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

2. The RHIC Detectors

3. 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

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

5. 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 2001 - present

6. 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: www.bnl.gov/physics/rhicIIscience RHIC II Science Workshop Nov. 11-12

7. 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

8. 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  10 26 cm -2 s -1 (100 GeV/nucleon) For protons: 2  10 11 protons/bunch (no IBS): 6x achieved 150  10 30 cm -2 s -1 ; 70 % polarization (250 GeV) Spin Program poised for definitive measurements: EBIS Construction funded in FY 2006. Operational in 2010 Short-term detector upgrades underway Significant funding from NASA

9. 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 ] 1.5 5.0 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

10. A Long Term Strategic View RHIC RHIC II Construction RHIC Spin eRHIC Constr. Short term upgrades Midterm Upgrades ~2012 2008 Luminosity & Det. upgrade E beam + new detector LHC Heavy Ion

11. 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

12. 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

13.  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

14. 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

15. 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

16. 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

17. 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

18. 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

19. 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

20. 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.

21. 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 ~ 10 33 cm -2 sec -1 RHIC Spin: Strongly interacting probes A-A: QGP physics at RHIC II luminosities

22. 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