Productions of X(1835) as baryonium with sizable gluon content

Details Productions of X(1835) as baryonium with sizable gluon content Productions of X(1835) as baryonium with sizable gluon content

2005-11-15

arxiv.org/abs/hep-ph/0511186v3

Eur.Phys.J.A28:351-360,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

21 pages, 4 figures

Scientific paper

10.1140/epja/i2006-10055-3

The X(1835) has been treated as a baryonium with sizable gluon content, and to be almost flavor singlet. This picture allows us to rationally understand X(1835) production in $J/\psi$ radiative decays, and its large couplings with $p\bar{p}$, $\eta^{\prime}\pi\pi$. The processes $\Upsilon(1S)\to \gamma X(1835)$ and $J/\psi\to \omega X(1835)$ have been examined. It has been found that $Br(\Upsilon(1S)\to\gamma X(1835))Br(X(1835)\to p\bar{p})<6.45\times10^{-7}$, which is compatible with CLEO's recently experimental result (Phys.Rev.$\mathbf{D73}$ (2006) 032001;hep-ex/0510015). The branching fractions of $Br(J/\psi\to\omega X(1835))$, $Br(J/\psi\to\rho X(1835))$ with $X(1835)\to p\bar{p}$ and $X(1835)\to\eta^{\prime}\pi^{+}\pi^{-}$ have been estimated by the quark-pair creation model. We show that they are heavily suppressed, so the signal of X(1835) is very difficult, if not impossible, to be observed in these processes. The experimental checks for these estimations are expected. The existence of the baryonium nonet is conjectured, and a model independent derivation of their production branching fractions is presented.

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