From photo data to poles Ron Workman Data

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From (photo) data to poles Ron Workman Data Analysis Center Institute for Nuclear Studies

From (photo) data to poles Ron Workman Data Analysis Center Institute for Nuclear Studies George Washington University Baryons 2013 University of Glasgow

Some thoughts on N* photo-couplings ● How do Breit-Wigner and pole photo-couplings compare? ●

Some thoughts on N* photo-couplings ● How do Breit-Wigner and pole photo-couplings compare? ● E 2/M 1 values are clearly different ● Some old pole values (VT) differ from more recent Bonn-Gatchina values. ● Is the similarity of Bonn-Gatchina pole/BW results dependent on model details?

A. V. Anisovich et al. , EPJ A 48 (2012) 15 Pole and Breit-Wigner

A. V. Anisovich et al. , EPJ A 48 (2012) 15 Pole and Breit-Wigner values similar apart from a phase

Pole vs BW widths very different for S 11 and P 11 | Rπ

Pole vs BW widths very different for S 11 and P 11 | Rπ | different from current values

Photo-decay amplitudes from multipoles Quantities (real) evaluated at BW resonance energy Quantities (complex) evaluated

Photo-decay amplitudes from multipoles Quantities (real) evaluated at BW resonance energy Quantities (complex) evaluated at pole position C: isospin factor

SAID model for pion photoproduction ( 1990 ) Tππ gives phase (Watson’s Thm) Phase

SAID model for pion photoproduction ( 1990 ) Tππ gives phase (Watson’s Thm) Phase determined by Tππ (smooth connection to Watson’s Thm)

Simple case: Δ(1232) 3/2+ 0. 054 phase: -115 o BG: ~ 0. 052 phase:

Simple case: Δ(1232) 3/2+ 0. 054 phase: -115 o BG: ~ 0. 052 phase: -125 o

Pole vs BW contributions for Δ(1232) RLW, R. A. Arndt, PRC 59, 1810 (1999)

Pole vs BW contributions for Δ(1232) RLW, R. A. Arndt, PRC 59, 1810 (1999) Largest contribution: E 2 (pole) 0 ~ linear Largest contribution: M 1 (pole) Term → 0 for W = 1232 Me. V ( no contribution to BW + background approach ) Don’t expect approaches to be similar for E 2/M 1

Dominant pieces for E 2 and M 1

Dominant pieces for E 2 and M 1

A 1/2 , A 3/2 for Δ(1232) at the pole

A 1/2 , A 3/2 for Δ(1232) at the pole

Some comparative results for A 1/2 , A 3/2 Breit-Wigner values extracted using a

Some comparative results for A 1/2 , A 3/2 Breit-Wigner values extracted using a form similar to MAID Agreement with pole values is reasonable even for cases with Rπ = Γπ / 2 being a poor approximation

Some other background forms plus Crawford/Morton ‘ 83 Berends/Donnachie ‘ 78 Arai/Fujii ‘ 82

Some other background forms plus Crawford/Morton ‘ 83 Berends/Donnachie ‘ 78 Arai/Fujii ‘ 82 Resonance Background

Kamano et al. , Dyn CC model Large differences

Kamano et al. , Dyn CC model Large differences

Kamano et al. , ar. Xiv 1305. 4351 ( May 2013) Program is ambitious

Kamano et al. , ar. Xiv 1305. 4351 ( May 2013) Program is ambitious Difficult to determine source of differences in photo-couplings: Fit quality vs DCC

Obtaining the residues ● analytic continuation / contour integrals ● speed plots ● Padé

Obtaining the residues ● analytic continuation / contour integrals ● speed plots ● Padé approx ● regularization method Zagreb/Tuzla ● ‘Pietarinen expansion’ BW: technically simple – but model dependent Pole: model independent – but new technical issues may arise

Laurent Padé Pietarinen (Pere Masjuan) (A. Svarc)

Laurent Padé Pietarinen (Pere Masjuan) (A. Svarc)

Cut plane Z f b c a e See, for example, H. Burkhardt Dispersion

Cut plane Z f b c a e See, for example, H. Burkhardt Dispersion Relation Dynamics, Ch. A 9 Unit circle e μ b a c f

Zagreb-Tuzla form Z Z 0 ZC Compare to:

Zagreb-Tuzla form Z Z 0 ZC Compare to:

F 15 SAID πN SP 06 ( A. Svarc )

F 15 SAID πN SP 06 ( A. Svarc )

Interesting results when applied to SES, with no analytic form available to determine poles

Interesting results when applied to SES, with no analytic form available to determine poles ( A. Svarc ) Application to multipoles is being studied

Other material

Other material

For next speaker: 2 fits with 1 or 2 D 13 states πN

For next speaker: 2 fits with 1 or 2 D 13 states πN

Characteristic forward peaking in charged-pion photoproduction Feature is absent in this plot from ar.

Characteristic forward peaking in charged-pion photoproduction Feature is absent in this plot from ar. Xiv: 1305. 4351 v 1