The puzzle of excessive non-D D component of the inclusive (3770) decay and the long-distant contribution
Abstract
In this letter we suggest that the obvious discrepancy between theoretical prediction on the non-D D decays of (3770) and data is to be alleviated by taking final state interaction (FSI) into account. By assuming that (3770) overwhelmingly dissociates into D D, then the final state interaction induces a secondary process, we calculate the branching ratios of (3770) D D J/η, π, ωη, K*K. Our results show that the branching ratio of (3770) non-DD can reach up to Bnon-DDFSI=(0.21.1)% while typical parameters I=0.4 GeV-2 and α=0.8 1.3 are adopted. This indicates that the FSI is obviously non-negligible.
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