Author:
Yue Zi-Li,Xiao Cheng-Jian,Chen Dian-Yong
Abstract
AbstractIn this work, we evaluated the widths of the pionic and radiative transitions from the $$T_{c\bar{s}0}^{+}(2900)$$
T
c
s
¯
0
+
(
2900
)
to the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
in the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
molecular frame and the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
charmed-strange meson frame. Our estimations demonstrate that the transition widths in the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
molecular frame are much larger than those in the the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
charmed-strange meson frame. Specifically, the ratio of the widths of $$\Gamma (T_{c\bar{s}0}^{+}(2900)\rightarrow D_{s1}^{+} \pi ^{0})$$
Γ
(
T
c
s
¯
0
+
(
2900
)
→
D
s
1
+
π
0
)
and $$\Gamma (T_{c\bar{s}0}^{+}(2900)\rightarrow D^{+(0)}K^{0(+)})$$
Γ
(
T
c
s
¯
0
+
(
2900
)
→
D
+
(
0
)
K
0
(
+
)
)
is estimated to be around 0.1 in the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
charmed-strange meson frame, whereas the lower limit of this ratio is 0.67 in the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
molecular frame. Thus, the aforementioned ratio could be employed as a tool for testing the nature of the $$D_{s1}^{+}(2460)$$
D
s
1
+
(
2460
)
.
Funder
National Natural Science Foundation of China
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Cited by
1 articles.
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