Abstract

The spin density matrix of the \(\omega \) has been determined for the reaction \({\bar{p}p}\,\rightarrow \,\omega \pi ^0\) with unpolarized in-flight data measured by the Crystal Barrel LEAR experiment at CERN. The two main decay modes of the \(\omega \) into \(\pi ^0 \gamma \) and \(\pi ^+ \pi ^- \pi ^0\) have been separately analyzed for various \({\bar{p}}\)momenta between 600 and 1940 MeV/c. The results obtained with the usual method by extracting the matrix elements via the \(\omega \) decay angular distributions and with the more sophisticated method via a full partial wave analysis are in good agreement. A strong spin alignment of the \(\omega \) is clearly visible in this energy regime and all individual spin density matrix elements exhibit an oscillatory dependence on the production angle. In addition, the largest contributing orbital angular momentum of the \({\bar{p}p~}\)system has been identified for the different beam momenta. It increases from \(L^{max}_{{\bar{p}p~}}\) \(=\) 2 at 600 MeV/c to \(L^{max}_{{\bar{p}p~}}\) \(=\) 5 at 1940 MeV/c.

Highlights

  • The spin density matrix of particles originating from pp annihilations provides important information about the underlying production process

  • The knowledge of this property is quite scarce in the low energy regime for pp in-flight reactions and is, very fundamental for high quality and high statistics future experiments like PANDA [1]

  • The performed partial wave analysis has taken into account the complete reaction chain starting from the pp coupling up to the final state particles

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Summary

Introduction

The spin density matrix of particles originating from pp annihilations provides important information about the underlying production process The knowledge of this property is quite scarce in the low energy regime for pp in-flight reactions and is, very fundamental for high quality and high statistics future experiments like PANDA [1]. For the neutral decay mode the polarization of the radiative photon has not been measured and it is needed to average over this property. Similar studies of this reaction for the charged decay mode of the ω have already been published in [3]. First preliminary results for the charged decay mode have already been presented in [2]

Crystal barrel experiment
Data selection and measured angular distributions
Signal-background separation
Overview of the selected data samples
Measured angular and λ-distributions
Partial wave analysis
Fits to data and determination of the parameters α
Comparison of data and fits
Spin density matrix of the ω
Findings
Summary

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