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

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

2004-03-10

arxiv.org/abs/hep-ex/0403016v1

Physics

High Energy Physics

High Energy Physics - Experiment

NATO ASI Structure and Dynamics of Elementary Matter Conference Proceeding for Poster Presentation

Scientific paper

In p+p, d+Au, and Au+Au collisions at \sqrt{s_{NN}}=200 GeV with the STAR
detector at RHIC, \Sigma(1385)\to\Lambda+\pi 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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