Abstract
Recent high-statistics Au+Au and Cu+Cu runs at RHIC have provided a wealth of new data that allow STAR to answer several outstanding questions regarding the nature of the hot, dense medium that is created in ultrarelativistic heavy-ion collisions. However, the new data also raise new questions that require further study. Here, we focus on a few qualitatively new results presented by STAR for the first time at Quark Matter ‘05.
Original language | English |
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Pages (from-to) | 409-414 |
Number of pages | 6 |
Journal | Nuclear Physics A |
Volume | 774 |
DOIs | |
Publication status | Published - 7 Aug 2006 |
Event | Quark Matter 2005: International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions, 18th - Budapest, Hungary Duration: 4 Aug 2005 → 9 Aug 2005 |