Physics Letters B 738 (2014) 172–177
Contents lists available at ScienceDirect
Physics Letters B
www.elsevier.com/locate/physletb
Enhanced breaking of heavy quark spin symmetry
Feng-Kun Guo
a,∗
, Ulf-G. Meißner
a,b
, Cheng-Ping Shen
c
a
Helmholtz-Institut für Strahlen- und Kernphysik and Bethe Center for Theoretical Physics, Universität Bonn, D-53115 Bonn, Germany
b
Institute for Advanced Simulation, Institut für Kernphysik and Jülich Center for Hadron Physics, Forschungszentrum Jülich, D-52425 Jülich, Germany
c
School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China
a r t i c l e i n f o a b s t r a c t
Article history:
Received
30 June 2014
Received
in revised form 16 July 2014
Accepted
19 September 2014
Available
online 26 September 2014
Editor: A.
Ringwald
Heavy quark spin symmetry is useful to make predictions on ratios of decay or production rates of
systems involving heavy quarks. The breaking of spin symmetry is generally of the order of O (Λ
QCD
/m
Q
),
with Λ
QCD
the scale of QCD and m
Q
the heavy quark mass. In this paper, we will show that a small
S-and D-wave mixing in the wave function of the heavy quarkonium could induce a large breaking
in the ratios of partial decay widths. As an example, we consider the decays of the Υ(10 860) into the
χ
bJ
ω ( J =0, 1, 2), which were recently measured by the Belle Collaboration. These decays exhibit a huge
breaking of the spin symmetry relation were the Υ(10 860) a pure 5S bottomonium state. We propose
that this could be a consequence of a mixing of the S-wave and D-wave components in the Υ(10 860).
Prediction on the ratio Γ(Υ(10 860) → χ
b0
ω)/Γ (Υ (10 860) → χ
b2
ω) is presented assuming that the
decay of the D-wave component is dominated by the coupled-channel effects.
© 2014 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license
(http://creativecommons.org/licenses/by/3.0/). Funded by SCOAP
3
.
A heavy quarkonium is a system consisting of a heavy quark
and a heavy antiquark. The ground states and low-lying excited
states below the open-flavor thresholds were well described in
terms of potential quark models, e.g., the Godfrey–Isgur quark
model [1], while the higher excited states are more complicated.
The complexity comes from, e.g., the nearby strongly coupled
thresholds, the existence of many new quarkonium-like states dis-
covered
in the last decade and so on. Because the heavy quark
mass m
Q
is much larger than the scale of quantum chromodynam-
ics
(QCD), Λ
QCD
, the amplitude of changing the spin orientation
of a heavy quark by interacting with soft gluons is small, sup-
pressed
by O(Λ
QCD
/m
Q
) relative to the spin-conserving case [2].
The resulting heavy quark spin symmetry (HQSS) [3] can lead
to important observable consequences. On the one hand, heavy
quarkonium states are organized into spin multiplets; on the other
hand, the decay or production rate involving one heavy quarko-
nium
can often be related to the one of its spin partners in the
leading approximation. Breaking of HQSS is typically of the order
of O(Λ
QCD
/m
Q
) or even higher. In this paper, we will argue that
the HQSS breaking could be much larger in certain processes. To
be specific, we will show that a small mixing of S- and D-wave
*
Corresponding author.
E-mail
addresses: fkguo@hiskp.uni-bonn.de (F.-K. Guo),
meissner@hiskp.uni-bonn.de (U.-G. Meißner), shencp@ihep.ac.cn (C.-P. Shen).
heavy quarkonia could result in a significant breaking of the spin
symmetry relations when the decay amplitude of the D-wave com-
ponent
is enhanced. As an example, we will calculate the processes
Υ(10 860) → χ
bJ
ω ( J = 0, 1, 2). Measurements for these transi-
tions
were done by the Belle Collaboration very recently, and the
results for the branching fractions are [4]
B
Υ(
10 860) → χ
b0
ω
<
3.9 ×10
−3
,
B
Υ(
10 860) → χ
b1
ω
=(
1.57 ±0.22
stat.
±0.21
sys.
) ×10
−3
,
B
Υ(
10 860) → χ
b2
ω
=(
0.60 ±0.23
stat.
±0.15
sys.
) ×10
−3
. (1)
One sees that the branching fraction for the χ
b1
ω mode is larger
than that for the χ
b2
ω. Comparing the HQSS prediction on the
ratio B(Υ (5S) → χ
b1
ω)/B(Υ (5S) → χ
b2
ω) = 0.63 assuming the
Υ(10 860) to be the 5S bottomonium state, see Eq. (6) below, with
the observed value 2.62 ± 1.30, the breaking is more than 100%.
This is a very large spin symmetry breaking. As we will show later,
a small mixture of a D-wave
¯
bb component in the Υ(10 860) is
able to cause the ratios of Γ(Υ(10 860) → χ
bJ
ω) to be very dif-
ferent
from the spin symmetry relations as observed.
Consequences
of HQSS can be easily analyzed using heavy me-
son
effective field theory (for a review, see Ref. [5]). Let us take the
transitions from a vector heavy quarkonium into the χ
J
ω as an
example, where χ
J
is a P -wave heavy quarkonium with quantum
http://dx.doi.org/10.1016/j.physletb.2014.09.043
0370-2693/
© 2014 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/3.0/). Funded by
SCOAP
3
.