https://doi.org/10.1140/epjp/s13360-023-04260-2
Regular Article
Strange partners of the doubly charmed tetraquark
1
Institute for Physical Problems, Baku State University, Az–1148, Baku, Azerbaijan
2
Department of Physics, University of Tehran, North Karegar Avenue, 14395-547, Tehran, Iran
3
Department of Physics, Doǧuş University, Dudullu-Ümraniye, 34775, Istanbul, Turkey
4
Department of Physics, Kocaeli University, 41380, Izmit, Turkey
5
Department of Physics Engineering, Istanbul Medeniyet University, 34700, Istanbul, Turkey
Received:
9
January
2023
Accepted:
6
July
2023
Published online:
17
July
2023
The spectroscopic parameters and widths of the axial-vector and scalar
,
strange partners of the doubly charmed exotic meson
with the content
, are calculated in the framework of the QCD sum rule method. We model
as the diquark–antidiquark state composed of axial-vector and scalar components, whereas scalar particles
and
are built of axial-vector and scalar diquarks, respectively. The masses and current couplings of these tetraquarks are calculated in the context of the two-point sum rule approach by taking into account the quark, gluon and mixed condensates up to dimension 10. The full width of the state
is found from analysis of the processes
and
. Decays to
,
and
mesons are utilized in the case of the scalar tetraquarks
and
, respectively. The partial widths of the aforementioned decays are determined via the strong couplings
,
,
,
and
, which describe the strong interactions of the particles at the relevant tetraquark–meson–meson vertices. These couplings are computed using the QCD three-point sum rule method, most appropriate for the strong decays under study. The predictions
and
, as well as
,
and
and
obtained for the masses and widths of these tetraquarks in the present work can be useful in future experimental investigations of the doubly charmed four-quark resonances.
Copyright comment Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.