Study on production of exotic 0+ meson DsJ*(2317) in decays of (4415)

Abstract

The newly observed DsJ* family containing DsJ*(2317), DsJ(2460) and DsJ(2632) attracts great interests. Determining their structure may be important tasks for both theorists and experimentalists. In this work we use the heavy quark effective theory (HQET) and a non-relativistic model to evaluate the production rate of DsJ*(2317) from the decays of (4415), and we find that it is sizable and may be observed at BES III and CLEO, if it is a p-wave excited state of Ds(1968). Unfortunately, the other two members of the family cannot be observed through decays of charmonia, because of the constraints from the final state phase space.

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