Amplitudes from photo-production data (with minimal model input)

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Presentation transcript:

Amplitudes from photo-production data (with minimal model input) Ron Workman

Amplitude reconstruction Need 8 (or more) Observables → H or b set Multipole analysis Schematically ML ≈ ∫ H ei φ(E,ϴ) PL (x) dx Need theory input at this stage More theory input → fewer required observables? Isospin decomposition ? Consider πN scattering and photo-production

Phases and isospin π-p + √2 π0n = π+p 3 charge channels 2 isospin states (triangle relation) √2 π0n + π+n + π-p = √2 π0p 4 charge channels 3 isospin states (quadrilateral relation)

Fixing overall phases π0p π +n phase fixed I=3/2 π+n Grushin method: [ by ‘known’ high-L part (real) ] I=3/2 π+n Grushin method:

I=3/2 π+ n and π- p phases fixed π0 p π0 n π+ n π- p

Grushin Fits to π0p data at 350 MeV L ≥ 2 Fit L ≤ 1 Fix one phase

Grushin fit (blue) Re-fit (red) to π+ n at 340 MeV Fit L ≤ 1 Born L≥ 2 Modified Grushin fit (blue) and Re-fit (red) at 340 MeV for π+n Modified Grushin fit (blue) and Re-fit (red) at 340 MeV for π+n

Fits/predictions of π+ n at 340 MeV Fit (red) Predict (black) Predict beam-target G

Omelaenko analysis of ambiguities notes dσ/dΩ, P, Σ, T, E, H, Ox , Cz , Tx , Lz (no change)

Low-energy zero trajectories (π0 p) α : ● β : o (accidental symmetries give additional solutions) [ see Omelaenko, Yad. Fiz. 34, 730 (1981) ]

Fits to π0 p data at 350 MeV Fits 1, 2, and CRS are identical for dσ/dΩ, P, Σ, T data

Global (ED) versus Single-Energy (SE) Fits ● Generate pseudo-data (MD07) ● Fit with SAID ED form - generate SE fits ● Reproduce MD07 ? Motivation ● Are SAID/MAID differences due to data issues? ● Are SE fits ‘equivalent’ to underlying datasets?

Towards a model independent PWA for pseudoscalar meson photoproduction (more details in the plenary talk by Lothar Tiator) Towards a model independent PWA for pseudoscalar meson photoproduction Motivation Complete Experiments Pseudo Data Complete Amplitude Analysis Complete Truncated PWA Summary and Conclusion Lothar Tiator Amplitude Analysis in Hadron Spectroscopy, ECT* Workshop, Trento, January 24-28, 2011 13

MD07 (red curve) Pseudo-data (black points) Real data (blue points) p0p at 320-340 MeV and comparison with real data

dσ/dΩ, P, Σ, T Prediction compared to a fit of double-polarization observable (sign issue) E, F, G, H Ox , Oz , Cx , Cz

Multipole: predicted vs input

SAID vs MAID phase differences ED fit

Effect of searching phases in SE fits

Fit to K+ Λ photo-production W=1680 MeV ( L<2 fit, L>1 Born [D13 modified] )

Fit OZ - predict OX , CX , CZ

Multipoles compared to the Kaon MAID solution Solid (real part) Open (imag part) (solution not unique)

Conclusions ● clarified the connection between ED and SE fits ● SAID is able to reproduce MAID amplitudes from data (up to the second-resonance region) ● multipole fits/amplitude reconstructions require different input from experiment and theory ● amplitude zeros (old method) may help to compare fits (unitarity is a problem) ● kaon photoproduction results are mixed