo
del,
in
Ref.
[102
â„„.
A
subsequen
t
reanalysis
[103
â„„
ga
v
e
additional
supp
ort
to
a
negativ
e
result,
while
also
getting
b
etter
agreemen
t
with
the
v
alue
of
Ref.
[102
â„„.
T
able
4:
V
arious
ev
aluations
of
a
(h.
LL)
10
11
and
of
the
pion
p
ole
on
tribution
a
(h.
LL;
0
)
10
11
.
{260(100)
onstituen
t
quark
lo
op
[99
,
2
â„„
+60(4)
onstituen
t
quark
lo
op
[100
â„„
+49(5)
lo
op,
0
and
resonane
p
oles,
a
(h.
LL;
0
)
=
65(6)
[100
â„„
{52(18)
lo
op,
0
and
resonane
p
oles,
and
quark
lo
op
a
(h.
LL;
0
)
=
55:60(3)
[101
â„„
{92(32)
ENJL,
a
(h.
LL ;
0
+
+
0
)
=
85(13)
[102
â„„
{79.2(15.4)
lo
op,
0
p
ole
and
quark
lo
op,
a
(h.
LL;
0
)
=
55:60(3)
[103
â„„
+83(12)
0
,
and
0
p
oles
only
[104
â„„
+89.6(15.4)
lo
op,
0
p
ole
and
quark
lo
op,
a
(h.
LL;
0
)
=
+55:60(3)
[105
â„„
+83(32)
ENJL,
a
(h.
LL ;
0
+
+
0
)
=
85(13)
[106
â„„
Needless
to
sa
y
,
these
ev
aluations
are
based
on
hea
vy
n
umerial
w
ork,
whi
h
has
the
dra
wba
k
of
making
the
nal
results
rather
opaque
to
an
in
tuitiv
e
understanding
of
the
ph
ysis
b
ehind
them.
W
e
16
therefore
deided
to
impro
v
e
things
on
the
analytial
side,
in
order
to
a
hiev
e
a
b
etter
understanding
of
the
relev
an
t
features
that
led
to
the
previous
results.
T
aking
adv
an
tage
of
the
observ
ation
that
the
pion
p
ole
on
tribution
a
(h.
LL;
0
)
w
as
found
to
dominate
the
nal
v
alues
obtained
for
a
(h.
LL)
,
w
e
onen
trated
our
eorts
on
that
part,
that
I
shall
no
w
desrib
e
in
greater
detail.
F
or
a
detailed
aoun
t
on
ho
w
the
other
on
tributions
to
a
(h.
LL)
arise,
I
refer
the
reader
to
the
original
w
orks
[100
â„„-[103
â„„.
The
on
tributions
to
(q
1
;
q
2
;
q
3
)
arising
from
single
neutral
pion
ex
hanges,
see
Fig.
11,
read
(
0
)
(q
1
;
q
2
;
q
3
)
=
i
F
0
(q
2
1
;
q
2
2
)
F
0
(q
2
3
;
(q
1
+
q
2
+
q
3
)
2
)
(q
1
+
q
2
)
2
M
2
"
q
1
q
2
"
q
3
(q
1
+
q
2
)
+i
F
0
(q
2
1
;
(q
1
+
q
2
+
q
3
)
2
)
F
0
(q
2
2
;
q
2
3
)
(q
2
+
q
3
)
2
M
2
"
q
1
(q
2
+
q
3
)
"
q
2
q
3
16
A.
Nyeler
and
m
yself,
in
Ref.
[104â„„.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
113
+
i
F
0
(q
2
1
;
q
2
3
)
F
0
(q
2
2
;
(q
1
+
q
2
+
q
3
)
2
)
(q
1
+
q
3
)
2
M
2
"
q
1
q
3
"
q
2
(q
1
+
q
3
)
:
(5.23)
Figure
11:
The
pion-p
ole
on
tributions
to
ligh
t-b
y-ligh
t
sattering.
The
shaded
blobs
represen
t
the
form
fator
F
0
.
The
rst
and
seond
graphs
giv
e
rise
to
iden
tial
on
tributions,
in
v
olving
the
funtion
T
1
(q
1
;
q
2
;
p)
in
Eq.
(5.25),
whereas
the
third
graph
giv
es
the
on
tribution
in
v
olving
T
2
(q
1
;
q
2
;
p).
The
form
fator
F
0
(q
2
1
;
q
2
2
),
whi
h
orresp
onds
to
the
shaded
blobs
in
Fig.
11,
is
dened
as
i
Z
d
4
xe
iq
x
h
jT
fj
(x)j
(0)gj
0
(p)i
=
"
q
p
F
0
(q
2
;
(p
q
)
2
)
;
(5.24)
with
F
0
(q
2
1
;
q
2
2
)
=
F
0
(q
2
2
;
q
2
1
).
Inserting
the
expression
(5.23)
in
to
(5.21)
and
omputing
the
orresp
onding
Dira
traes
in
Eq.
(5.22),
w
e
obtain
a
(h.
LL;
0
)
=
e
6
Z
d
4
q
1
(2
)
4
Z
d
4
q
2
(2
)
4
1
q
2
1
q
2
2
(q
1
+
q
2
)
2
[(p
+
q
1
)
2
m
2
â„„[(p
q
2
)
2
m
2
â„„
F
0
(q
2
1
;
(q
1
+
q
2
)
2
)
F
0
(q
2
2
;
0)
q
2
2
M
2
T
1
(q
1
;
q
2
;
p)
+
F
0
(q
2
1
;
q
2
2
)
F
0
((q
1
+
q
2
)
2
;
0)
(q
1
+
q
2
)
2
M
2
T
2
(q
1
;
q
2
;
p)
;
(5.25)
where
T
1
(q
1
;
q
2
;
p)
and
T
2
(q
1
;
q
2
;
p)
denote
t
w
o
p
olynomials
in
the
in
v
arian
ts
p
q
1
,
p
q
2
,
q
1
q
2
.
Their
expressions
an
b
e
found
in
Ref.
[104
â„„.
The
former
arises
from
the
t
w
o
rst
diagrams
sho
wn
in
Fig.
11,
whi
h
giv
e
iden
tial
on
tributions,
while
the
latter
orresp
onds
to
the
third
diagram
on
this
same
gure.
A
t
this
stage,
it
should
also
b
e
p
oin
ted
out
that
the
expression
(5.23)
do
es
not,
stritly
sp
eaking,
represen
t
the
on
tribution
arising
from
the
pion
p
ole
only
.
The
latter
w
ould
require
that
the
n
umerators
in
(5.23)
b
e
ev
aluated
at
the
v
alues
of
the
momen
ta
that
orresp
ond
to
the
p
ole
indiated
b
y
the
orresp
onding
denominators.
F
or
instane,
the
n
umerator
of
the
term
prop
ortional
to
T
1
(q
1
;
q
2
;
p)
in
Eq.
(5.25)
should
rather
read
F
0
(q
2
1
;
(q
2
1
+
2q
1
q
2
+
M
2
)
F
0
(M
2
;
0)
with
q
2
2
=
M
2
.
Ho
w
ev
er,
Eq.
(5.25)
orresp
onds
to
what
previous
authors
ha
v
e
alled
the
pion
p
ole
on
tribution,
and
for
the
sak
e
of
omparison
I
shall
adopt
the
same
denition.
From
here
on,
information
on
the
form
fator
F
0
(q
2
1
;
q
2
2
)
is
required
in
order
to
pro
eed.
The
simplest
mo
del
for
the
form
fator
follo
ws
from
the
W
ess-Zumino-Witten
(WZW)
term
[107
,
108
â„„
that
desrib
es
the
Adler-Bell-Ja
kiw
anomaly
[109
,
110
â„„
in
hiral
p
erturbation
theory
.
Sine
in
this
ase
the
form
fator
is
onstan
t,
one
needs
an
ultra
violet
uto,
at
least
in
the
on
tribution
to
Eq.
(5.25)
in
v
olving
T
1
,
the
one
in
v
olving
T
2
giv
es
a
nite
result
ev
en
for
a
onstan
t
form
fa-
tor
[100
â„„.
Therefore,
this
mo
del
annot
b
e
used
for
a
reliable
estimate,
but
at
b
est
serv
es
only
114
M.
Kne
h
t
S
eminaire
P
oinar
e
illustrativ
e
purp
oses
in
the
presen
t
on
text.
17
Previous
alulations
[100
,
101
,
103
â„„
ha
v
e
also
used
the
usual
v
etor
meson
dominane
form
fator
[see
also
Ref.
[111
â„„â„„.
The
expressions
for
the
form
fator
F
0
based
on
the
ENJL
mo
del
that
ha
v
e
b
een
used
in
Ref.
[102
â„„
do
not
allo
w
a
straigh
t-
forw
ard
analytial
alulation
of
the
lo
op
in
tegrals.
Ho
w
ev
er,
ompared
with
the
results
obtained
in
Refs.
[100
,
101
,
103
â„„,
the
orresp
onding
n
umerial
estimates
are
rather
lose
to
the
VMD
ase
[within
the
error
attributed
to
the
mo
del
dep
endeneâ„„.
Finally
,
represen
tations
of
the
form
fator
F
0
,
based
on
the
large-N
C
appro
ximation
to
QCD
and
that
tak
es
in
to
aoun
t
onstrain
ts
from
hiral
symmetry
at
lo
w
energies,
and
from
the
op
erator
pro
dut
expansion
at
short
distanes,
ha
v
e
b
een
disussed
in
Ref.
[112
â„„
.
They
in
v
olv
e
either
one
v
etor
resonane
[lo
w
est
meson
dom-
inane,
LMDâ„„
or
t
w
o
v
etor
resonanes
(LMD+V),
see
[112
â„„
for
details.
The
four
t
yp
es
of
form
fators
just
men
tioned
an
b
e
written
in
the
form
[F
is
the
pion
dea
y
onstan
tâ„„
F
0
(q
2
1
;
q
2
2
)
=
F
3
f
(q
2
1
)
X
M
V
i
1
q
2
2
M
2
V
i
g
M
V
i
(q
2
1
)
:
(5.26)
F
or
the
VMD
and
LMD
form
fators,
the
sum
in
Eq.
(5.26)
redues
to
a
single
term,
and
the
orresp
onding
funtion
is
denoted
g
M
V
(q
2
).
It
dep
ends
on
the
mass
M
V
of
the
v
etor
resonane,
whi
h
will
b
e
iden
tied
with
the
mass
of
the
meson.
F
or
our
presen
t
purp
oses,
it
is
enough
to
onsider
only
these
t
w
o
last
ases,
along
with
the
onstan
t
WZW
form
fator.
The
orresp
onding
funtions
f
(q
2
)
and
g
M
V
(q
2
)
are
displa
y
ed
in
T
able
5.
T
able
5:
The
funtions
f
(q
2
)
and
g
M
V
(q
2
)
of
Eq.
(5.26)
for
the
dieren
t
form
fators.
N
C
is
the
n
um
b
er
of
olors,
tak
en
equal
to
3,
and
F
=
92:4
MeV
is
the
pion
dea
y
onstan
t.
F
urthermore,
V
=
N
C
4
2
M
4
V
F
2
.
f
(q
2
)
g
M
V
(q
2
)
W
Z
W
N
C
4
2
F
2
0
V
M
D
0
N
C
4
2
F
2
M
4
V
q
2
M
2
V
LM
D
1
q
2
M
2
V
q
2
+
M
2
V
V
q
2
M
2
V
W
e
ma
y
no
w
ome
ba
k
to
Eq.
(5.25).
With
a
represen
tation
of
the
form
(5.26),
the
angular
in
tegrations
an
b
e
p
erformed,
using
for
instane
standard
Gegen
bauer
p
olynomial
te
hniques
(h
yp
erspherial
approa
h),
see
Refs.
[113
,
114
,
56
â„„.
This
leads
to
a
t
w
o-dimensional
in
tegral
repre-
sen
tation:
a
(h.
LL;
0
)
=
3
h
a
(
0
;1)
+
a
(
0
;2)
i
;
(5.27)
a
(
0
;1)
=
Z
1
0
dQ
1
Z
1
0
dQ
2
"
w
f
1
(Q
1
;
Q
2
)
f
(1)
(Q
2
1
;
Q
2
2
)
+
w
g
1
(M
V
;
Q
1
;
Q
2
)
g
(1)
M
V
(Q
2
1
;
Q
2
2
)
#
;
(5.28)
17
In
the
on
text
of
an
eetiv
e
eld
theory
approa
h,
the
pion
p
ole
with
WZW
v
erties
represen
ts
a
hirally
suppressed,
but
large-N
C
dominan
t
on
tribution,
whereas
the
harged
pion
lo
op
is
dominan
t
in
the
hiral
expansion,
but
suppressed
in
the
large-N
C
limit.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
115
a
(
0
;2)
=
Z
1
0
dQ
1
Z
1
0
dQ
2
"
X
M
=M
;M
V
w
g
2
(M
;
Q
1
;
Q
2
)
g
(2)
M
(Q
2
1
;
Q
2
2
)
#
:
(5.29)
The
funtions
f
(1)
(Q
2
1
;
Q
2
2
),
g
(1)
M
V
(Q
2
1
;
Q
2
2
),
g
(2)
M
(Q
2
1
;
Q
2
2
)
and
g
(2)
M
V
(Q
2
1
;
Q
2
2
)
are
expressed
in
terms
of
the
funtions
giv
en
in
T
able
5,
see
Ref.
[104
â„„,
where
the
univ
ersal
[for
the
lass
of
form
fators
that
ha
v
e
a
represen
tation
of
the
t
yp
e
sho
wn
in
Eq.
(5.26)â„„
w
eigh
t
funtions
w
in
Eqs.
(5.28)
and
(5.29)
an
also
b
e
found.
The
latter
are
plotted
in
Fig.
12.
0
0.5
1
1.5
0
0.5
1
1.5
0
2
4
6
Q
1
[GeV]
w
f
1
(Q
1
,Q
2
)
Q
2
[GeV]
0
0.5
1
1.5
0
0.5
1
1.5
0
2
4
6
Q
1
[GeV]
w
g
1
(M
V
,Q
1
,Q
2
)
Q
2
[GeV]
0
1
2
0
1
2
−0.5
0
0.5
1
Q
1
[GeV]
w
g
2
(M
Ï€
,Q
1
,Q
2
)
Q
2
[GeV]
0
1
2
0
1
2
−0.04
−0.02
0
0.02
0.04
0.06
Q
1
[GeV]
w
g
2
(M
V
,Q
1
,Q
2
)
Q
2
[GeV]
Figure
12:
The
w
eigh
t
funtions
app
earing
in
Eqs.
(5.28)
and
(5.29).
Note
the
dieren
t
ranges
of
Q
i
in
the
subplots.
The
funtions
w
f
1
and
w
g
1
are
p
ositiv
e
denite
and
p
eak
ed
in
the
region
Q
1
Q
2
0:5
GeV.
Note,
ho
w
ev
er,
the
tail
in
w
f
1
in
the
Q
1
-diretion
for
Q
2
0:2
GeV.
The
funtions
w
g
2
(M
;
Q
1
;
Q
2
)
and
w
g
2
(M
V
;
Q
1
;
Q
2
)
tak
e
b
oth
signs,
but
their
magnitudes
remain
small
as
ompared
to
w
f
1
(Q
1
;
Q
2
)
and
w
g
1
(M
V
;
Q
1
;
Q
2
).
W
e
ha
v
e
used
M
V
=
M
=
770
MeV.
The
funtions
w
f
1
and
w
g
1
are
p
ositiv
e
and
onen
trated
around
momen
ta
of
the
order
of
0:5
GeV.
This
feature
w
as
already
observ
ed
n
umerially
in
Ref.
[102
â„„
b
y
v
arying
the
upp
er
b
ound
of
the
in
tegrals
[an
analogous
analysis
is
on
tained
in
Ref.
[101
â„„â„„.
Note,
ho
w
ev
er,
the
tail
in
w
f
1
in
the
116
M.
Kne
h
t
S
eminaire
P
oinar
e
Q
1
diretion
for
Q
2
0:2
GeV.
On
the
other
hand,
the
funtion
w
g
2
has
p
ositiv
e
and
negativ
e
on
tributions
in
that
region,
whi
h
will
lead
to
a
strong
anellation
in
the
orresp
onding
in
tegrals,
pro
vided
they
are
m
ultiplied
b
y
a
p
ositiv
e
funtion
omp
osed
of
the
form
fators
[see
the
n
umerial
results
b
elo
wâ„„.
As
an
b
e
seen
from
the
plots,
and
he
k
ed
analytially
,
the
w
eigh
t
funtions
v
anish
for
small
momen
ta.
Therefore,
the
in
tegrals
are
infrared
nite.
The
b
eha
viors
of
the
w
eigh
t
funtions
for
large
v
alues
of
Q
1
and/or
Q
2
an
also
b
e
w
ork
ed
out
analytially
.
F
rom
these,
one
an
dedue
that
in
the
ase
of
the
WZW
form
fator,
the
orresp
onding,
div
ergen
t,
in
tegral
for
a
(
0
;1)
b
eha
v
es,
as
a
funtion
of
the
ultra
violet
ut
o
,
as
a
(
0
;1)
C
ln
2
,
with
[104
â„„
C
=
3
N
C
12
2
m
F
2
=
0:0248
:
(5.30)
The
log-squared
b
eha
vior
follo
ws
from
the
general
struture
of
the
in
tegral
(5.28)
for
a
(
0
;1)
in
the
ase
of
a
onstan
t
form
fator,
as
p
oin
ted
out
in
[5â„„.
The
expression
(5.30)
of
the
o
eÆien
t
C
has
b
een
deriv
ed
indep
enden
tly
,
in
Ref.
[115
â„„,
through
a
renormalization
group
argumen
t
in
the
eetiv
e
theory
framew
ork.
T
able
6:
Results
for
the
terms
a
(
0
;1)
,
a
(
0
;2)
and
for
the
pion
ex
hange
on
tribution
to
the
anoma-
lous
magneti
momen
t
a
h.
LL;
0
aording
to
Eq.
(5.27)
for
the
dieren
t
form
fators
onsidered.
In
the
WZW
mo
del
w
e
used
a
uto
of
1
GeV
in
the
rst
on
tribution,
whereas
the
seond
term
is
ultra
violet
nite.
F
orm
fator
a
(
0
;1)
a
(
0
;2)
a
h.
LL;
0
10
10
WZW
0.095
0.0020
12.
2
VMD
0.044
0.0013
5.6
LMD
0.057
0.0014
7.3
In
the
ase
of
the
other
form
fators,
the
in
tegration
o
v
er
Q
1
and
Q
2
is
nite
and
an
no
w
b
e
p
erformed
n
umerially
.
18
F
urthermore,
sine
b
oth
the
VMD
and
LMD
mo
del
tend
to
the
WZW
onstan
t
form
fator
as
M
V
!
1,
the
results
for
a
(
0
;1)
in
these
mo
dels
should
sale
as
C
ln
2
M
2
V
for
a
large
resonane
mass.
This
has
b
een
he
k
ed
n
umerially
,
and
the
v
alue
of
the
o
eÆien
t
C
obtained
that
w
a
y
w
as
in
p
erfet
agreemen
t
with
the
v
alue
giv
en
in
Eq.
(5.30).
The
results
of
the
in
tegration
o
v
er
Q
1
and
Q
2
are
displa
y
ed
in
T
able
6.
They
denitely
sho
w
a
sign
dierene
when
ompared
to
those
obtained
in
Refs.
[100
,
101
,
103
,
111
â„„,
although
in
absolute
v
alue
the
n
um
b
ers
agree
p
erfetly
.
After
the
results
of
T
able
6
w
ere
made
publi
[104
â„„,
previous
authors
he
k
ed
their
alulations
and
so
on
diso
v
ered
that
they
had
made
a
sign
mistak
e
at
some
stage
[105
,
106
â„„.
Almost
sim
ultaneously
,
the
results
presen
ted
in
T
able
6
and
in
Refs.
[104
,
115
â„„
also
reeiv
ed
indep
enden
t
onrmations
[117
,
116
â„„.
The
analysis
of
[104
â„„
leads
to
the
follo
wing
estimates
a
h.
LL;
0
=
5:8(1:0)
10
10
;
(5.31)
and
a
h.
LL;
0
e
=
5:1
10
14
:
(5.32)
T
aking
in
to
aoun
t
the
other
on
tributions
omputed
b
y
previous
authors,
and
adopting
a
onser-
v
ativ
e
attitude
to
w
ards
the
error
to
b
e
asrib
ed
to
their
mo
del
dep
endenes,
the
total
on
tribution
to
a
oming
from
the
hadroni
ligh
t-b
y-ligh
t
sattering
diagrams
amoun
ts
to
a
h.
LL
=
8(4)
10
10
:
(5.33)
18
In
the
ase
of
the
VMD
form
fator,
an
analytial
result
is
no
w
also
a
v
ailable
[116â„„.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
117
5.3
Eletro
w
eak
on
tributions
to
a
Eletro
w
eak
orretions
to
a
ha
v
e
b
een
onsidered
at
the
one
and
t
w
o
lo
op
lev
els.
The
one
lo
op
on
tributions,
sho
wn
in
Fig.
13,
ha
v
e
b
een
w
ork
ed
out
some
time
ago,
and
read
[118
â„„-[122
â„„
a
W(1)
=
G
F
p
2
m
2
8
2
"
5
3
+
1
3
1
4
sin
2
W
2
+
O
m
2
M
2
Z
log
M
2
Z
m
2
!
+
O
m
2
M
2
H
log
M
2
H
m
2
!
#
;
(5.34)
where
the
w
eak
mixing
angle
is
dened
b
y
sin
2
W
=
1
M
2
W
=
M
2
Z
.
νν
H
W
W
W
Z
0
µ
Figure
13:
One
lo
op
w
eak
in
teration
on
tributions
to
the
anomalous
magneti
momen
t.
Numerially
,
with
G
F
=
1:16639(1)
10
5
GeV
2
and
sin
2
W
=
0:224,
a
W(1)
=
19:48
10
10
;
(5.35)
It
is
on
v
enien
t
to
separate
the
t
w
o{lo
op
eletro
w
eak
on
tributions
in
to
t
w
o
sets
of
F
eynman
graphs:
those
whi
h
on
tain
losed
fermion
lo
ops,
whi
h
are
denoted
b
y
a
EW(2);f
,
and
the
others,
a
EW(2);b
.
In
this
notation,
the
eletro
w
eak
on
tribution
to
the
m
uon
anomalous
magneti
momen
t
is
a
EW
=
a
W(1)
+
a
EW(2);f
+
a
EW(2);b
:
(5.36)
I
shall
review
the
alulation
of
the
t
w
o{lo
op
on
tributions
separately
.
5.3.1
Tw
o
lo
op
b
osoni
on
tributions
The
leading
logarithmi
terms
of
the
t
w
o{lo
op
eletro
w
eak
b
osoni
orretions
ha
v
e
b
een
extrated
using
asymptoti
expansion
te
hniques,
see
e.g.
Ref.
[123
â„„.
In
the
appro
ximation
where
sin
2
W
!
0
and
M
H
M
W
these
alulations
simplify
onsiderably
and
one
obtains
a
EW(2);b
=
G
F
p
2
m
2
8
2
65
9
ln
M
2
W
m
2
+
O
sin
2
W
ln
M
2
W
m
2
:
(5.37)
In
fat,
these
on
tributions
ha
v
e
no
w
b
een
ev
aluated
analytially
,
in
a
systemati
expansion
in
p
o
w
ers
of
sin
2
W
,
up
to
O
[(sin
2
W
)
3
â„„
;
where
ln
M
2
W
m
2
terms,
ln
M
2
H
M
2
W
terms,
M
2
W
M
2
H
ln
M
2
H
M
2
W
terms,
M
2
W
M
2
H
terms
and
onstan
t
terms
are
k
ept
[75â„„.
Using
sin
2
W
=
0:224
and
M
H
=
250
GeV
;
the
authors
of
Ref.
[75
â„„
nd
a
EW(2);b
=
G
F
p
2
m
2
8
2
5:96
ln
M
2
W
m
2
+
0:19
=
G
F
p
2
m
2
8
2
(
79:3)
;
(5.38)
sho
wing,
in
retrosp
et,
that
the
simple
appro
ximation
in
Eq.
(5.37)
is
rather
go
o
d.
118
M.
Kne
h
t
S
eminaire
P
oinar
e
5.3.2
Tw
o
lo
op
fermioni
on
tributions
The
disussion
of
the
t
w
o{lo
op
eletro
w
eak
fermioni
orretions
is
more
deliate.
First,
it
on
tains
a
hadroni
on
tribution.
Next,
b
eause
of
the
anellation
b
et
w
een
lepton
lo
ops
and
quark
lo
ops
in
the
eletro
w
eak
U
(1)
anomaly
,
one
annot
separate
hadroni
eets
from
leptoni
eets
an
y
longer.
In
fat,
as
disussed
in
Refs.
[124
,
125
â„„,
it
is
this
anellation
whi
h
eliminates
some
of
the
large
logarithms
whi
h,
inorretly
w
ere
k
ept
in
Ref.
[126
â„„.
It
is
therefore
appropriate
to
separate
the
t
w
o{lo
op
eletro
w
eak
fermioni
orretions
in
to
t
w
o
lasses:
One
is
the
lass
arising
from
F
eynman
diagrams
on
taining
a
lepton
or
a
quark
lo
op,
with
the
external
photon,
a
virtual
photon
and
a
virtual
Z
0
atta
hed
to
it,
see
Fig.
14.
19
The
quark
lo
op
of
ourse
again
represen
ts
non
p
erturbativ
e
hadroni
on
tributions
whi
h
ha
v
e
to
b
e
ev
aluated
using
some
mo
del.
This
rst
lass
is
denoted
b
y
a
EW(2);f
(`;
q
).
It
in
v
olv
es
the
QCD
orrelation
funtion
W
(q
;
k
)
=
Z
d
4
x
e
iq
x
Z
d
4
y
e
i(k
q
)y
h
jTfj
(x)A
(Z
)
(y
)j
(0)gji
;
(5.39)
with
k
the
inoming
external
photon
four-momen
tum
asso
iated
with
the
lassial
external
mag-
neti
eld.
As
previously
,
j
denotes
the
hadroni
part
of
the
eletromagneti
urren
t,
and
A
(Z
)
is
the
axial
omp
onen
t
of
the
urren
t
whi
h
ouples
the
quarks
to
the
Z
0
gauge
b
oson.
The
other
lass
is
dened
b
y
the
rest
of
the
diagrams,
where
quark
lo
ops
and
lepton
lo
ops
an
b
e
treated
separately
,
and
is
alled
a
EW(2);f
(residual
).
Z
Z
p
q
+
p'
p'
p
p
p'
-
q
γ
γ
γ
γ
µ
µ
Figure
14:
Graphs
with
hadroni
on
tributions
to
a
EW(2);f
(`;
q
)
and
in
v
olving
the
QCD
three
p
oin
t
funtion
W
(q
;
k
).
The
on
tribution
from
a
EW(2);f
(residual)
brings
in
fators
of
the
ratio
m
2
t
=
M
2
W
.
It
has
b
een
esti-
mated,
to
a
v
ery
go
o
d
appro
ximation,
in
Ref.
[125
â„„,
with
the
result
a
EW(2);f
(residual
)
=
G
F
p
2
m
2
8
2
1
2
sin
2
W
5
8
m
2
t
M
2
W
log
m
2
t
M
2
W
7
3
+
Higgs
;
(5.40)
where
Higgs
denotes
the
on
tribution
from
diagrams
with
Higgs
lines,
whi
h
the
authors
of
Ref.
[125
â„„
estimate
to
b
e
Higgs
=
5:5
3:7
;
(5.41)
and
therefore,
a
EW(2);f
(residual
)
=
G
F
p
2
m
2
8
2
[
21(4)â„„
:
(5.42)
19
If
one
w
orks
in
a
renormalizable
gauge,
the
on
tributions
where
the
Z
0
is
replaed
b
y
the
neutral
unph
ysial
Higgs
should
also
b
e
inluded.
The
nal
result
do
es
not
dep
end
on
the
gauge
parameter
Z
,
if
one
w
orks
in
the
lass
of
't
Ho
oft
gauges.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
119
Let
us
nally
disuss
the
on
tributions
to
a
EW(2);f
(`;
q
).
Here,
it
is
on
v
enien
t
to
treat
the
on
tri-
butions
from
the
three
generations
separately
.
The
on
tribution
from
the
third
generation
an
b
e
alulated
in
a
straigh
tforw
ard
w
a
y
,
with
the
result
[124
,
125
â„„
a
EW(2);f
(
;
t;
b)
=
G
F
p
2
m
2
8
2
3
ln
M
2
Z
m
2
ln
M
2
Z
m
2
b
8
3
ln
m
2
t
M
2
Z
+
8
3
+
O
M
2
Z
m
2
t
ln
m
2
t
M
2
Z
=
G
F
p
2
m
2
8
2
(
30:6)
:
(5.43)
In
fat
the
terms
of
O
M
2
Z
m
2
t
ln
m
2
t
M
2
Z
and
O
M
2
Z
m
2
t
ha
v
e
also
b
een
alulated
in
Ref.
[125
â„„.
There
are
in
priniple
QCD
p
erturbativ
e
orretions
to
this
estimate,
whi
h
ha
v
e
not
b
een
alulated,
but
the
result
in
Eq.
(5.43)
is
go
o
d
enough
for
the
auray
required
at
presen
t.
The
on
tributions
of
the
remaining
harged
standard
mo
del
fermions
in
v
olv
e
the
ligh
t
quarks
u
and
d,
as
w
ell
as
the
seond
generation
s
quark,
for
whi
h
non
p
erturbativ
e
eets
tied
to
the
sp
on
taneous
breaking
of
hiral
symmetry
are
imp
ortan
t
[124
,
127
â„„.
The
on
tributions
from
the
rst
and
seond
generation
are
th
us
most
on
v
enien
tly
tak
en
together,
with
the
result
a
EW(2);f
(e;
;
u;
d;
s;
)
=
G
F
p
2
m
2
8
2
3
ln
M
2
Z
m
2
5
2
3
ln
M
2
Z
m
2
+
4
ln
M
2
Z
m
2
11
6
+
8
9
2
8
+
"
4
3
ln
M
2
Z
m
2
+
2
3
+
O
m
2
M
2
Z
ln
M
2
Z
m
2
!
#
1:38(35)
+
0:06(2)
)
(5.44)
=
G
F
p
2
m
2
8
2
[
34:5(4)â„„
;
(5.45)
where
the
rst
line
sho
ws
the
result
from
the
e
lo
op
and
the
seond
line
the
result
from
the
lo
op
and
the
quark,
whi
h
is
treated
as
a
hea
vy
quark.
The
term
b
et
w
een
bra
k
ets
in
the
third
line
is
the
one
indued
b
y
the
anomalous
term
in
the
hadroni
three
p
oin
t
funtion
W
(q
;
k
)
The
other
on
tributions
ha
v
e
b
een
estimated
on
the
basis
of
an
appro
ximation
to
the
large-N
C
limit
of
QCD,
similar
to
the
one
disussed
for
the
t
w
o-p
oin
t
funtion
(Q
2
)
after
Eq.
(5.12),
see
Ref.
[127
â„„
for
details.
The
result
in
Eq.
(5.44)
for
the
on
tribution
from
the
rst
and
seond
generations
of
quarks
and
leptons
is
oneptually
v
ery
dieren
t
to
the
orresp
onding
one
prop
osed
in
Ref.
[125
â„„,
a
EW(2);f
(`;
q
)(e;
;
u;
d;
s;
)
=
G
F
p
2
m
2
8
2
3
ln
M
2
Z
m
2
+
4
ln
M
2
Z
m
2
u
ln
M
2
Z
m
2
d
5
2
6
o
3
ln
M
2
Z
m
2
+
4
ln
M
2
Z
m
2
ln
M
2
Z
m
2
s
11
6
+
8
9
2
6
(5.46)
=
G
F
p
2
m
2
8
2
(
31:9)
:
(5.47)
where
the
ligh
t
quarks
are,
arbitr
arily,
treated
the
same
w
a
y
as
hea
vy
quarks,
with
m
u
=
m
d
=
0:3
GeV
;
and
m
s
=
0:5
GeV
:
Although,
n
umerially
,
the
t
w
o
results
turn
out
not
to
b
e
to
o
dif-
feren
t,
the
result
in
Eq.
(5.46)
follo
ws
from
an
hadroni
mo
del
whi
h
is
in
on
tradition
with
basi
prop
erties
of
QCD.
This
is
at
the
origin
of
the
spurious
anellation
of
the
ln
M
Z
terms
in
Eq.
(5.46).
120
M.
Kne
h
t
S
eminaire
P
oinar
e
Putting
together
the
n
umerial
results
in
Eqs.
(5.38),
(5.42),
(5.43)
with
the
new
result
in
Eq.
(5.44),
w
e
nally
obtain
the
v
alue
a
EW
=
G
F
p
2
m
2
8
2
5
3
+
1
3
1
4
sin
2
W
2
(165:4(4:0)
=
15:0(1)
10
10
;
(5.48)
whi
h
sho
ws
that
the
t
w
o{lo
op
orretion
represen
ts
indeed
a
redution
of
the
one{lo
op
result
b
y
an
amoun
t
of
23%.
The
nal
error
here
do
es
not
inlude
higher
order
eletro
w
eak
eets
[128
â„„.
5.4
Comparison
with
exp
erimen
t
W
e
ma
y
no
w
put
all
the
piees
together
and
obtain
the
v
alue
for
a
predited
b
y
the
standard
mo
del.
W
e
ha
v
e
seen
that
in
the
ase
of
the
hadroni
v
auum
p
olarization
on
tributions,
the
latest
ev
aluation
[92
â„„
sho
ws
a
disrepany
b
et
w
een
the
v
alue
obtained
exlusiv
ely
from
e
+
e
data
and
the
v
alue
that
arises
if
data
are
also
inluded.
This
giv
es
us
the
t
w
o
p
ossibilities
a
SM
(e
+
e
)
=
(11
659
169:1
7:5
4:0
0:3)
10
10
a
SM
(
)
=
(11
659
186:3
6:2
4:0
0:3)
10
10
;
(5.49)
where
the
rst
error
omes
from
hadroni
v
auum
p
olarization,
the
seond
from
hadroni
ligh
t-b
y-
ligh
t
sattering,
and
the
last
from
the
QED
and
w
eak
orretions.
When
ompared
to
the
presen
t
exp
erimen
tal
a
v
erage
a
exp
=
(11
659
203
8)
10
10
(5.50)
there
results
a
dierene,
a
exp
a
SM
(e
+
e
)
=
33:9(11:2)
10
10
;
a
exp
a
SM
(
)
=
16:7(10:7)
10
10
;
whi
h
represen
ts
3.0
and
1.6
standard
deviations,
resp
etiv
ely
.
Although
exp
erimen
t
and
theory
ha
v
e
no
w
b
oth
rea
hed
the
same
lev
el
of
auray
,
8
10
10
or
0:7
ppm,
the
presen
t
disrepany
b
et
w
een
the
e
+
e
and
based
ev
aluations
mak
es
the
in
terpretation
of
the
ab
o
v
e
results
a
deliate
issue
as
far
as
evidene
for
new
ph
ysis
is
onerned.
Other
ev
aluations
of
omparable
auray
[88
,
90
,
41
â„„
o
v
er
a
similar
range
of
v
ariation
in
the
dierene
b
et
w
een
exp
erimen
t
and
theory
.
One
p
ossibilit
y
to
ome
to
a
onlusion
w
ould
b
e
to
ha
v
e
the
exp
erimen
tal
result
still
more
aurate,
so
that
ev
en
the
dierene
a
exp
a
SM
(
)
w
ould
b
eome
suÆien
tly
signian
t.
In
this
resp
et,
it
is
ertainly
v
ery
imp
ortan
t
that
the
Bro
okha
v
en
exp
erimen
t
is
giv
en
the
means
to
impro
v
e
on
the
v
alue
of
a
exp
,
bringing
its
error
do
wn
to
4
10
10
or
0:35
ppm.
F
urthermore,
the
v
alue
obtained
for
a
SM
(e
+
e
)
relies
strongly
on
the
lo
w-energy
data
obtained
b
y
the
CMD-2
exp
erimen
t,
with
none
of
the
older
data
able
to
he
k
them
at
the
same
lev
el
of
preision.
In
this
resp
et,
the
prosp
ets
for
additional
high
statistis
data
in
the
future,
either
from
KLOE
or
from
BaBar,
are
most
w
elome.
On
the
other
hand,
if
the
presen
t
disrepany
in
the
ev
aluations
of
the
hadroni
v
auum
p
olarization
nds
a
solution
in
the
future,
and
if
the
exp
erimen
tal
error
is
further
redued,
b
y
,
sa
y
,
a
fator
of
t
w
o,
then
the
theoretial
unertain
t
y
on
the
hadroni
ligh
t-b
y-ligh
t
sattering
will
onstitute
the
next
serious
limitation
on
the
theoretial
side.
It
is
ertainly
w
orth
while
to
dev
ote
further
eorts
to
a
b
etter
understanding
of
this
on
tribution,
for
instane
b
y
nding
w
a
ys
to
feed
more
onstrain
ts
with
a
diret
link
to
QCD
in
to
the
desriptions
of
the
four-p
oin
t
funtion
(q
1
;
q
2
;
q
3
).
6
Conluding
remarks
With
this
review,
I
hop
e
to
ha
v
e
on
vined
the
reader
that
the
sub
jet
of
the
anomalous
magneti
momen
ts
of
the
eletron
and
of
the
m
uon
is
an
exiting
and
fasinating
topi.
It
pro
vides
a
go
o
d
example
of
m
utual
stim
ulation
and
strong
in
terpla
y
b
et
w
een
exp
erimen
t
and
theory
.
V
ol.
2,
2002
The
Anomalous
Magneti
Momen
ts
of
the
Eletron
and
the
Muon
121
The
anomalous
magneti
momen
t
of
the
eletron
onstitutes
a
v
ery
stringen
t
test
of
QED
and
of
the
pratial
w
orking
of
the
framew
ork
of
p
erturbativ
ely
renormalized
quan
tum
eld
theory
at
higher
orders.
It
tests
the
v
alidit
y
of
QED
at
v
ery
short
distanes,
and
pro
vides
at
presen
t
the
b
est
determination
of
the
ne
struture
onstan
t.
The
anomalous
magneti
momen
t
of
the
m
uon
represen
ts
the
b
est
ompromise
b
et
w
een
sensitivit
y
to
new
degrees
of
freedom
desribing
ph
ysis
b
ey
ond
the
standard
mo
del
and
exp
erimen
tal
feasibil-
it
y
.
Imp
ortan
t
progress
has
b
een
a
hiev
ed
on
the
exp
erimen
tal
side
during
the
last
ouple
of
y
ears,
with
the
results
of
the
E821
ollab
oration
at
BNL.
The
exp
erimen
tal
v
alue
of
a
is
no
w
kno
wn
with
an
auray
of
0.7ppm.
Hop
efully
,
the
Bro
okha
v
en
exp
erimen
t
will
b
e
giv
en
the
opp
ortunit
y
to
rea
h
its
initial
goal
of
a
hieving
a
measuremen
t
at
the
0.35
ppm
lev
el.
As
an
b
e
inferred
from
the
examples
men
tioned
in
this
text,
the
sub
jet
onstitutes,
from
a
theo-
retial
p
oin
t
of
view,
a
diÆult
and
error
prone
topi,
due
to
the
te
hnial
diÆulties
enoun
tered
in
the
higher
lo
op
alulations.
The
theoretial
preditions
ha
v
e
rea
hed
a
preision
omparable
to
the
exp
erimen
tal
one,
but
unfortunately
there
app
ears
a
disrepany
b
et
w
een
the
most
reen
t
ev
aluations
of
the
hadroni
v
auum
p
olarization
aording
to
whether
data
are
tak
en
in
to
a-
oun
t
or
not.
Hadroni
on
tributions,
esp
eially
from
v
auum
p
olarization
and
from
ligh
t-b
y-ligh
t
sattering,
are
resp
onsible
for
the
bulk
part
of
the
nal
unertain
t
y
in
the
theoretial
v
alue
a
SM
.
F
urther
eorts
are
needed
in
order
to
bring
these
asp
ets
under
b
etter
on
trol.
A
kno
wledgmen
ts
I
wish
to
thank
A.
Nyeler,
S.
P
eris,
M.
P
errottet,
and
E.
de
Rafael
for
stim
ulating
and
v
ery
pleas-
an
t
ollab
orations,
and
for
sharing
man
y
insigh
ts
on
this
v
ast
sub
jet
and
on
related
topis.
Most
of
the
gures
app
earing
in
this
text
w
ere
kindly
pro
vided
b
y
M.
P
errottet,
to
whom
I
am
also
most
grateful
for
a
areful
and
ritial
reading
of
the
man
usript.
Finally
,
I
wish
to
thank
B.
Duplan
tier
and
V.
Riv
asseau
for
the
in
vitation
to
giv
e
a
presen
tation
at
the
\S
eminaire
P
oinar
e".
This
w
ork
is
supp
orted
in
part
b
y
the
EC
on
trat
No.
HPRN-CT-2002-00311
(EURIDICE).
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h
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eminaire
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oinar
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T.
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eltman,
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[14â„„
E.
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v
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B.
E.
Lautrup
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de
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E.
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L.
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T.
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J.
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ory
of
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A
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