S- and p-wave structure of S = -1 meson- baryon scattering in the - PowerPoint PPT Presentation

S- and p-wave structure of S = -1 meson- baryon scattering in the resonance region Supported by DOE SCGSR, NSF (PIF No.1415459, CAREER PHY-1452055), DOE DE-AC05-06OR23177 & DE-SC0016582), DFG MA 7156/1-1. Daniel Sadasivan Maxim Mai Michael Doring 1

Motivation 2

What is a Resonance 1.5 2.5 1.0 2.0 Re f � fm � Re f � fm � 0.5 1.5 0.0 1.0 � 0.5 0.5 0.0 1340 1360 1380 1400 1420 1440 1340 1360 1380 1400 1420 1440 W CMS � MeV � W CMS � MeV � • Seen in peak at a certain energy in scattering cross sections. • Assigned to certain quantum numbers. • Can be studied through analytic continuation • Useful to relate results to other theories like quark models and lattice QCD. 3

Resonances We Are Looking For 4

Applications • Λ (1405) is dominated by KN interaction • A similar mechanism can be responsible for the generation of K − pp bound states. See for example, S. Ajimura et al arXiv:1805.12275 [nucl-ex]. • The equation of state of neutron stars is sensitive to the antikaon condensate and thus to the propagation of antikaons in nuclear medium. 5

Method 6

Model T V T V A depiction of the operator form of the Bethe Saltpeter Equation. The bubble chain summation caused by iteration of the Bethe Salpeter Ansatz The chiral expansion of the driving term, V. 7

Possible Meson Baryon Interactions for S=-1 Possible channels for S=-1 interactions. The data that exists in the energy region of interest is shown in red. 8

Fit to the Data: Old Data In addition, we fit to threshold data including data from the SIDDHARTA Experiment Total cross sections fitted by the model. The dashed black line shows the contribution of the s-wave part of the amplitude only. 9

Fit to the Data: New Data 10 K - p → K 0 n ( 225 MeV ) K - p → K 0 n ( 235 MeV ) K - p → K 0 n ( 245 MeV ) K - p → K 0 n ( 255 MeV ) 8 d Ω ( mb ) 6 d σ 4 2 5.0 K - p → K 0 n ( 265 MeV ) K - p → K 0 n ( 275 MeV ) K - p → K 0 n ( 285 MeV ) K - p → K 0 n ( 295 MeV ) 4.5 4.0 d Ω ( mb ) 3.5 d σ 3.0 2.5 2.0 2.0 K - p → K 0 n ( 235 MeV ) K - p → K 0 n ( 245 MeV ) K - p → K 0 n ( 255 MeV ) K - p → K 0 n ( 265 MeV ) 1.5 d Ω ( mb ) 1.0 d σ 0.5 0.0 2.0 K - p → K 0 n ( 275 MeV ) K - p → K 0 n ( 285 MeV ) K - p → K 0 n ( 295 MeV ) 1.5 d Ω ( mb ) 1.0 d σ 0.5 0.0 - 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 Cos θ Cos θ Cos θ Cos θ Differential cross sections fitted by the model. 10

More Data arbitrary units Fit ( χ 2pp = 1.07) to the π Σ invariant mass distribution (M inv ) from γ p → K+( πΣ ) reaction. K. Moriya et al. (CLAS), Phys. Rev. C87, 035206 (2013), arXiv:1301.5000 [nucl-ex]. 1.30 1.35 1.40 1.45 1.50 W tot = 2. GeV W tot = 2.1 GeV W tot = 2.2 GeV � 0 � 0 3. � + � - M �� [ GeV ] d � / dM inv [ � b / GeV ] Fit of the generic couplings K − p → Σ (1660) π− and � - � + 2. Σ (1660) → ( π−Σ +) π +to the invariant mass 1. distribution in arbitrary units. R. J. Hemingway, Nucl. Phys. B253, 742 (1985). W tot = 2.3 GeV W tot = 2.4 GeV W tot = 2.5 GeV d � / dM inv [ � b / GeV ] . 1 0.5 W tot = 2.6 GeV W tot = 2.7 GeV W tot = 2.8 GeV 0.6 d � / dM inv [ � b / GeV ] 0.4 0.2 1.35 1.4 1.45 1.35 1.4 1.45 1.35 1.4 1.45 M inv [ GeV ] M inv [ GeV ] M inv [ GeV ] 11

Predictions 12

PWA Amplitudes Imaginary part of ̄ KN partial Real part of ̄ KN partial I(J P ) 1. 0 ( 1 / 2 + ) 0 ( 1 / 2 - ) 16. 12. I [ GeV - 1 ] 8. 0. 4. 0. - 1. f J - 4. - 8. - 2. 1 ( 1 / 2 - ) 1 ( 1 / 2 + ) 4. 1. 3. I [ GeV - 1 ] 0. 2. - 1. 1. f J - 2. 0. - 1. - 3. 1.25 1.30 1.35 1.40 1.45 1.25 1.30 1.35 1.40 1.45 W [ GeV ] W [ GeV ] 13

Λ (1405) Left: Pole positions (black stars) for the 0(1/2 − ). The error ellipses are from a re-sampling procedure shown explicitly in the corresponding insets. The shaded squares show the prediction from other literature for the narrow (blue) and broad (orange) pole of Λ (1405) Below: A plot of the amplitude in the complex plane that shows the two peaks. 14

An Anomalous Structure Left: A representation of the position of a pole in the best fit of our model in the 1(1/2 + ) Channel. Below: The amplitudes of the couplings for the poles observed in the best fit. 15

Analysis 16

Possible Explanations of the Anomalous Structure When a structure is observed in a good fit to good data and does not have the quantum numbers of any known state, categorically speaking there are three possibilities. 1. It’s present because the data demonstrate that there exists an undiscovered state in nature. 2. It’s present because the data require the model to account for something it isn’t currently accounting for. 3. It’s completely arbitrary; it’s existence does not improve the fit in any way. 17

Lasso Test of Robustness The amplitude that is penalized. Plot of Lasso (Least Absolute Shrinkage and Selection Operator) Method. 18

Possible Explanations of the Anomalous Structure When a structure is observed in a good fit to the data and does not have the quantum numbers of any known state, categorically speaking there are three possibilities. 1. It’s present because the data demonstrate that there exists an undiscovered state in nature. 2. It’s present because the data require the model to account for something it isn’t currently accounting for. 3. It’s completely arbitrary; it’s existence does not improve the fit in any way. 19

Σ (1385) The partial waves of the best fit. We additionally include a black line to show the best fit when the partial waves are reversed. 10 K - p → K - p ( w = 225 MeV ) K - p → K - p ( w = 235 MeV ) K - p → K - p ( w = 245 MeV ) K - p → K - p ( w = 255 MeV ) 8 d σ / d Ω [ mb ] 6 Real Formula for the differential cross section 4 2 5.0 K - p → K - p ( w = 265 MeV ) K - p → K - p ( w = 275 MeV ) K - p → K - p ( w = 285 MeV ) K - p → K - p ( w = 295 MeV ) 4.5 d σ / d Ω [ mb ] 4.0 3.5 Reversed Formula for the differential cross 3.0 2.5 section 2.0 2.0 K - p → K 0 n ( w = 235 MeV ) K - p → K 0 n ( w = 245 MeV ) K - p → K 0 n ( w = 255 MeV ) 1.5 d σ / d Ω [ mb ] 1.0 0.5 0.0 2.0 K - p → K 0 n ( w = 265 MeV ) K - p → K 0 n ( w = 275 MeV ) K - p → K 0 n ( w = 285 MeV ) K - p → K 0 n ( w = 295 MeV ) 1.5 d σ / d Ω [ mb ] 1.0 0.5 0.0 - 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 1.0 - 0.5 0.0 0.5 1.0 Cos θ Cos θ Cos θ Cos θ 20

Possible Explanations of the Anomalous Structure When a structure is observed in a good fit to the data and does not have the quantum numbers of any known state, categorically speaking there are three possibilities. 1. It’s present because the data demonstrate that there exists an undiscovered state in nature. 2. It’s present because the data require the model to account for something it isn’t currently accounting for. 3. It’s completely arbitrary; it’s existence does not improve the fit in any way. 21

Summary • The Mai-Meissner Model is fit to differential cross section as well as older data. This constitutes the first ever simultaneous fit of all data without explicit resonances. • Both poles of the Λ (1405) were reproduced • A new anomalous structure was observed that didn’t have the right parity for the Σ (1385). • This statistically robust state likely exists because the differential cross section data demand a p-wave resonance and a NLO model cannot give it the right J. 22

Thank You 23