Thomas Roser NSAC subcommittee April 4, 2005 Facility Strategy RHIC performance overview Luminosity and polarization evolution (towards “enhanced luminosity”)

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Presentation transcript:

Thomas Roser NSAC subcommittee April 4, 2005 Facility Strategy RHIC performance overview Luminosity and polarization evolution (towards “enhanced luminosity”) Future upgrades EBIS RHIC luminosity upgrade eRHIC

Gold Ion Collisions in RHIC RHIC AGS BOOSTER TANDEMS 9 GeV/u Q = MeV/u Q = +32 Beam Energy = 100 GeV/u

RHIC Au-Au performance – 2 x design luminosity Injector RHIC design luminosity Luminosity [x10 26 ]

RHIC Run 5 Delivered Cu-Cu Luminosity

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

New AGS helical snakes 2.6 m 30% s.c. helical snake build at BNL SMD Installed in March 2005  Warm snake avoids polarization mismatch at AGS injection and extraction.  Cold strong snake eliminates all depolarizing resonances in AGS. 5 % helical snake build at Tokana Industries funded by RIKEN.

Siberian Snake in RHIC Tunnel Siberian Snake: 4 superconducting helical dipoles, 4Tesla, 2.4 m long with full 360  twist Funded by RIKEN, Japan Designed and constructed at BNL

Polarization survival in RHIC 06:0007:0008:0009:0010:0011: % Polarization Luminosity cm -2 s -1 Protons x Spin rotator rampAcceleration and squeeze ramp

RHIC – a Uniquely Flexible High Luminosity Collider (Nucleon-pair luminosity A 1 A 2 L allows comparison of different species) Luminosity increased by 2 orders of magnitude in 4 years.

RHIC Accelerator Complex Operations 7 major accelerator systems (2 Tandems, Linac, Booster, AGS, 2 RHIC rings) consisting of: l 6 miles of evacuated beam lines (large part of it below Torr) l 4.5 miles of superconducting magnets and cryostat l 25 He refrigerator (12 turbines, 25 compressors,…) l 2 rapid cycling synchrotrons (  16 MW and  40 MW power supplies) l 42 high power rf systems (0.1 – 200 MHz) l 1300 programmable DC power supplies l 54 pulsed power systems FY05 operations budget ($95M, equal to the recommendation of $95M [2005$] from 2002 RHIC operations review) is sufficient for safe and efficient operation of 31 cryo- weeks with excellent availability. Ongoing investment to improve operating efficiency (cryo upgrade: 2 MW reduction of el. power consumption, EBIS)

RHIC availability and time in store  Excellent availability despite very complex operation modes.  Machine set-up time reduced to just 3 weeks. FY05Q2 Weekly Availability

Major contributions from non-DOE sources to the RHIC accelerator complex: RIKEN, Japan: RHIC Spin (~ $70M, RBRC) NASA: NASA Space Radiation Laboratory ($4.5M contribution to EBIS) NSF and Canada: RSVP (construction not started yet, major infrastructure upgrade to Booster and AGS) Connection to other programs

Future plans for RHIC Machine goals for next few years with upgrades in progress: Enhanced RHIC luminosity (112 bunches,  * = 1m): Au – Au: 8  cm -2 s -1 (100 GeV/nucleon) For protons also 2  protons/bunch (no IBS): p  – p  : 60  cm -2 s -1 ; 70 % polarization (100 GeV) 150  cm -2 s -1 ; 70 % polarization (250 GeV) (luminosity averaged over store delivered to 2 IRs) EBIS (low maintenance linac-based pre-injector; all species incl. U and pol. He3; avoid Tandem investment; ~ 3 year pay-back period) RHIC luminosity upgrade (e-cooling, ~10  more luminosity, R&D in progress) eRHIC (high luminosity (1  cm -2 s -1 ) eA and pol. ep collider) 2  achieved 6  achieved

EBIS/Linac-based RHIC Pre-Injector l Highly successful development of Electron Beam Ion Source (EBIS) at BNL: meets RHIC performance requirements. l EBIS allows for a reliable, low maintenance Linac-based pre-injector replacing the Tandem Van de Graaffs l Greatly reduced operating costs, and avoidance of ~ 9 M$ in reliability-driven investments in the tandems l Highly flexible to handle the multiple simultaneous needs of RHIC and NSRL l Produces beams of ALL ion species including noble gas ions (NSRL), Uranium (RHIC) and polarized He 3 (eRHIC) l Ready to start construction, CD0 received; Cost: 19.4 M$; 3.5 year construction schedule: FY2006 – 09 NASA participation ($ 4.5M)

EBIS layout EBIS test stand

RHIC luminosity upgrade Eliminate beam blow-up from intra-beam scattering with electron beam cooling at full energy! What will remain the same: l 120 bunch pattern n 100 ns collision spacing ( ~ same data acquisition system) n Only one beam collision between DX magnets l 20 m magnet-free space for detectors n No “mini-beta” quadrupoles l Approx. the same bunch intensity n No new beam intensity issues n Background similar as before upgrade What changes: l Smaller transverse and longitudinal emittance n Smaller vertex region (Increased luminosity within detector acceptance) l Beta squeeze during store to level luminosity l Store length is limited to ~ 5 hours by “burn-off” due to Au-Au interactions (~ 200 b)

Superconducting ERL Electron Cooling R&D Buncher Cavity Cooling Solenoids (2 x 13m, 2-5 T) Debuncher Cavity Gold beam  Benchmarking of IBS and cooling simulation codes  Demonstrate high precision (<10 ppm) solenoid (2-5 T)  Demonstrate 20 nC, mA MHz CW SCRF electron gun  Develop MHz CW superconducting cavity for high intensity beams  Build R&D Energy Recovering Linac (ERL) 54 MeV, 100 mA electron beam

RHIC Luminosity with and without Cooling With e-cooling Without e-cooling Luminosity leveling through continuously adjusted cooling Store length limited to 4 hours by “burn-off” Four IRs with two at high luminosity 2 mm 5 hours Electron cooling simulations Transverse beam profile during store Also able to pre-cool polarized protons at injection energy

RHIC Luminosity Upgrade with Electron Cooling Gold collisions (100 GeV/n x 100 GeV/n): w/o e-coolingwith e-cooling Emittance (95%)  m15   3 Beta function at IR [m]  0.5 Number of bunches Bunch population [10 9 ]11  0.3 Beam-beam parameter per IR Ave. store luminosity [10 26 cm -2 s -1 ]870 Pol. Proton Collision (250 GeV x 250 GeV): Emittance (95%)  m2012 Beta function at IR [m] Number of bunches Bunch population [10 11 ]22 Beam-beam parameter per IR ? Ave. store luminosity [10 32 cm -2 s -1 ]1.55.0

Electron-Ion Collider at RHIC: eRHIC 10 GeV, 0.5 A e-ring with 1/3 of RHIC circumference (similar to PEP II HER) 10 GeV electron beam  s 1/2 for e-A : 63 GeV/u; s 1/2 for e  -p  : 100 GeV Electron cooling required for high luminosity e-A and low energy e-p collisions Polarized e-He3 (e-n) collisions with EBIS Existing RHIC interaction region allows for typical asymmetric detector Luminosity: up to 1  cm  2 s  1 per nucleon (1  cm  2 s  1 with linac – ring scheme) BNL, MIT collaboration

Summary Since 2000 RHIC has collided, for the first time, l Heavy ions l Light on heavy ions l Polarized protons (45% beam polarization) Heavy ion luminosity increased by factor 100 For next 4 years planned: l Factor 2 increase in heavy ion luminosity l Factor 6 increase in proton luminosity l Factor 2 increase in proton beam polarization Future upgrades: l RHIC luminosity upgrade (~10x) using electron cooling at store l Electron-ion collider eRHIC

Back-up material

RHIC design, achieved and enhanced design parameters ModeNo of bunches Ions/bunch [  9 ]  * [m] Beam polarization L peak [cm -2 s -1 ] L store ave [cm -2 s -1 ] A 1 A 2 L store ave [cm -2 s -1 ] Design values (1999) Au – Au    p – pp – p   Achieved values (2004) Au – Au    p – pp – p % 5   p – pp – p   Enhance design values (2008) Au – Au    p – pp – p % 80   Other high luminosity hadron colliders: achieved goalscaled to 200 GeV Tevatron (2 TeV)100    LHC (14 TeV)   10 30

Alternative eRHIC Design: Linac - Ring Electron ring replaced by energy-recovering linac, electrons in RHIC arcs: Higher luminosity (1  cm  2 s  1 ), simpler IR design, multiple IRs possible, 20 GeV upgrade possible

EBIS Completion

FY06 cryo-weeks reduced from 31 to 12 weeks l Combine FY06-07 runs for some models. Avoid summer running. Begin on 10/1/06 after 15 month shutdown. l $300K (ions) - $325K (polarized proton) / week running and $75K / week power costs when off l EBIS construction is expedited. Funding increased from $2.0M to $3.6M (+ $1.5M from NASA). Reprogram AIP ($0.5M), capital ($0.7M + $0.4M) Operations manpower reductions of FTE (355-> FTE) l The efficient and safe operation of the accelerator complex with the proposed staff size is more difficult. Present staff workload and stress levels are high. Concern that key accelerator physicists will move across the Atlantic. Loss of expertise is a major issue. l Some staff would be assigned to RSVP, if funding arrives in time. Electron cooling R&D will be reduced as EBIS takes priority and RHICII recedes into future Reassign waste management funding. 50% used to support FY06 Impact of FY2006 Presidential on Accel. Ops.

Impact of FY06P + constant effort (flat) funding on Accel. Ops. Combined FY06-07 run. With EBIS: l Reprogram funds to complete EBIS project (FY06-09). l No run in FY08 l Combined FY09-10 run. l Yearly 24 cryo-weeks running FY11 and later. Reduced operations cost form EBIS completion allows for more running. Without EBIS: l Reprogram funds to complete Tandem reliability upgrade (FY07-09) l Combined FY08-08 run l Yearly 20 cryo-weeks running FY10 and later The efficient and safe operation of the accelerator complex with the staff size is more difficult. This funding model supports the most favorable but still a dwindling long term physics program

Impact of FY06P + “flat-flat” on Accel. Ops. EBIS will not be built. Flat-flat funding would only allow for a combined FY06-07 and a combined FY08-09 run and then unable to support a physics program thereafter. Loss of expertise to complete the proposed runs is significant. The efficient and safe operation of the accelerator complex with the FY06 staff size is more difficult. This funding model rapidly leads to RHIC termination.

BNL proposed (FY constant effort) 31 cryo-week each year l Physics program includes ions and polarized protons to 500 GeV cm. EBIS project completed in 3.5 years l Reduce injector group manpower Accelerator R&D support of electron cooling for future RHICII and eRHIC would remain on a fast track. AIP support to continue to replace aging machine components and improve performance, eg. RHIC cryogenic system is 25 years old, would be accomplished in an orderly manner. RHIC running efficiency and safety are not a concern.