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

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

Jan 26, 2024 159 likes •403 views

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

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SLIDE 1

S- and p-wave structure of S = -1 meson- baryon scattering in the resonance region

Daniel Sadasivan Maxim Mai Michael Doring

Supported by DOE SCGSR, NSF (PIF No.1415459, CAREER PHY-1452055), DOE DE-AC05-06OR23177 & DE-SC0016582), DFG MA 7156/1-1. 1

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SLIDE 2

Motivation

2

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SLIDE 3

What is a Resonance

  • 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.

1340 1360 1380 1400 1420 1440 0.5 0.0 0.5 1.0 1.5 WCMS MeV Re f fm 1340 1360 1380 1400 1420 1440 0.0 0.5 1.0 1.5 2.0 2.5 WCMS MeV Re f fm

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SLIDE 4

Resonances We Are Looking For

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SLIDE 5

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.

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SLIDE 6

Method

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SLIDE 7

Model

T T V 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

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SLIDE 8

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

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SLIDE 9

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

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SLIDE 10

10

  • 1.0
  • 0.5

0.0 0.5 1.0 0.0 0.5 1.0 1.5 2.0 Cos θ dσ dΩ (mb)

K- p→K0 n (275 MeV)

0.0 0.5 1.0 1.5 2.0 dσ dΩ (mb)

K- p→K0 n (235 MeV)

2.0 2.5 3.0 3.5 4.0 4.5 5.0 dσ dΩ (mb)

K- p→K0 n (265 MeV)

2 4 6 8 10 dσ dΩ (mb)

K- p→K0 n (225 MeV)

1.0

  • 0.5

0.0 0.5 1.0 Cos θ

K- p→K0 n (285 MeV) K- p→K0 n (245 MeV) K- p→K0 n (275 MeV) K- p→K0 n (235 MeV)

1.0

  • 0.5

0.0 0.5 1.0 Cos θ

K- p→K0 n (295 MeV) K- p→K0 n (255 MeV) K- p→K0 n (285 MeV) K- p→K0 n (245 MeV)

1.0

  • 0.5

0.0 0.5 1.0 Cos θ

K- p→K0 n (265 MeV) K- p→K0 n (295 MeV) K- p→K0 n (255 MeV)

Fit to the Data: New Data

Differential cross sections fitted by the model.

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SLIDE 11

More Data

1.30 1.35 1.40 1.45 1.50 M [GeV] arbitrary units

1. 2. 3. d/dMinv [b/GeV] Wtot=2. GeV Wtot=2.1 GeV

00 +-
  • +

Wtot=2.2 GeV 0.5 1 d/dMinv [b/GeV] Wtot=2.3 GeV Wtot=2.4 GeV Wtot=2.5 GeV 1.35 1.4 1.45 0.2 0.4 0.6 Minv [GeV] d/dMinv [b/GeV] Wtot=2.6 GeV 1.35 1.4 1.45 Minv [GeV] Wtot=2.7 GeV 1.35 1.4 1.45 Minv [GeV] Wtot=2.8 GeV

Fit of the generic couplings K−p→Σ(1660)π−and Σ(1660)→(π−Σ+)π+to the invariant mass distribution in arbitrary units.

  • R. J. Hemingway, Nucl. Phys. B253, 742 (1985).

. 11 Fit (χ2pp= 1.07) to theπ Σ invariant mass distribution (Minv) from γp→K+(πΣ) reaction.

  • K. Moriya et al. (CLAS), Phys. Rev. C87,

035206 (2013), arXiv:1301.5000 [nucl-ex].

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SLIDE 12

Predictions

12

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SLIDE 13
  • 8.
  • 4.

0. 4. 8. 12. 16. fJ

I [GeV-1]

0(1/2-)

  • 1.
  • 2.

0.

  • 1. 0(1/2+)

1.25 1.30 1.35 1.40 1.45

  • 1.

0. 1. 2. 3. 4. W [GeV] fJ

I [GeV-1]

1(1/2-)

1.25 1.30 1.35 1.40 1.45

  • 3.
  • 1.
  • 2.

0. 1. W [GeV]

1(1/2+)

PWA Amplitudes

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I(JP) Imaginary part of ̄KN partial Real part of ̄KN partial

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SLIDE 14

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

  • ther 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.

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SLIDE 15

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.

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SLIDE 16

Analysis

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SLIDE 17

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.

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SLIDE 18

Lasso Test of Robustness

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

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SLIDE 19

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.

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SLIDE 20

Σ(1385)

  • 1.0
  • 0.5

0.0 0.5 1.0 0.0 0.5 1.0 1.5 2.0 Cos θ dσ/dΩ [mb] K-p→K 0n (w=265 MeV) 0.0 0.5 1.0 1.5 2.0 dσ/dΩ[mb] 2.0 2.5 3.0 3.5 4.0 4.5 5.0 dσ/dΩ[mb] K-p→K-p (w=265 MeV) 2 4 6 8 10 dσ/dΩ[mb] K-p→K-p (w=225 MeV) 1.0

  • 0.5

0.0 0.5 1.0 Cos θ K-p→K 0n (w=275 MeV) K-p→K 0n (w=235 MeV) K-p→K-p (w=275 MeV) K-p→K-p (w=235 MeV) 1.0

  • 0.5

0.0 0.5 1.0 Cos θ K-p→K 0n (w=285 MeV) K-p→K 0n (w=245 MeV) K-p→K-p (w=285 MeV) K-p→K-p (w=245 MeV) 1.0

  • 0.5

0.0 0.5 1.0 Cos θ K-p→K 0n (w=295 MeV) K-p→K 0n (w=255 MeV) K-p→K-p (w=295 MeV) K-p→K-p (w=255 MeV)

Reversed Formula for the differential cross section The partial waves of the best fit. We additionally include a black line to show the best fit when the partial waves are reversed. Real Formula for the differential cross section

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SLIDE 21

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.

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SLIDE 22

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.

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SLIDE 23

Thank You

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