RHIC Detector Upgrades Science, Scope, Strategy T. Ludlam New Frontiers at RHIC Oct. 30, 2005.

Slides:



Advertisements
Similar presentations
CMS Heavy Ion Physics Edwin Norbeck University of Iowa.
Advertisements

Determination of the gluon polarisation at COMPASS & RHIC Sébastien Procureur (CEA - Saclay) Determination of  G at COMPASS & RHICPAVI06, Milos S.Procureur.
PHENIX Decadal Plan o Midterm upgrades until 2015 o Long term evolution after 2015 Dynamical origins of spin- dependent interactions New probes of longitudinal.
Centauro and STrange Object Research (CASTOR) - A specialized detector system dedicated to the search for Centauros and Strangelets in the baryon dense,
Jin Huang Brookhaven National Lab For the PHENIX Collaboration A MERICAN P HYSICAL S OCIETY A PRIL M EETING, A PRIL 13, 2015, B ALTIMORE, M ARYLAND Outline:
Axel Drees, Stony Brook University Rutgers NJ, January High T QCD at RHIC: Hard Probes Fundamental open questions for high T QCD Nature of matter.
04/11/2008Lijuan Ruan (WWND2008)1 Prototype Performance of Novel Muon Telescope Detector at STAR Outline: Motivation Simulation Intrinsic timing and spatial.
March 1, 2003University of Rochester - Graduate Student Days1 Nuclear Physics at the University of Rochester Steven Manly Grad. Student Days March 1, 2003.
The Physics Potential of the PHENIX VTX and FVTX Detectors Eric J. Mannel WWND 13-Apr-2012.
Sourav Tarafdar Banaras Hindu University For the PHENIX Collaboration Hard Probes 2012 Measurement of electrons from Heavy Quarks at PHENIX.
Thomas Roser RHIC Open Planning Meeting December 3-4, 2003 RHIC II machine plans Electron cooling at RHIC Luminosity upgrade parameters.
Output from this Series of Workshops: A science vision for the RHIC future 1.Provide a science case for the future RHIC program that makes clear its importance.
Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab The Relativistic Nuclear Collisions (RNC) group.
RHIC program and machine performances Hugo Pereira Da Costa, CEA Saclay, PHENIX Collaboration, 3 Juillet 2006.
Recent Results from STAR: Correlations James C. Dunlop Brookhaven National Laboratory for the STAR Collaboration March 20, J.C. Dunlop, Moriond.
RHIC R.K. CHOUDHURY BARC. Relativistic Heavy Ion Collider at Brookhaven National Laboratory (BNL), USA World’s First Heavy Ion Collider became.
Frontiers of Nuclear Physics A Personal Outlook Huan Zhong Huang Department of Physics and Astronomy University of California, Los Angeles Department of.
Sean Kelly, QWG 9/03 Prospects for Quarkonia Physics In Media at the LHC.
Thomas Roser NSAC subcommittee April 4, 2005 Facility Strategy RHIC performance overview Luminosity and polarization evolution (towards “enhanced luminosity”)
1 QM2006 D.I.Lowenstein RHIC : The Path Forward Presented to Quark Matter 2006 Shanghai, PRC Derek I. Lowenstein Brookhaven National Laboratory November.
HFT + TOF: Heavy Flavor Physics Yifei Zhang University of Science & Technology of China Lawrence Berkeley National Lab TOF Workshop, Hangzhou, April,
Axel Drees, Stony Brook University RHIC II workshop, BNL, November 19, 2004 Decadal Plan PHENIX Decadal Plan Presented at open meeting and to.
Jim Thomas - LBL 1 News about RHIC with comments about PHOBOS, BRAHMS and the Upgrade Plans for STAR and PHENIX Jim Thomas Lawrence Berkeley National Laboratory.
Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab The Relativistic Nuclear Collisions (RNC) group.
Brookhaven Science Associates The Future of RHIC Quark Matter 2005, Budapest Samuel Aronson, BNL August 8, 2005 ► Past & present – ► Near-term.
Small x issues in nucleon spin structure (focus: polarized gluon distribution) Abhay Deshpande Stony Brook University RIKEN BNL Research Center December.
Office of Science U.S. Department of Energy RHIC Users Meeting BNL; June 8, 2006 Gulshan Rai RHIC/AGS Users Meeting Gulshan Rai Program Manager for Heavy.
Thomas Roser Snowmass 2001 June 30 - July 21, 2001 Polarized Proton Acceleration and Collisions Spin dynamics and Siberian Snakes Polarized proton acceleration.
Nu Xu1/16STAR Collaboration Meeting, Nov. 12 – 17, 2010, BNL, USA STAR Experiment at RHIC: - Physics Programs - Management Issues Nu Xu.
STAR Spin Related Future Upgrades STAR Spin Physics Program Current Capabilities Heavy Flavor Physics W Program Transverse Program Upgrades: Plans & Technologies.
Spin Physics with PHENIX (an overview, but mainly  G) Abhay Deshpande Stony Brook University RIKEN BNL Research Center July 28, 2011.
Proton-Proton Elastic Scattering at RHIC
Axel Drees, University Stony Brook Washington DC, December High T and  QCD in the BNL QCD Lab Era Introduction QCD phase diagram Status of heavy.
The W program at PHENIX R. Seidl (University of Illinois and RBRC) for the PHENIX Collaboration Workshop on Parity Violating Spin Asymmetries BNL, April.
Axel Drees, Stony Brook University NSAC subcommittee meeting, Bethesda, April 4, 2005 Detector Strategy What I will talk about: The Goals of Upgrades:
ERHIC with Self-Polarizing Electron Ring V.Ptitsyn, J.Kewisch, B.Parker, S.Peggs, D.Trbojevic, BNL, USA D.E.Berkaev, I.A.Koop, A.V.Otboev, Yu.M.Shatunov,
S. Esumi, sPHNIX for US-J, 21/Dec/2011, KEK1 1. New questions and needs 2. sPHENIX concept and acceptance 3. soft physics and thermal photons 4. critical.
Axel Drees, Stony Brook University BNL review of RHIC detector upgrades, March 14 th 2006 Overview of PHENIX upgrades Goals of PHENIX upgrades program.
 Big questions  why are quarks confined inside protons ? artist’s view :)  what does the vacuum look like ?  can we use understanding.
RHIC Mid-Term Strategic Plan Science Outlook, Upgrades, Resources T. Ludlam, July 24, 2006 QCD Collider Laboratory Mid Term Plan Brookhaven Science Associates.
Nu Xu1/20STAR Regional Meeting, VECC, India, November, 2008 STAR Experiment STAR at RHIC Nu Xu Lawrence Berkeley National Laboratory.
High Density Matter and Searches for Huan Z. Huang Department of Physics and Astronomy University of California, Los Angeles The STAR Collaboration.
Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab The Relativistic Nuclear Collisions (RNC) group.
Dec 2002 Craig Ogilvie 1 Physics Goals of Si Vertex Detector  Physics priorities latter part of this decade –spin carried by gluons:  G vs x –modification.
PHENIX FUTURE PLANS & UPGRADES Stefan Bathe for PHENIX, Users’ Meeting 2009.
Nu Xu1/7STAR Analysis Meeting, Junior Meeting, April 16 th, 2012, BNL STAR STAR Experiment Nu Xu - Introduction: Structure of the QCD Matter - Near future.
Craig Ogilvie1 Silicon Vertex Upgrade for PHENIX  A+A: from discovery to characterizing properties dense phase – Need broad range of early probes: charm,
1 RHIC II – Ion Operation Wolfram Fischer RHIC II Workshop, BNL – Working Group: Equation of State 27 April 2005.
Spin Physics with PHENIX (an overview, but mainly  G) Abhay Deshpande Stony Brook University RIKEN BNL Research Center PANIC’11 at MIT July 28, 2011.
Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab Large Hadron Collider (LHC) Spin physics program.
International Workshop on Radiation Imaging Detectors, Glasgow, July 25-29, 2004 Johann M. Heuser, RIKEN for the PHENIX Collaboration - RHIC and PHENIX.
1 Machine issues for RHIC II Wolfram Fischer PANIC Satellite Meeting – New Frontiers at RHIC 30 October 2005.
Overview of the sea quark polarization measurements of PHENIX at RHIC DIS April 12, Rusty Towell Abilene Christian University on behalf of the PHENIX.
Brookhaven Science Associates U.S. Department of Energy BNL’s Plans for RHIC Detector Advisory Committee December 19, 2002 T. Ludlam.
Axel Drees, SUNY Stony Brook GSI, May January 15 th 2002 PHENIX Upgrade Plans for RHIC II Overview of baseline PHENIX detector Physics goals of RHIC II.
From RHIC to eRHIC E.Kistenev XIX International Baldin Seminar, Dubna, 2008.
Extending the PHENIX physics reach Physics beyond the baseline accessible at RHIC II Capabilities needed to address the new physics Detector upgrades to.
RHIC Detector Upgrades S. Aronson 8/5/02. From the RHIC Program Review Close-out: 2) Plans for upgrading the RHIC Facility The RHIC physics program is.
11 Nov J. Schukraft1 Future of Heavy SPS/RHIC programs SPS/RHIC programs Initial LHC Program Initial LHC Program  ~ 2017 Long.
RHIC Update & Future Program
Silicon Pixel Detector for the PHENIX experiment at the BNL RHIC
Explore the new QCD frontier: strong color fields in nuclei
Future upgrades of PHENIX
eRHIC with Self-Polarizing Electron Ring
PheniX, STAr AND AN EIC E.C. Aschenauer
Heavy Ion Physics in RUN14-16
Transverse Spin Physics at PHENIX
ShinIchi Esumi, Univ. of Tsukuba
Transverse Spin Physics at RHIC II
Presentation transcript:

RHIC Detector Upgrades Science, Scope, Strategy T. Ludlam New Frontiers at RHIC Oct. 30, 2005

The RHIC Detectors

RHIC polarized proton accelerator complex BRAHMS STAR PHENIX AGS LINAC BOOSTER Pol. H - Source Spin Rotators (longitudinal polarization) Solenoid Partial Siberian Snake Siberian Snakes 200 MeV Polarimeter AGS Internal Polarimeter Rf Dipole RHIC pC Polarimeters Absolute Polarimeter (H  jet) AGS pC Polarimeters Strong Helical AGS Snake Helical Partial Siberian Snake PHOBOS Spin Rotators (longitudinal polarization) Spin flipper Siberian Snakes

Summary of RHIC Runs 1-5 Delivered Luminosity; Physics Weeks Note: delivered Lum. is summed over all expts.

Four experiments: BRAHMS, PHENIX, PHOBOS, STAR Complementarity and concordance among their results is a hallmark of the program Tremendous scientific impact Hundreds of publications; thousands of citations 3- year retrospective “white papers” published by each of the 4 experiments Major discoveries have changed the view of high energy nuclear physics: Jet Quenching Gluon saturation/Color Glass Indications “Near-Perfect-Liquid” behavior Significant experimental advances Hard Scattering Auto-generated probes Fully calibrated comparison data p-p, d-Au, Au-Au under identical conditions First high energy polarized proton collider Major Achievements with RHIC present

The Big Questions QCD at High Temperature and Density: What are the properties of quark-gluon matter above T C ? Is chiral symmetry restored? Viscosity? Conductivity? What is the physics of superdense, strongly-interacting matter? QCD at High Energy and low x: Is the initial state a Color Glass Condensate? What is the physics of strong color fields? QCD and the structure of hadrons: What is the origin of nucleon spin? RHIC II Science Working Groups: RHIC II Science Workshop Nov

Where do We Go from Here… Key Measurements Hard Probes: created early in the collision and propagate through the medium. Their interactions with the medium help characterize its properties High Pt particles and jet fragmentation Heavy quarkonia (J/ ,  ’,  c and Upsilon (1s, 2s, 3s) Open charm and bottom Electromagnetic Probes: direct information from the medium Low-mass e + e - pairs and Thermal radiation Polarized proton collisions: W-production at s 1/2 = 500 GeV for sea quark flavor selection Facility Operation Systematic species and energy scans This has proved crucial! Balance of Running RHIC and investing in upgrades

Where Do We Stand Now? Four Detectors Two Large Detectors Machine Goals for Next Few Years: Enhanced Ion luminosity (112 bunches,  * = 1m): 2x achieved Au – Au: 8  cm -2 s -1 (100 GeV/nucleon) For protons: 2  protons/bunch (no IBS): 6x achieved 150  cm -2 s -1 ; 70 % polarization (250 GeV) Spin Program poised for definitive measurements: EBIS Construction funded in FY Operational in 2010 Short-term detector upgrades underway Significant funding from NASA

RHIC II Luminosity Upgrade with Electron Cooling Gold collisions (100 GeV/n x 100 GeV/n): w/o e-coolingwith e-cooling Ave. store luminosity [10 26 cm -2 s -1 ] 8 70 Pol. Proton Collision (250 GeV x 250 GeV): Ave. store luminosity [10 32 cm -2 s -1 ] LinacRf Gun Buncher Cavity Cooling Solenoid (26 m, 2-5 T) Debuncher Cavity e-Beam Dump Gold beam R&D in Progress: proof-of-principle expected in 2006

A Long Term Strategic View RHIC RHIC II Construction RHIC Spin eRHIC Constr. Short term upgrades Midterm Upgrades ~ Luminosity & Det. upgrade E beam + new detector LHC Heavy Ion

The Mid-Term Challenge Extend the reach of the RHIC facility to address key questions in the coming 5-6 years… Requires improved machine performance and significant running time Requires enhanced capability for PHENIX and STAR Complement the early results from LHC Heavy Ion running Set the stage for RHIC II

Major Physics Measurements Required Upgrades Spin: Complete initial  G/G measurement No upgrades needed Transversity measurement Forward particle measurement W measurements at 500 GeV Forward tracking/triggering in PHENIX and STAR Heavy Ion: e-pair mass spectrum “Hadron Blind” Dalitz pair rejection Open charm measurements in AA High Resolution vertex detection Charmonium Spectroscopy High luminosity; precision vertex, particle ID Jet Tomography High luminosity; High-rate DAQ; particle ID Monojet in d-Au particle detection at forward rapidity * DOE performance milestones set by NSAC PM: 2010 PM: 2012 PM: 2008 PM: 2013

 e + e -    e + e - S/B ~ 1/500 “combinatorial pairs” total background Irreducible charm background all signal charm signal signal electron Cherenkov blobs partner positron needed for rejection e+e+ e-e-  pair opening angle Full scale prototype Low-Mass e + e - Pairs A Hadron-Blind detector for PHENIX ~ 1 m Engineering run FY 06 Operational FY 07

Flavor tagging at large P T MRPC Time of Flight Barrel in STAR Construction FY 06 – FY 08 23,000 channels covering TPC & Barrel Calorimeter Significant contribution from China

Precision Vertex Detectors Direct Observation of Charm and Beauty PHENIX VTX: Barrel– 4 layers, Si pixels and strips End Caps: 4 layers Si mini-strips STAR Heavy Flavor Tracker: 2 layers CMOS Active Pixel sensors Significant funding from Japan

Low-x Physics: Color Glass; gluon density Forward Upgrades.001 < x < 0.1 in Au-Au, d-Au PHENIX: Nose Cone CalorimeterSTAR: Forward Meson Spectrometer

W Physics Upgrades STAR Forward Tracking Upgrade Heavy Flavor Tracker Inner Silicon Tracker Forward Silicon Tracker GEM layer on endcap PHENIX Muon Trigger Resistive Plate Chambers Funded by NSF

FY 2006FY 2007FY 2008FY 2009FY 2010FY 2011FY 2012 High statistics Au Au; 500 GeV Spin Runs Short-term upgrades: HBD, TOF, DAQ, FMS, Muon Trigger Mid-Term Upgrades: Vtx detectors, NCC, forward tracking RHIC II Construction Machine and detector R&D; continued luminosity improvements A timeline for physics operation, detector upgrades, machine evolution LHC Heavy Ion Program pp 200 Ion Run? Ion scan pp 200 d-Au 200 pp 200/500

RHIC II FY 2006FY 2007FY 2008FY 2009FY 2010FY 2011FY 2012FY 2013 RHIC Mid-Term Strategic Plan L HI LP 4 RHIC II CD-0 CD-1 CD-2 CD-3 CD-4 PHENIX + STAR Hi Rate DAQ 1000 PID HBD TOF VTX Forward FMS Mu Trigger Nose Cone Calorimeter EBIS Heavy Ion Luminosity SPIN F.O.M. e-pair spectrum Open Charm Jet Tomography Mono-Jet U+U PHENIXSTAR  G/G Transversity and P-V W ± prod. PHENIX & STAR VTX upgrades STAR forward tracking

Will there be a major New Detector for RHIC II? This is not part of the mid-term plan Plans are afoot for a dedicated new detector for eRHIC It is very possible, even likely, that the “QCD Lab” will require a new detector to exploit HI collisions in the eRHIC era.

The Long Term Vision: RHIC as a QCD Laboratory eRHIC: DIS at collider energies e-A at 63 GeV/u Polarized e-p at 100 GeV L ~ cm -2 sec -1 RHIC Spin: Strongly interacting probes A-A: QGP physics at RHIC II luminosities

Realizing the Vision: Mid Term View Phased implementation of key upgrades for PHENIX and STAR, plus EBIS, over the next 5-6 years. Annual data runs during this period will exploit these upgrades for critical advances in the Heavy Ion and Spin physics programs— Along with continued improvements in machine performance. With the help of funding and collaborative resources outside of DOE, this strategy appears possible within a “constant effort” budget scenario based on FY 05 levels. Two large detectors well equipped for RHIC II physics Fast-track RHIC II luminosity upgrade (e-cooling) along technically-driven schedule Success will require a concerted effort to define and focus the science objectives