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Role of $$\Xi (1690)$$ in the $$J/\psi \rightarrow \Xi ^0{\bar{\Lambda }}K^0$$ reaction
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Abstract
Motivated by the recent BESIII measurements of the
$$J/\psi \rightarrow \Xi ^0 {\bar{\Lambda }}K_S^0 + c.c.$$
J
/
ψ
→
Ξ
0
Λ
¯
K
S
0
+
c
.
c
.
process, we investigate this reaction by considering the contributions from the
$$\Xi (1690)$$
Ξ
(
1690
)
,
$$\Lambda (1890)$$
Λ
(
1890
)
and
$$\Lambda (1830)$$
Λ
(
1830
)
resonances. The
$$\Xi (1690)$$
Ξ
(
1690
)
state is dynamically generated from the
S
-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach. Our theoretical model provides a good description of the
$${\bar{\Lambda }}K^0$$
Λ
¯
K
0
,
$$\Xi ^0 K^0$$
Ξ
0
K
0
, and
$${\bar{\Lambda }}\Xi ^0$$
Λ
¯
Ξ
0
invariant mass distributions. The results indicate that the
$$\Xi (1690)$$
Ξ
(
1690
)
resonance, which was neglected in the experimental analysis by BESIII, plays a crucial role in this process. Furthermore, we evaluate the theoretical uncertainties of our model using the parametric bootstrap method. Future high-precision measurements of this process will further help to elucidate the properties of the
$$\Xi (1690)$$
Ξ
(
1690
)
,
$$\Lambda (1890)$$
Λ
(
1890
)
and
$$\Lambda (1830)$$
Λ
(
1830
)
states.
Springer Science and Business Media LLC
Title: Role of $$\Xi (1690)$$ in the $$J/\psi \rightarrow \Xi ^0{\bar{\Lambda }}K^0$$ reaction
Description:
Abstract
Motivated by the recent BESIII measurements of the
$$J/\psi \rightarrow \Xi ^0 {\bar{\Lambda }}K_S^0 + c.
c.
$$
J
/
ψ
→
Ξ
0
Λ
¯
K
S
0
+
c
.
c
.
process, we investigate this reaction by considering the contributions from the
$$\Xi (1690)$$
Ξ
(
1690
)
,
$$\Lambda (1890)$$
Λ
(
1890
)
and
$$\Lambda (1830)$$
Λ
(
1830
)
resonances.
The
$$\Xi (1690)$$
Ξ
(
1690
)
state is dynamically generated from the
S
-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach.
Our theoretical model provides a good description of the
$${\bar{\Lambda }}K^0$$
Λ
¯
K
0
,
$$\Xi ^0 K^0$$
Ξ
0
K
0
, and
$${\bar{\Lambda }}\Xi ^0$$
Λ
¯
Ξ
0
invariant mass distributions.
The results indicate that the
$$\Xi (1690)$$
Ξ
(
1690
)
resonance, which was neglected in the experimental analysis by BESIII, plays a crucial role in this process.
Furthermore, we evaluate the theoretical uncertainties of our model using the parametric bootstrap method.
Future high-precision measurements of this process will further help to elucidate the properties of the
$$\Xi (1690)$$
Ξ
(
1690
)
,
$$\Lambda (1890)$$
Λ
(
1890
)
and
$$\Lambda (1830)$$
Λ
(
1830
)
states.
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