RHIC Physics and the importance of particle identification R. Bellwied (Wayne State University)

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

Elliptic flow of thermal photons in Au+Au collisions at 200GeV QNP2009 Beijing, Sep , 2009 F.M. Liu Central China Normal University, China T. Hirano.
Supported by DOE 11/22/2011 QGP viscosity at RHIC and LHC energies 1 Huichao Song 宋慧超 Seminar at the Interdisciplinary Center for Theoretical Study, USTC.
1 Jet Structure of Baryons and Mesons in Nuclear Collisions l Why jets in nuclear collisions? l Initial state l What happens in the nuclear medium? l.
The Phase Diagram of Nuclear Matter Oumarou Njoya.
The Color Glass Condensate and RHIC Phenomenology Outstanding questions: What is the high energy limit of QCD? How do gluons and quarks arise in hadrons?
Heavy Quark Probes of QCD Matter at RHIC Huan Zhong Huang University of California at Los Angeles ICHEP-2004 Beijing, 2004.
Forward-Backward Correlations in Relativistic Heavy Ion Collisions Aaron Swindell, Morehouse College REU 2006: Cyclotron Institute, Texas A&M University.
The Quark Gluon Plasma what is it and why should it exist ?
Relativistic Heavy-Ion Collisions: Recent Results from RHIC David Hardtke LBNL.
24/04/2007ALICE – Masterclass Presentation1 ALICE Hannah Scott University of Birmingham.
Quark recombination in high energy collisions for different energies Steven Rose Worcester Polytechnic Institute Mentor: Dr. Rainer Fries Texas A&M University.
Forward-Backward Correlations in Heavy Ion Collisions Aaron Swindell, Morehouse College REU Cyclotron 2006, Texas A&M University Advisor: Dr. Che-Ming.
We distinguish two hadronization mechanisms:  Fragmentation Fragmentation builds on the idea of a single quark in the vacuum, it doesn’t consider many.
200 GeV Au+Au Collisions, RHIC at BNL Animation by Jeffery Mitchell.
1 The Quark Gluon Liquid The AIP Science Story of 2005 R. Bellwied for the WSU RHIC group WSU Physics Colloquium 12-Dec-2005.
1 Particle production mechanisms from RHIC to LHC Rene Bellwied Wayne State University 23 rd International Winter Workshop on Nuclear Dynamics, Big Sky.
Finite Size Effects on Dilepton Properties in Relativistic Heavy Ion Collisions Trent Strong, Texas A&M University Advisors: Dr. Ralf Rapp, Dr. Hendrik.
Intro to Particle and Nuclear Physics and the Long Island Gold Rush Steven Manly Univ. of Rochester REU seminar June 1, 2006
1 ALICE Status Orlando Villalobos Baillie University of Birmingham NuPECC Meeting Edinburgh 10 th October 2014.
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
John Chin-Hao Chen1 Quark Gluon Plasma: the Hottest Matter on Earth John Chin-Hao Chen ( 陳勁豪 ) RIKEN Brookhaven Research Center Brookhaven National.
New States of Matter and RHIC Outstanding questions about strongly interacting matter: How does matter behave at very high temperature and/or density?
1 The Quark Gluon Plasma and the Perfect Fluid Quantifying Degrees of Perfection Jamie Nagle University of Colorado, Boulder.
Frontiers of Nuclear Physics A Personal Outlook Huan Zhong Huang Department of Physics and Astronomy University of California, Los Angeles Department of.
Discovery of the Higgs Boson Gavin Lawes Department of Physics and Astronomy.
Helen Caines Yale University Yale Colloquium – April 2006 Sampling the flavor of the Quark-Gluon Plasma. QGP – Phase of matter where quark and gluons are.
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.
Complex Plasmas as a Model for the Quark-Gluon-Plasma Liquid
Jet quenching and direct photon production F.M. Liu 刘复明 Central China Normal University, China T. Hirano 平野哲文 University of Tokyo, Japan K.Werner University.
High Energy Nuclear Physics and the Nature of Matter Outstanding questions about strongly interacting matter: How does matter behave at very high temperature.
09/15/10Waye State University1 Elliptic Flow of Inclusive Photon Ahmed M. Hamed Midwest Critical Mass University of Toledo, Ohio October, 2005 Wayne.
MA Lisa - Sambamurti Lecture, BNL - 28 Jul Size Matters Spacetime geometry in subatomic collisions Mike Lisa The Ohio State University  What is.
High Pt physics with TOF ALICE B.V.Zagreev ITEP
Relativistic Heavy Ion Collider and Ultra-Dense Matter.
Hadron Collider Physics 2012, 12/Nov/2012, KyotoShinIchi Esumi, Univ. of Tsukuba1 Heavy Ion results from RHIC-BNL ShinIchi Esumi Univ. of Tsukuba Contents.
Quark-Gluon Plasma Sijbo-Jan Holtman.
Physics of Dense Matter in Heavy-ion Collisions at J-PARC Masakiyo Kitazawa J-PARC 研究会、 2015/8/5 、 J-PARC.
QuarkNet 2006 Lets go smash some Atoms! Peripheral Collision:Central Collision Head-On Collision: Largest # of Nucleons Participate Glancing Collision:
Presentation for NFR - October 19, Trine S.Tveter Recent results from RHIC Systems studied so far at RHIC: - s NN 1/2 = 
 Big questions  why are quarks confined inside protons ? artist’s view :)  what does the vacuum look like ?  can we use understanding.
Heavy Ion Physics at the LHC & RHIC - Recreating the Big Bang in the Laboratory Rene Bellwied (for the Bellwied/Pinsky group) University of Houston
1 Tatsuya Chujo Univ. of Tsukuba Hadron Physics at RHIC HAWAII nd DNP-APS/JPS Joint Meeting (Sep. 20, 2005)
John Harris (Yale) LHC Conference, Vienna, Austria, 15 July 2004 Heavy Ions - Phenomenology and Status LHC Introduction to Rel. Heavy Ion Physics The Relativistic.
Heavy Ions at the LHC Theoretical issues Super-hot QCD matter What have we learned from RHIC & SPS What is different at the LHC ? Goals of HI experiments.
Heavy-Ion Physics - Hydrodynamic Approach Introduction Hydrodynamic aspect Observables explained Recombination model Summary 전남대 이강석 HIM
High-p T Particles and RHIC Paradigm of Jet Quenching Ahmed M. Hamed NN2012 The 11 th International Conference on Nucleus-Nucleus Collisions 1.
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.
News from ALICE Jan PLUTA Heavy Ion Reaction Group (HIRG) Warsaw University of Technology February 22, XIII GDRE Workshop, SUBATECH, Nantes.
The Quark-Gluon Plasma Marco van Leeuwen. 2 Elementary particles Atom Electron elementary, point-particle Protons, neutrons Composite particle  quarks.
Roy A. Lacey, Stony Brook, ISMD, Kromĕříž, Roy A. Lacey What do we learn from Correlation measurements at RHIC.
Results from ALICE Christine Nattrass for the ALICE collaboration University of Tennessee at Knoxville.
24 Nov 2006 Kentaro MIKI University of Tsukuba “electron / photon flow” Elliptic flow measurement of direct photon in √s NN =200GeV Au+Au collisions at.
1 Probing dense matter at extremely high temperature Rudolph C. Hwa University of Oregon Jiao Tong University, Shanghai, China April 20, 2009.
New Physics at the Relativistic Heavy Ion Collider Associate Professor Jamie Nagle University of Colorado at Boulder XXXIV SLAC Summer Institute July 17-28,
Intermediate pT results in STAR Camelia Mironov Kent State University 2004 RHIC & AGS Annual Users' Meeting Workshop on Strangeness and Exotica at RHIC.
Elliptic Flow of Inclusive Photon Elliptic Flow of Inclusive Photon Ahmed M. Hamed Midwest Critical Mass University of Toledo, Ohio Oct. 22,
What have we learned from the RHIC experiments so far ? Berndt Mueller (Duke University) KPS Meeting Seoul, 22 April 2005.
Quark Gluon Plasma Presented by: Rick Ueno Welcome to the presentation of:
Elliptic flow from initial states of fast nuclei. A.B. Kaidalov ITEP, Moscow (based on papers with K.Boreskov and O.Kancheli) K.Boreskov and O.Kancheli)
Review of ALICE Experiments
The 'Little Bang’ in the Laboratory - Physics at the LHC
Strangeness Production in Heavy-Ion Collisions at STAR
Probing Quark Matter in the PHENIX Experiment at RHIC
QCD (Quantum ChromoDynamics)
STAR and RHIC; past, present and future.
Institute of Particle Physics Huazhong Normal University
QGP at RHIC: Seen through Modified Jet Fragmentation
of Hadronization in Nuclei
Introduction of Heavy Ion Physics at RHIC
Presentation transcript:

RHIC Physics and the importance of particle identification R. Bellwied (Wayne State University)

Did we serve up the perfect liquid ? (The AIP Science Story of 2005) “The truly stunning finding at RHIC that the new state of matter created in the collisions of gold ions is more like a liquid than a gas gives us a profound insight into the earliest moments of the universe. The possibility of a connection between string theory, cosmology and RHIC collisions is unexpected and exhilarating. It may well have a profound impact on the physics of the twenty-first century.” said Dr. Raymond L. Orbach, Director of the DOE Office of Science. “Once again, the physics research sponsored by the Department of Energy is producing historic results,” said Secretary of Energy Samuel Bodman. “The DOE is the principal federal funder of basic research in the physical sciences, including nuclear and high-energy physics. With today’s announcement we see that investment paying off.”

Strong color field Force grows with separation !!! Analogies and differences between QED and QCD to study structure of an atom… “white” proton …separate constituents Imagine our understanding of atoms or QED if we could not isolate charged objects!! nucleus electron quark quark-antiquark pair created from vacuum “white” proton (confined quarks) “white”  0 (confined quarks) Confinement: fundamental & crucial (but not understood!) feature of strong force - colored objects (quarks) have  energy in normal vacuum neutral atom To understand the strong force and the phenomenon of confinement: Create and study a system of deconfined colored quarks (and gluons)

Generating a deconfined state Nuclear Matter (confined) Hadronic Matter (confined) Quark Gluon Plasma deconfined ! Present understanding of Quantum Chromodynamics (QCD) heating compression  deconfined color matter !

Expectations from Lattice QCD  /T 4 ~ # degrees of freedom confined: few d.o.f. deconfined: many d.o.f. T C ≈ 173 MeV ≈ 2  K ≈ 130,000  T[Sun’s core]  C  0.7 GeV/fm 3

The phase diagram of QCD Temperature baryon density Neutron stars Early universe nuclei nucleon gas hadron gas colour superconductor quark-gluon plasma TcTc 00 critical point ? vacuum CFL

RHIC BRAHMS PHOBOS PHENIX STAR AGS TANDEMS Relativistic Heavy Ion Collider (RHIC) 1 km v =  c  s NN =200 GeV

Study all phases of a heavy ion collision If the QGP was formed, it will only live for s !!!! BUT does matter come out of this phase the same way it went in ???

microexplosionsfemtoexplosions ss0.1  J 1  J  J/m 3 5 GeV/fm 3 = J/m 3 T10 6 K200 MeV = K rate10 18 K/s10 35 K/s

The STAR Experiment 450 scientists from 50 international institutions Conceptual Overview

Actual Collision in STAR TPC QGP signatures: strangeness enhancement, early collectivity partonic degrees of freedom, energy loss in medium

Strangeness yields from pp to AA Production not well modeled by N part (correlation volume) Canonical suppression increases with increasing strangeness  and  are not flat

Elliptic (anisotropic) flow – a strong indicator of early collectivity Dashed lines: hard sphere radii of nuclei Reaction plane In-plane Out-of-plane Y X Flow Y X Time Directed flowElliptic flow

Elliptic flow described by fluid dynamics

Kink analysis in STAR Λ->p+π(64%) Charged -> positive+negative (V0) K  μν (63%) K  ππ0 (21%) Charged -> charged + neutral (Kink)  = baryon (q-q-q) = u-d-s K = meson (q-qbar) = ubar-s or u-sbar

Constituent quarks might be relevant

Fate of jets in heavy ion collisions? p p ? Au+Au idea: p+p same  s NN = 200 GeV as reference ?: what happens in Au+Au to jets which pass through medium? Prediction: scattered quarks radiate energy (~ GeV/fm) in the colored medium:  decreases their momentum (fewer high p T particles)  “kills” jet partner on other side

High pt suppression at RHIC strange R CP well behaved all particles have same R CP for p T >~5 GeV: dominance of fragmentation? no flavor dependence in fragmentation region ?

An unexpected liquid phase with very drastic thermodynamic properties ? The ideal liquid requires very strong interaction cross sections, vanishing mean free path and sudden thermalization (in less than 1 fm/c). Perturbative calculations of gluon scattering lead to long equilibration times (> 2.6 fm/c) and very small v2 The state above T c can not be simple mass less partons = constituent quarks liquid ? Liquid

A novel ideal liquid behavior First time in Heavy-Ion Collisions a system created which, at low p t,is in quantitative agreement with ideal hydrodynamic model. The new phase behaves like an ideal liquid. But are the degrees of freedom partonic ?

400 times less viscous than water,10 times less viscous than superfluid helium ! ? An example: lower viscosity bound in strong quantum field theory Motivated by calculation of lower viscosity bound in black hole via supersymmetric N=4 Yang Mills theory in AdS (Anti deSitter) space (conformal field theory)

An example: thermalization through Hawking mechanism Black holes emit thermalized Hawking radiation due to strongly varying accelerator gradients on both sides of the event horizon (splitting of e+e- pair from virtual photons). RHIC collisions might have black-hole like gradients due to very different gluon densities inside and outside the fireball (leads to  -gradients). This might explain sudden thermalization

We have successfully created the Quark Gluon Plasma, an early universe phase of matter, which might still exist in black holes. Surprisingly it behaves like a perfect liquid !! Now we need to understand its exciting properties: low viscosity rapid equilibration (thermalization) novel hadron formation mechanisms jet quenching and medium reaction temperature determination degrees of freedom Conclusions

The future is bright A three prong approach: improved facility expanded facility higher energy LHC ( ?): Large Hadron Collider with ALICE, CMS, ATLAS heavy ion programs RHIC-II ( ): Upgrades to STAR & PHENIX EoS of sQGP QCD, CGC, QGP wQGP (?) QCDLab ( ): A high luminosity RHIC with eA and AA detectors AGS BOOSTER RHIC e- cooling LINAC EBIS recirculating linac injector 5-10 GeV static electron ring