Slide 1 K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at  s NN = 200 GeV & 62.4 GeV Motivation Analysis and Results Summary 1 Sadhana Dash Institute of…

Sadhana Dash Institute of Physics, Bhubaneswar (For STAR Collaboration) Outline: Importance of K* studies K*/, /K*  information on interplay of rescattering and…

NCC Task Force Richard Seto NCC Task Force Meeting Jan 8, 2007 BNL Agenda Assessment of where we are and time schedule - plans for work over the holiday. I would like to…

Pentaquark Search and S* Results from STAR What is Q+ ? Why S* ? How can we search for them at RHIC? What did we learn so far? What else can we do in the near future? Sevil…

Sadhana Dash Institute of Physics, Bhubaneswar (For STAR Collaboration) Outline: Importance of K* studies K*/, /K*  information on interplay of rescattering and…

Measurement of non-statistical fluctuations D. Kresan GSI, Darmstadt Three contributions to data due to the finite number of particles produced and observed per event,…

* June 2, 2009 D.P. Weygand Vector Mesons in the Nuclear Medium and the CLAS Collaboration D.P. Weygand R. Nasseripour, M. H. Wood, C. Djalali R. Nasseripour et al. Jul 2007.Phys.Rev.Lett.99:262302,2007.…

Charged Particle Multiplicity at Mid-Rapidity in Au-Au Collisions at RHIC David Silvermyr Div. of Cosmic and Subatomic Physics Lund University Outline Predictions for dNch/dh…