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Sigma(1385) Resonance Studies with STAR at sqrt{s_{NN}}=200 GeV

Sevil Salur
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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)\toΛ+πwere 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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Sevil Salur. 2004-03-10. Sigma(1385) Resonance Studies with STAR at sqrt{s_{NN}}=200 GeV. https://arxiv.org/abs/hep-ex/0403016

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