17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Exploring the Phase Diagram: The RHIC Contribution  RHIC is currently.

Slides:



Advertisements
Similar presentations
Mass, Quark-number, Energy Dependence of v 2 and v 4 in Relativistic Nucleus- Nucleus Collisions Yan Lu University of Science and Technology of China Many.
Advertisements

, CZE ISMD2005 Zhiming LI 11/08/ and collisions at GeV Entropy analysis in and collisions at GeV Zhiming LI (For the NA22 Collaboration)
Study of the Elementary Reaction Pete Markowitz Florida International University 28/05/2014.
Quark Matter 2006 ( ) Excitation functions of baryon anomaly and freeze-out properties at RHIC-PHENIX Tatsuya Chujo (University of Tsukuba) for.
Jet probes of nuclear collisions: From RHIC to LHC Dan Magestro, The Ohio State University Midwest Critical Mass October 21-22, 2005.
ICPAQGP, Kolkata, February 2-6, 2015 Itzhak Tserruya PHENIX highlights.
A probe for hot & dense nuclear matter. Lake Louise Winter Institute 21 February, 2000 Manuel Calderón de la Barca Sánchez.
Particle Production in p + p Reactions at GeV K. Hagel Cyclotron Institute Texas A & M University for the BRAHMS Collaboration.
January 12, 2007J. Sandweiss Two Important Long Range Programs for RHIC In addition to the many important RHIC research programs that are currently underway.
Experimental Results for Fluctuations And Correlations as a Signature of QCD Phase Transitions in Heavy Ion Collisions Gary Westfall Michigan State University,
5-12 April 2008 Winter Workshop on Nuclear Dynamics STAR Particle production at RHIC Aneta Iordanova for the STAR collaboration.
TIME-LIKE BARYON FORM FACTORS: EXPERIMENTAL SITUATION AND POSSIBILITIES FOR PEP-N Roberto Calabrese Dipartimento di Fisica and I.N.F.N. Ferrara, Italy.
Patrick Robbe, LAL Orsay, for the LHCb Collaboration, 16 December 2014
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
Peter Paul 12/16/06e-A Collider concept1 Brief History of the e-A Collider Concept Peter Paul BNL/SBU.
1 QM2006 D.I.Lowenstein RHIC : The Path Forward Presented to Quark Matter 2006 Shanghai, PRC Derek I. Lowenstein Brookhaven National Laboratory November.
1 Identified particle production in the Beam Energy Scan from STAR Anthony Timmins for the STAR Collaboration  The Beam energy scan  The STAR experiment.
RESEARCH POSTER PRESENTATION DESIGN © The RHIC Beam Energy Scan (BES) was proposed to search for the possible critical.
Nu Xu1/12 ”DNP“, Newport Beach, California, December , 2012 Energy Dependence of the High Moments from Transport Model Simulations Xiaofeng Luo.
1 Nov. 15 QM2006 Shanghai J.H. Lee (BNL) Nuclear Induced Particle Suppression at Large-x F at RHIC J.H. Lee Physics Department Brookhaven National Laboratory.
Study of hadron properties in cold nuclear matter with HADES Pavel Tlustý, Nuclear Physics Institute, Řež, Czech Republic for the HADES Collaboration ,
The Color Glass Condensate Outstanding questions: What is the high energy limit of QCD? How do gluons and quarks arise in hadrons? What are the possible.
An experimental perspective on first jet measurements at LHC: Lessons from RHIC Dan Magestro, The Ohio State University ALICE-USA Collaboration Meeting.
U N C L A S S I F I E D 7 Feb 2005 Studies of Hadronic Jets with the Two-Particle Azimuthal Correlations Method Paul Constantin.
Grazyna Odyniec STAR physics program and technical challenges with the RHIC Au+Au energy scan Grazyna Odyniec/LBNL for STAR collaboration QM 2008, Jaipur,
Higher moments of net-charge multiplicity distributions at RHIC energies in STAR Nihar R. Sahoo, VECC, India (for the STAR collaboration) 1 Nihar R. Sahoo,
Energy calibration at LHC J. Wenninger. Motivation In general there is not much interest for accurate knowledge of the momentum in hadron machines. 
Study the particle ratio fluctuations in heavy- ion collisions Limin Fan ( 樊利敏 ) Central China Normal University (CCNU) 1.
Slide 1 of 40 Brovko, Haag, Cebra January 06, 2011 LF Spectra Phone Conference STAR as a Fixed Target Experiment? Sam Brovko, Brooke Haag, Daniel Cebra.
Optimization of parameters for jet finding algorithm for p+p collisions at E cm =200 GeV T. G. Dedovich & M.V. Tokarev JINR, Dubna  Motivations.
Fixed Target Program in STAR Fixed-target running allows much higher rates without e-cooling at lower energies Top of  B range now ~ 400 MeV; extends.
October 14, 2004 Single Spin Asymmetries 1 Single Spin Asymmetries for charged pions. Overview  One physics slide  What is measured, kinematic variables.
1 Jeffery T. Mitchell – Quark Matter /17/12 The RHIC Beam Energy Scan Program: Results from the PHENIX Experiment Jeffery T. Mitchell Brookhaven.
Hadron Collider Physics 2012, 12/Nov/2012, KyotoShinIchi Esumi, Univ. of Tsukuba1 Heavy Ion results from RHIC-BNL ShinIchi Esumi Univ. of Tsukuba Contents.
Fiducial Cuts for the CLAS E5 Data Set K. Greenholt (G.P. Gilfoyle) Department of Physics University of Richmond, Virginia Goal: To generate electron fiducial.
Nucleon-Nucleon collisions. Nucleon-nucleon interaction at low energy Interaction between two nucleons: basic for all of nuclear physics Traditional goal.
Lecture 07: particle production in AA collisions
Robert Pak (BNL) 2012 RHIC & AGS Annual Users' Meeting 0 Energy Ro Robert Pak for PHENIX Collaboration.
Ivan Vitev & The First Precise Determination of Quark Energy Loss in Nuclei Ivan Vitev (PI), Ming Liu (Co-PI), Patrick McGaughey, Benwei Zhang T-16 and.
C H I C Charm in Heavy Ion SPS 1.J/  – Suppression in A+A 2.CHIC – Physics motivations 3.CHIC – Experimental aspects 1F. Fleuret - LLR.
ISMD 2004, Sonoma State University R. Muresan NBI BEC studies 1 Raluca Muresan NBI Copenhagen Bose-Einstein Correlation Studies at HERA-B.
The Color Glass Condensate and Glasma What is the high energy limit of QCD? What are the possible form of high energy density matter? How do quarks and.
Frictional Cooling A.Caldwell MPI f. Physik, Munich FNAL
Oct 論文セミナー. Abstract  Au+Au √s NN =62.4GeV  mid-rapidity, 7 centrality classes  m T spectra  dN/dy  energy dependence (SPS, AGS data)  yield.
K 0 S and  production at ZEUS, A. Savin, University of Wisconsin DIS 2006, April 22, K 0 S and  production at ZEUS Alexander A. Savin University.
Prospects for RHIC Low-Energy Operations Todd Satogata (W. Fischer, T. Roser, A. Fedotov, N. Tsoupas, M. Brennan, C. Montag, and others) “Can We Discover.
1 Charged hadron production at large transverse momentum in d+Au and Au+Au collisions at  s=200 GeV Abstract. The suppression of hadron yields with high.
QM2008 Jaipur, India Feb.4– Feb. 10, STAR's Measurement of Long-range Forward- backward Multiplicity Correlations as the Signature of “Dense Partonic.
High Density Matter and Searches for Huan Z. Huang Department of Physics and Astronomy University of California, Los Angeles The STAR Collaboration.
Hyperon Polarization in Heavy ion Collisions C. C. Barros Jr. Universidade Federal de Santa Catarina Brasil Strangeness in Quark Matter 2013 University.
Interactions with Rest Gas – Typical Case Interactions with Rest Gas – ELENA Quantitative analysis for ELENA Evaluations at 100 keV Ejection Energy Evaluations.
Diagnosing energy loss: PHENIX results on high-p T hadron spectra Baldo Sahlmüller, University of Münster for the PHENIX collaboration.
October 22, 2004 Single Spin Asymmetries at RHIC 1 F.Videbaek Physics Department, Brookhaven National.
24 June 2007 Strangeness in Quark Matter 2007 STAR 2S0Q0M72S0Q0M7 Strangeness and bulk freeze- out properties at RHIC Aneta Iordanova.
P.F.Ermolov SVD-2 status and experimental program VHMP 16 April 2005 SVD-2 status and experimental program 1.SVD history 2.SVD-2 setup 3.Experiment characteristics.
June 2009 H. Ströbele, Uni. Frankfurt Matter Effects at SPS energies What we can learn about stopping from the system size dependence of net.
The First Transverse Single Spin Measurement in High Energy Polarized Proton-Nucleus Collision at the PHENIX experiment at RHIC RIKEN/RBRC Itaru Nakagawa.
Past Fermilab Accumulator Experiments Antiproton Source Accumulator Ring (Inner Ring) Debuncher Ring (Outer Ring) AP50 Experiment Area PRECISION Precision.
Open and Hidden Beauty Production in 920 GeV p-N interactions Presented by Mauro Villa for the Hera-B collaboration 2002/3 data taking:
Kansas OCT 2004 Ramiro Debbe for the BRAHMS collaboration Physics Department BRAHMS Forward Physics Program Forward Physics at RHIC and LHC University.
Al+Au Analysis Plan Why study asymmetric systems like Al+Au (or Cu+Au as was recently done at RHIC)? Collisions of symmetric heavy ions do not create a.
EIC NAS review Charge-2 What are the capabilities of other facilities, existing and planned, domestic and abroad, to address the science opportunities.
Electromagnetic Physics Working Group discussion
Explore the new QCD frontier: strong color fields in nuclei
HADES The Baryon-rich Side of the Phase Diagram
EIC NAS review Charge-2 What are the capabilities of other facilities, existing and planned, domestic and abroad, to address the science opportunities.
Global Beam Energy Scan Global Beam Energy Scan
Tatsuya Chujo University of Tsukuba (for the PHENIX Collaboration)
Search for the onset of baryon anomaly at RHIC-PHENIX
The np -> d p0 reaction measured with g11 data
Presentation transcript:

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Exploring the Phase Diagram: The RHIC Contribution  RHIC is currently a unique facility for understanding the physics of high energy density, low net-baryon density, strongly- interacting matter.  RHIC could soon be one of several facilities for exploring the physics of a larger range of the phase diagram of strongly-interacting matter.  Both experimental and theoretical hints suggest that the additional regions of the QCD phase diagram may hold some intriguing new physics.  Not news to this audience…

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter  Old work of Busza and others on rapidity loss of leading baryon in p+A suggested that high(est??) baryon densities are created in collisions of beams around GeV on fixed targets.  AGS program also focused on high baryon density but may have had a tad too low beam energy. Motivation – I

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Motivation II – Gazdzicki QM04 Several other observables show similar non-monotonic behavior.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter What does it mean?  See other talks today…  I hope we all agree it is very interesting, whatever the explanation!

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter RHIC Beam Regions RHIC BEAM Fixed Here there be dragons RHIC BEAM Colliding

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter 20 o Experimental Phase Space Only need to measure on one side if symmetric 10 Y CM 10 Y CM o

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Low Energy Collider Mode??  In principle, RHIC can circulate and collide beams at below the normal injection energies.  AGS has experience running at lower energies.  Decelerating the beam may even be a possibility.  Would use existing experiments most efficiently. BUT…

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Low Energy Collider Mode??  May require significant machine development.  Certainly requires dedicated beam program.  If luminosity drops like 1/(Energy) 2, the rate could be a serious issue, requiring a long program.  Would still need “forward” angles. Reasonable coverage of rapidity distributions requires data down to  < ~10-20 o. BUT…

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter High Rapidity at RHIC  Same Physics??  At lower SPS energies, p/p ~ 0.05 or less.  At full RHIC Au+Au energies, p/p is still ~ 0.25 at rapidity as large as 3.  So, technically very challenging! but similar physics??

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter High Rapidity at RHIC  Same Physics??  Protons rising and antiprotons dropping fast so conditions are not stable over a broad region.  Out on the tails of the rapidity distributions where kinematics have a big effect.  K + and K  deviate already around rapidity of 2.  Saturation effects (CGC, etc) may strongly impact physics, especially particle production.  So, very interesting region to investigate but perhaps (probably??) not the same physics as midrapidity at  s NN ~4-10 GeV. BUT…

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Beam & Machine Issues  Effective beam current is frighteningly high.  0.7  10 9 ions/bunch  3  ions/second!  Beam loss cross sections are comparable to nuclear interaction cross sections so particle losses are of the same order as the data rate.  Only a very narrow beam region near 21.3 GeV is inaccessible to machine due to transition.  Some data near transition obtainable during ramp.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Target Options  Foil target: Would anything survive the beam?  Wire: Could be moving or located in halo.  Gas jet: Fairly standard technology but need to be careful about RHIC vacuum and choice of target material somewhat limited.  Ion beam: Might be possible due to huge effective beam current. Many advantages of control, choice of targets, local expertise.  Biggest design issue ($$$?) may be beam pipe.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Kaon Data Samples in Au+Au  Typical dN/dy values for kaons in the interesting energy regime are K  yield might be as low as 0.1 in region away from c.m. rapidity for non-central collisions at ~10 GeV beam energies.  With 1 million events, you don’t need much acceptance to get enough kaons to accurately determine the yield and slope.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Possible Running Modes  Dedicated running  With only 100 Hz DAQ, 1 million events takes < 3 hours. For 3 energies (10, 25, 40) and 8 spectrometer settings per energy (4 angles, 2 polarities), you need ~ 3 days.  Taking survey data during ramp  RHIC currently ramps 90 GeV in  5 min, so each ramp gives 17 seconds per 5 GeV bin in beam energy.  With 6 ramps per day, 200 Hz DAQ rate, and 6 weeks, data sample is almost 1 million events in each 5 GeV bin.  Slower ramping is possible.  Early proof-of-principle run mode?

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Fixed Target in ??  Sadly, probably not worth it, too bad…

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter 20

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Fixed Target in ?? 2.3  30 o 25  90 o

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Fixed Target in ??  Angular range and PID clearly not a problem!  Acceptance: Rough calculation of BRAHMS yield   (  /2  ) for both spectrometers are comparable and of the order of 0.5  1.5  10  3.  Even for dN/dy ~ 0.1, 1M events gives 100 particles.  Does not include full momentum acceptance, but not a big effect.  Modest data samples are probably adequate.  More realistic calculation clearly required.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Can RHIC compete with this:

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter The Ideal Solution??

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Comparing RHIC and NA49  Think complementarity, rather than competition.  Independent verification is crucial!  Multiple experiments a great strength at RHIC.  NA49 has a huge acceptance but smaller event samples (typically a few hundred thousand).  Much easier at RHIC to do many energies quickly.  With a modest effort, an initial survey energy scan could be very competitive with existing NA49 data.

17-Nov-2004G.S.F.Stephans Exploring the Phase Diagram of Strongly Interacting Matter Closing Thoughts  RHIC can make an important contribution to the exploration of this exciting new regime.  A first survey program could be done with a modest investment of time and money.  Some early data could be taken during ramping the beam energy in normal collider operations.  I look forward to an exciting program at a multitude of locations!