Abstract

Since its first observation in 2005, the vector charmonium Y(4260)Y(4260) has turned out to be one of the prime candidates for an exotic state in the charmonium spectrum. It was recently proposed that the Y(4260)Y(4260) should have a prominent D1Dˉ+c.c.D_1\bar{D}+c.c. molecular component that is strongly correlated with the production of the charged Zc(3900)Z_c(3900). In this paper we demonstrate that the nontrivial cross section line shapes of e+e−→J/ψππe^+e^-\to J/ψππ and hcππh_cππ can be naturally explained by the molecular scenario. As a consequence we find a significantly smaller mass for the Y(4260)Y(4260) than previous studied. In the e+e−→DˉD∗π+c.c.e^+e^-\to \bar D D^*π+c.c. process, with the inclusion of an additional SS-wave Dˉ∗π\bar D^*π contribution constrained from data on the DDˉ∗D\bar D^* invariant mass distribution, we obtain a good agreement with the data of the angular distributions. We also predict an unusual line shape of Y(4260)Y(4260) in this channel that may serve as a smoking gun for a predominantly molecular nature of Y(4260)Y(4260). Improved measurements of these observables are therefore crucial for a better understanding of the structure of this famous resonance.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.