Transcript Hollis
Forward Calorimeter Upgrades in PHENIX: Past and Future Richard Hollis for the PHENIX Collaboration University of California, Riverside Winter Workshop on Nuclear Dynamics 8th January 2010 Overview The next decade at RHIC&PHENIX Motivation and Needs Calorimeter Upgrades Past: MPC – currently operational Future: FoCal – proposal soon Summary NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 2 The next decade at PHENIX A biased (to Forward Calorimetry) view: Gluon density at low-x in cold nuclear matter Proton spin contribution from Gluon Polarization Measure g-jet production, correlations in Au+Au collisions Test predictions for the relation between single-transverse spin in p+p and those in DIS For data taking and analysis over the course of the next decade… First step: measurements at high h NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 3 Onset of Gluon Saturation d+Au collisions BRAHMS: PRL93 (2009) 242303 Nuclear modification factor: Increasing suppression with h Consistent with the onset of gluon saturation at small-x in the Au nucleus. Need to study this in more detail by identifying particles expanding forward coverage Central Arms Muon Arms NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 4 Proton spin contribution from gluon polarization p+p collisions Spin contribution from gluon polarization xDg derived from measured ALL currently over a narrow region of x Large uncertainty at low-x Need to measure ALL over a broader region of x forward h measure direct photons RHIC range 0.05 < x < 0.2 NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 5 Building detectors to suit physics needs Need: Forward rapidities Direct photons Well defined energy scale for g measurements NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 6 PHENIX Acceptance Tracking Central region and forward muon arms mTr f coverage 2p mTr Calorimetry 0 (F)VTX Very limited acceptance In f and h -3 -2 -1 0 1 2 3 h 1 2 3 h What do we need for the future? 0 and how can we obtain it? f coverage 2p EMC NUCLEARDYNAMICS -3 WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 7 -2 -1 0 PHENIX Acceptance -3 -2 -1 MPC 0 1 2 EMC 3 h MPC 0 f coverage 3.1<|h|<3.9 (F)VTX 0 Muon Piston Calorimeter (MPC) 2p Staged Calorimeter Upgrades mTr f coverage 2p mTr NUCLEARDYNAMICS -3 WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 8 -2 -1 0 1 2 3 h Muon Piston Calorimeter (MPC) MPC(N) 18cm long ~20X0 2.2x2.2cm transverse 220 (196) Crystals in N (S) Counts Lead Scintillator (PbW04) Raw Signal South Arm: -3.7<h<-3.1 North Arm: 3.1<h< 3.9 Measure p0’s up to 17 GeV pT~1.7 GeV/c pT>1.7GeV/c – measure single “clusters” NUCLEARDYNAMICS Mixed-event Background Yield WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 9 12 < E < 15 GeV Physics Application Mid-rapidity p0 Trigger Two-particle correlations Correlation of central arm p0 and h with MPC p0 Measure jet modification in d+Au collisions Forward Associates dN df Df NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 10 Physics Application Mid-rapidity p0 Trigger Two-particle correlations Correlation of central arm p0 and h with MPC p0 Measure jet modification in d+Au collisions Probe low-x (0.006<x<0.1) IdA suppression – a signature of CGC NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 11 Forward Associates Physics Application Calorimeters are versatile Measurements using identified cC and h are underway 3.0<h<4.0 Preliminary results on transverse single-spin asymmetries • Measurements over a broad phase space will provide quantitative tests for models How do the calorimeters contribute to DG – the gluon contribution to proton spin Would like to measure direct gs NUCLEARDYNAMICS p+pp0+X at s=62.4 GeV/c2 WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 12 PHENIX Acceptance 2p mTr f coverage Staged Calorimeter Upgrades (F)VTX 0 Muon Piston Calorimeter (MPC) -3 3.1<|h|<3.9 -2 -1 0 1 2 EMC 3 h MPC 0 f coverage 2p MPC Forward Calorimeter (FoCal) 1<|h|<3 mTr NUCLEARDYNAMICS -3 WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 13 -2 -1 0 1 2 3 h Finding space in PHENIX MPC MPC installed ~ 3<|h|<4 FoCal: where could it fit? NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 14 Finding space in PHENIX Small space in front of nosecone 40 cm from vertex 20 cm deep Calorimeter needs to be high density Silicon-Tungsten sampling calorimeter NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 15 FoCal Transverse View Silicon-Tungsten sampling calorimeter 21 layers ~21X0 Each Arm: 1<|h|<3 Longitudinal View Expect good resolution in E and h/f 6.1cm Active readout ~1.5x1.5cm Distinct 2-shower p0 up to pT~3 GeV/c (h~1) NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 16 FoCal x Coverage p+p collisions x versus pT (p+p, 500 GeV) (FoCal Acceptance) NUCLEARDYNAMICS x coverage: Weak pT dependence WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 17 FoCal x Coverage p+p collisions x versus h (p+p, 500 GeV) (FoCal Acceptance) NUCLEARDYNAMICS x coverage: Weak pT dependence Strong h dependence WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 18 FoCal x Coverage p+p collisions x versus h (p+p, 500 GeV) (FoCal & MPC Acceptance) NUCLEARDYNAMICS x coverage: Weak pT dependence Strong h dependence FoCal complementary to MPC WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 19 FoCal x Coverage x for h bins (p+p, 500 GeV) (FoCal Acceptance) x coverage: Weak pT dependence Strong h dependence FoCal complementary to MPC Selecting h region probes a specific x range NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 20 FoCal (Expected) Performance d+Au collisions Can one see jets over the background Sufficiently isolated? Average background • Units are measured energy (~2% of total) Single-event background • ~20 times higher 30GeV embedded jet • Visible over the background NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 21 What about direct g identification? Important for our measurements in the next decade in Spin d+Au Au+Au NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 22 Identifying p0 and g p+p collisions First: use physics Ratio of background/signal (NLO calculation) Direct g typically are alone Whilst p0 are produced as part of a hadronic jet Measurement of accompanying energy can reduce background at minimal expense to g Still, this does not provide full decontamination Need direct p0 identification NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 23 High energy p0 shower p+p collisions Origin of all shower particles (red) Shown with effective resolution of pads Individual tracks not distinguishable NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 24 High energy p0 shower p+p collisions Finer resolution could “see” individual tracks from p0 Up to ~50GeV Make the whole detector with finer resolution!! Not realistic → what can be designed? NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 25 High energy p0 shower p+p collisions Finer resolution could “see” individual tracks from p0 Up to ~50GeV Make the whole detector with finer resolution!! Not realistic → what can be designed? EM0 EM1 EM2 ~2 towers ~70 strips Add highly segmented layers of x/y strips into first segment. Measure the development of the shower at its infancy With a resolution to distinguish individual g tracks NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 26 x y x y x y x y High energy p0 shower Finer resolution could “see” individual tracks from p0 Tracks are visibly Separable Track showers Merge Up to ~50GeV Make the whole detector with finer resolution!! Not realistic → what can be designed? Add highly segmented layers of x/y strips into first segment. Measure the development of the shower at its infancy With a resolution to distinguish individual g tracks NUCLEARDYNAMICS Catch the shower, before it’s too late WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 27 High energy p0 shower Using a Hough Transform, Transverse/longitudinal coordinate Find the best track as most frequently occurring Houghslope Use each track vector, full track energy → calculate invariant mass NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 28 Performance of FoCal Reconstruction Reconstruction of p0 (p+p 500 GeV minimum bias pythia) NUCLEARDYNAMICS Signal reconstruction (d+Au 200 GeV minimum bias + embedded pythia g+jet signal) WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 29 Summary PHENIX Calorimeter upgrades (will) provide much extended coverage for a variety of physics topics Proven p0 reconstruction in the MPC further our understanding of forward jet production in d+Au collisions FoCal complements the MPC in terms of additional phase-space coverage and direct photon identification capabilities at high energies. For p+p, d+Au (and Au+Au) collisions NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 30 An energy scale for jet suppression A+A collisions h-h correlations exhibit interesting features … but have limitations: may be subject to surface bias may not reveal the jet energy scale STAR: PRL103 (2009) 172301 STAR: NPA830 (2009) 685C g-h or g-jet could provide an energy scale • (assuming) the g is not [energy] suppressed Reduced surface bias • as the trigger probe is not modified NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 31 MPC x Coverage x versus h (p+p, 500 GeV) (MPC Acceptance) NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 32 d+Au collisions Correlation of central arm p0 and h with MPC p0 Measured associate yields relative to pp Systematic suppression with centrality No appreciable trigger dependence Probe low-x (0.006<x<0.1) NUCLEARDYNAMICS WINTER●WORKSHOP Richard Hollis 8th January 2010 ● 33