'Energy scan' diaporamas de présentation

The freeze-out source shape: recent results from the STAR energy scan

The freeze-out source shape: recent results from the STAR energy scan. Mike Lisa (Ohio State University) for the STAR Collaboration. Outline. general motivation RHIC BES program asHBT a growing database of asHBT systematics (another) anomalous behaviour at SPS? new STAR data

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STAR Future Plans and Upgrades

STAR Future Plans and Upgrades. Run 10 Run 11 Beyond. Hank Crawford UCB/SSL for the STAR Collaboration. STAR Physics Goals for Run 10. search for QCD Critical point and for disappearance of signatures seen at top RHIC energy through Beam Energy Scan (BES) .

573 views • 50 slides

Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt

Towards the Heavy-Ion Program at J-PARC. 1. Introduction 2. H eavy ion acceleration scheme 3. Physics goals 4 . E xperimental design 5. Summary. Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt. Introduction. LHC RHIC. SPS.

615 views • 49 slides

Report from

( ). *. ( ) still a conventional name !. *. Report from. A. Passeri. Expression of Interest Physics goals Detector developments Collaboration setup. http://www.lnf.infn.it/lnfadmin/direzione/KLOE2-LoI.pdf. 72 physicists. 12 institutions. Expression of Interest.

486 views • 40 slides

Report from

( ). *. ( ) still a conventional name !. *. Report from. A. Passeri. Expression of Interest Physics goals Detector developments Collaboration setup. http://www.lnf.infn.it/lnfadmin/direzione/KLOE2-LoI.pdf. 72 physicists. 12 institutions. Expression of Interest.

544 views • 40 slides

QCD in Twenty-One Century

508 views • 36 slides

DRS-II results on electron energy scan (Signal integration method)

DRS-II results on electron energy scan (Signal integration method). F.Bedschi, R. Carosi, M.Incagli, F.Scuri. - A summary of what we learned on features and limits of the DRS chip version II by looking at the Cherenkov and the Scintillation electron signals from the

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STAR Perspectives for RHIC Energy Scan

355 views • 27 slides

Low energy scan and collective flow at 9 GeV

Low energy scan and collective flow at 9 GeV. Jiayun Chen , Feng Liu, Shusu Shi, Kejun Wu. Weihai , Aug. 9,2009. Outline. Motivation Collectivity from STAR at 9.2GeV MC Simulation at 9 GeV Summary and Outlook. Motivation. QM09 : SS Shi (STAR Collaboration). QCD Phase diagram.

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ILC Physics and Detectors

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STAR Physics at RNC Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory

STAR Physics at RNC Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory. (1) Introduction (2) Selected recent results - partonic collectivity, coalescence, di-jets (3) Plan for FY09 - 11 - collective velocity, full jet reconstruction, direct radiation.

294 views • 20 slides

Run 2001 Muon Physics Opportunities

Run 2001 Muon Physics Opportunities. Vince Cianciolo Muon Meeting BNL, 12/16/2000. What Will RHIC Provide?. 4 weeks of cooldown (starting 4/1). 3 weeks AuAu beam tests plus minimum 300 m b-1 AuAu full energy (12 weeks). 3 weeks spin commisioning + 5 weeks running (goal to reach BB).

273 views • 15 slides

STAR Ready to move on to 7.7 GeV Bill Christie For The STAR Collaboration April 13, 2010.

STAR Ready to move on to 7.7 GeV Bill Christie For The STAR Collaboration April 13, 2010. Please N.B. All data plots shown in this presentation are online QA plots, and are not for distribution. STAR BUR10. Run 10: 30 cryo-weeks, 25 weeks for physics production with a single species

213 views • 10 slides