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Σ(1385) Resonance Studies with Star at \(\sqrt {{S_{NN}}} = 200\;GeV\)

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Structure and Dynamics of Elementary Matter

Part of the book series: NATO Science Series ((NAII,volume 166))

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Abstract

In p+p, d+Au, and Au+Au collisions at \(\sqrt {{S_{NN}}} = 200\;GeV\) with the STAR detector at RHIC, Σ (1385) → Λ + π were measured using two techniques; three-particle mixing and a hybrid mixing technique. We present results from both of these methods and compare the invariant mass spectra and the backgrounds.

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References

  1. Marcus Bleicher, hep-ph/0212378

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Author information

Authors and Affiliations

  1. Physics Department, Yale University, 272 Whitney Ave., New Haven, CT, USA

    Sevil Salur

Authors
  1. Sevil Salur
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Editor information

Editors and Affiliations

  1. Institut für Theoretische Physik, Johann Wolfgang Goethe-Universität, Robert Mayer Str. 10, 60054, Frankfurt am Main, Germany

    Walter Greiner  & Joachim Reinhardt  & 

  2. Flerov Laboratory of Nuclear Reactions, Joint Institute of Nuclear Research, 141980, Dubna, Moscow region, Russia Federation

    Mikhail G. Itkis

  3. Department of Physics, Istanbul Technical University, 80626, Maslak, Istanbul, Turkey

    Mehmet Cem Güçlü

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© 2004 Springer Science+Business Media Dordrecht

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Salur, S. (2004). Σ(1385) Resonance Studies with Star at \(\sqrt {{S_{NN}}} = 200\;GeV\) . In: Greiner, W., Itkis, M.G., Reinhardt, J., Güçlü, M.C. (eds) Structure and Dynamics of Elementary Matter. NATO Science Series, vol 166. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2705-5_60

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  • DOI: https://doi.org/10.1007/978-1-4020-2705-5_60

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-1-4020-2446-7

  • Online ISBN: 978-1-4020-2705-5

  • eBook Packages: Springer Book Archive

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