Double Ks0 Photoproduction off the proton at CLAS

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Presentation transcript:

Double Ks0 Photoproduction off the proton at CLAS S. Chandavar and K. Hicks CLAS Collaboration Meeting Oct. 4, 2017

Which scalar mesons are we interested in? There are 4 isoscalar states identified by experiment: f0(980), f0(1370), f0(1500) and f0(1710) There are only 2 slots for the f0 states in the quark model The assignments of the f0 states is still uncertain.

What theory predicts Mixing scenario LQCD calculations Physical states f0(1370), f0(1500), f0(1710) are a mixture of bare states Dependence on model Case 1: f0(1370) strong SU(3) singlet component f0(1500) strong SU(3) octet component f0(1710) strong glueball component Case 2: f0(1500) strong glueball component f0(1710) strong SU(3) octet component Figure: Y Chen et al., PRD 73:014516 (2006) V. Crede, C.Meyer arXiv:0812.0600v3

PWA formalism The intensity I(t)is expanded into a set of amplitudes : Isobar Model The intensity I(t)is expanded into a set of amplitudes : t = final state variables V = production amplitudes A = decay amplitudes J.P. Cummings , D.P. Weygand, arXiv: physics/0309052v1

PWA formalism Data is binned in mass and each mass bin is fit independently For each event, production amplitudes are calculated to maximize the likelihood of the event Amplitudes are factored into production amplitudes, eVkb (to be fitted), and decay amplitudes, eAb (calculated)

What previous experiments observed Clear peak at 1500, no peak at 1710 P pbar annihilation : Crystal Barrel C. Amsler and N.A. Tornqvist, Phys. Rept. 389 (2004) 61.

What previous experiments observed The f0(1500) and f2’(1525) are seen in the K+K- anaysis. The hh data also indicates the presence of the f0(1500) Coupled channel PWA analysis of K+K- and p+p- data Central Production : WA102 D. Barberis et al., [ WA102 Collaboration ], Phys. Lett. B462 (1999) 462, hep-ex/9907055

What previous experiments observed f0(1710) f0(1710) f0(1710) is seen here, but there is an absence of f0(1500) Partial wave analysis of J/ Y gp+p- and gp0p0 J/ψ radiative decay : BES II M. Ablikim et al., [ BES Collaboration ] Phys. Lett. B 642 (2006) 441

What previous experiments observed The K+K- spectrum is dominated by a peak at 1500 MeV B+  K+K+K- B meson decays : Belle P. Minkowski and W. Ochs, Eur. Phys. J. C39 (2005) 71, hep-ph/0404194

What previous experiments observed The LEP data shows a peak at 1710 MeV with undetermined spin gg  Ks0 Ks0 ᵞᵞ Collisions : LEP M. Acciarri et al., [ L3 Collaboration ] Phys. Lett. B501 (2001) 173, hep-ex/0011037

The paper that got us interested.. Why choose strange decay? M.Chanowitz suggests in PRL 95, 172001 (2005) that glueballs are more likely to decay to strange channels Why choose Ks0Ks0 ? Ensure that the final state has the same PC =++ as the lightest glueball ZEUS Collaboration: S. Chekanov, et al, Inclusive K0SK0S resonance production in ep collisions at HERA, Phys.Rev.Lett.101:112003,2008, arXiv:0806.0807v2

Photoproduction of scalar mesons Photoproduction might be effective in producing scalar mesons via Pomeron Exchange or via the hadronic component of the photon. Vincent Mathieu, Nikolai Kochelev, Vicente Vento arXiv:0810.4453 s-channel t-channel Photoproduction is a good way to study scalar mesons. Dominant mechanism : r, w exchange A. Donnachie, Y.S Kalashnikova arXiv:0806.3698v1

Event selection Missing mass off of 4p K0S invariant mass The adjoining plot shows the high correlation between the two K0s

Event selection The threshold photon energy to produce an f0(1500) is 2.7 GeV. In our analysis, we make a cut Eg > 2.7 GeV

Cuts used in this analysis

M(KsKs) Spectra Signal + Background (S+B) Signal - Background (S-B) Background (2-D sidebands)

Cuts on Mandelstam t t < 1.0 GeV2 t > 1.0 GeV2

Dalitz Plots (cut on t)

Phase space MC with f0(1500)

Angular Distributions (1475 MeV)

Angular Distributions (1525 MeV)

Angular Distributions (1575 MeV)

S-wave/D-wave fraction vs. M(KK)

Summary We see a significant peak above background at a mass of 1.50 GeV in M(KsKs) in g12 data. The calibrations for g12 are better than ~5 MeV. The peak at 1.50 GeV is enhanced at low |t|. This is indicative of t-channel production. Angular distribution in the GJ frame suggest (but do not prove) that it is mostly S-wave. This suggests we see the f0(1500) but cannot rule out some portion of the f2(1525) being present. Better data will be available at CLAS12 with FT.