\newcommand{\ksks}{$K_S^0 K_S^0$\xspace} \newcommand{\Ks}{$K_S^0$\xspace} \newcommand{\ffa}{$f_{2}(1270)/a_{2}^{0}(1320)$\xspace} \newcommand{\ffb}{$f_{2}^{'}(1525)$\xspace} \newcommand{\ffc}{$f_{0}(1710)$\xspace} Title: Inclusive \ksks resonance production in $ep$ collisions at HERA Speaker: Changyi Zhou on behalf of ZEUS Collaboration McGill University czhou@physics.mcgill.ca The lightest glueball is predicted to have $J^{PC}=0^{++}$ \cite{1 and 2} and a mass in the range 1450--1750 MeV. Thus, it can mix with $q\overline{q}$ states from the scalar meson nonet, which have $I=0$ and similar masses. In the literature, the state \ffc is frequently considered to be a state with a possible glueball or tetraquark composition (see for example the reviews \cite{Klempt:2007cp,*Oller}). Inclusive \ksks production in $ep$ collisions dominated by photoproduction with exchanged photon virtuality, $Q^2$, below 1 $\gev^2$. at HERA has been studied with the ZEUS detector using an integrated luminosity of 0.5 fb-1 from "HERAI and HERAII" combined. \Ks mesons were identified through the charged-decay mode, $K_s^0 \to\pi^{+}\pi^{-}$, and reconstructed with various track quality cuts for selection. The \ksks invariant mass distribution was reconstructed by combining two \Ks candidates. Enhancements in the mass spectrum have been observed attributed to the production of f2(1270)/a02(1320), f'2(1525) and f0(1710). The three states $f_{2}(1270)$, $a_{2}^{0}(1320)$ and \ffb are all of $J^P = 2^+$ and so their interference is seen in the total cross-section. The intensity is the modulus-squared of the sum of these three amplitudes plus the incoherent addition of \ffc and the non-resonant background. The amplitudes for $f_{2}(1270)$, $a_{2}^{0}(1320)$ and \ffb production were fixed at the SU(3) ratios of $5:-3:2$ as expected for production via an electromagnetic process~\cite{Althoff,lipkin}. Very competitive measurements on peak position and width for \ffb and \ffc are done with interference fit and the overall fit describes the data very well. Complete systematic checks have been performed. The final values with statistical and systematical uncertainties were compared well with the PDG values~\cite{7.PDG}. References: 1. C. J. Morningstar and M. Peardon, Phys. R173 Rev. D 60, 034509 (1999); 2. C. Michael and M. Teper, Nucl. Phys. B 314, 347 (1989). 3. E. Klempt and A. Zaitsev, Phys. Rept. 454, 1 (2007); 4. M. Albaladejo, J. A. Oller, Preprint hep-ph/0801.4929, 2008. 5. Althoff, M. and others, Phys. Lett. B121, 216 (1983). 6. Faiman, D. and Lipkin, H. J. and Rubinstein, H. R., Phys. Lett. B59, 269 (1975). 7. Particle Data Group, W.-M. Yao et al., J. Phys. G33, 1 (2006); and 2007 partial update for edition 2008 (URL:http://pdf.lbl.gov).