Abstract
AbstractIn this paper, we make a detailed discussion on the $$\eta $$
η
and $$\eta ^\prime $$
η
′
-meson leading-twist light-cone distribution amplitude $$\phi _{2;\eta ^{(\prime )}}(u,\mu )$$
ϕ
2
;
η
(
′
)
(
u
,
μ
)
by using the QCD sum rules approach under the background field theory. Taking both the non-perturbative condensates up to dimension-six and the next-to-leading order (NLO) QCD corrections to the perturbative part, its first three moments $$\langle \xi ^n_{2;\eta ^{(\prime )}}\rangle |_{\mu _0} $$
⟨
ξ
2
;
η
(
′
)
n
⟩
|
μ
0
with $$n = (2, 4, 6)$$
n
=
(
2
,
4
,
6
)
can be determined, where the initial scale $$\mu _0$$
μ
0
is set as the usual choice of 1 GeV. Numerically, we obtain $$\langle \xi _{2;\eta }^2\rangle |_{\mu _0} =0.231_{-0.013}^{+0.010}$$
⟨
ξ
2
;
η
2
⟩
|
μ
0
=
0
.
231
-
0.013
+
0.010
, $$\langle \xi _{2;\eta }^4 \rangle |_{\mu _0} =0.109_{ - 0.007}^{ + 0.007}$$
⟨
ξ
2
;
η
4
⟩
|
μ
0
=
0
.
109
-
0.007
+
0.007
, and $$\langle \xi _{2;\eta }^6 \rangle |_{\mu _0} =0.066_{-0.006}^{+0.006}$$
⟨
ξ
2
;
η
6
⟩
|
μ
0
=
0
.
066
-
0.006
+
0.006
for $$\eta $$
η
-meson, $$\langle \xi _{2;\eta '}^2\rangle |_{\mu _0} =0.211_{-0.017}^{+0.015}$$
⟨
ξ
2
;
η
′
2
⟩
|
μ
0
=
0
.
211
-
0.017
+
0.015
, $$\langle \xi _{2;\eta '}^4 \rangle |_{\mu _0} =0.093_{ - 0.009}^{ + 0.009}$$
⟨
ξ
2
;
η
′
4
⟩
|
μ
0
=
0
.
093
-
0.009
+
0.009
, and $$\langle \xi _{2;\eta '}^6 \rangle |_{\mu _0} =0.054_{-0.008}^{+0.008}$$
⟨
ξ
2
;
η
′
6
⟩
|
μ
0
=
0
.
054
-
0.008
+
0.008
for $$\eta '$$
η
′
-meson. Next, we calculate the $$D_s\rightarrow \eta ^{(\prime )}$$
D
s
→
η
(
′
)
transition form factors (TFFs) $$f^{\eta ^{(\prime )}}_{+}(q^2)$$
f
+
η
(
′
)
(
q
2
)
within QCD light-cone sum rules approach up to NLO level. The values at large recoil region are $$f^{\eta }_+(0) = 0.476_{-0.036}^{+0.040}$$
f
+
η
(
0
)
=
0
.
476
-
0.036
+
0.040
and $$f^{\eta '}_+(0) = 0.544_{-0.042}^{+0.046}$$
f
+
η
′
(
0
)
=
0
.
544
-
0.042
+
0.046
. After extrapolating TFFs to the allowable physical regions within the series expansion, we obtain the branching fractions of the semi-leptonic decay, i.e. $$D_s^+\rightarrow \eta ^{(\prime )}\ell ^+ \nu _\ell $$
D
s
+
→
η
(
′
)
ℓ
+
ν
ℓ
, i.e. $${{\mathcal {B}}}(D_s^+ \rightarrow \eta ^{(\prime )} e^+\nu _e)=2.346_{-0.331}^{+0.418}(0.792_{-0.118}^{+0.141})\times 10^{-2}$$
B
(
D
s
+
→
η
(
′
)
e
+
ν
e
)
=
2
.
346
-
0.331
+
0.418
(
0
.
792
-
0.118
+
0.141
)
×
10
-
2
and $${{\mathcal {B}}}(D_s^+ \rightarrow \eta ^{(\prime )} \mu ^+\nu _\mu )=2.320_{-0.327}^{+0.413}(0.773_{-0.115}^{+0.138})\times 10^{-2}$$
B
(
D
s
+
→
η
(
′
)
μ
+
ν
μ
)
=
2
.
320
-
0.327
+
0.413
(
0
.
773
-
0.115
+
0.138
)
×
10
-
2
for $$\ell = (e, \mu )$$
ℓ
=
(
e
,
μ
)
channels respectively. And in addition to that, the mixing angle for $$\eta -\eta '$$
η
-
η
′
with $$\varphi $$
φ
and ratio for the different decay channels $${{\mathcal {R}}}_{\eta '/\eta }^\ell $$
R
η
′
/
η
ℓ
are given, which show good agreement with the recent BESIII measurements.
Funder
Central University Basic Research Fund of China
China Postdoctoral Science Foundation
Guizhou Science and Technology Department
Guizhou Minzu University
National Natural Science Foundation of China
Department of Education of Guizhou Province
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Cited by
12 articles.
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