Abstract
Abstract
A new proposal to compute the anomalous chromomagnetic dipole moment of the top quark,
μ
ˆ
t
, in the Standard Model is presented. On the basis of the five-dimensional effective Lagrangian operator that characterizes the quantum-loop induced chromodipolar vertices
gt
t
¯
and
ggt
t
¯
, the
μ
ˆ
t
anomaly is derived via radiative correction at the 1-loop level from the non-Abelian 4-body vertex function
ggt
t
¯
. We evaluate
μ
ˆ
t
(
s
)
as a function of the energy scale s = ±E
2, for E = [10, 1000] GeV, taking into account the running of the quark masses and alpha strong through the
MS
¯
scheme. In particular, we find that at the typical energy scale E = m
Z
for high-energy physics, similarly to
α
s
(
m
Z
2
)
,
α
(
m
Z
2
)
and
s
W
(
m
Z
2
)
, the spacelike evaluation yields
μ
ˆ
t
(
−
m
Z
2
)
= −0.025 + 0.00384i and the timelike
μ
ˆ
t
(
m
Z
2
)
= −0.0318 − 0.0106i. This Re
μ
ˆ
t
(
−
m
Z
2
)
= −0.025 from
ggt
t
¯
is even closer to the experimental central value
μ
ˆ
t
Exp
=
−0.024, than that coming from the known 3-body vertex function
gt
t
¯
, −0.0224. Once again, the Im
μ
ˆ
t
(
−
m
Z
2
)
part is due to the contribution of virtual charged currents, just like in the
gt
t
¯
case. We can infer that the spacelike prediction is the favored one.
Subject
Nuclear and High Energy Physics