4/10/20121 A N DY Status Commissioning with colliding beams L.C.Bland, for AnDY 10 April 2012 Time Meeting, BNL.

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4/10/20121 A N DY Status Commissioning with colliding beams L.C.Bland, for AnDY 10 April 2012 Time Meeting, BNL

4/10/20122 Changes to A N DY for Run-12 GEANT model of proposed A N DY apparatus (run-13) Proposed A N DY detector (left), as submitted, consists of annular ECal, annular HCal, preshower + tracking through the (modified) PHOBOS split-dipole The HCal module pair used in run 11 was modified to become an annular 12-row x 20 column HCal for run 12. The picture to the right shows the phototube (PMT) end of HCal upon completion of its installation in December, before installing all PMT. Separated-beams test on and shows most things are working, and identifies some things to fix (a few holes) on the access. Thanks to C.Folz, et al.

4/10/20123 Summary of A N DY Timeline March 2010 – initial documentation of plans June 2010 – letter of intent to program advisory committee (PAC) August 2010 – cleanup of IP2 begun December 2010 – implementation of run-11 apparatus complete June 2011 – run-11 goals achieved, proposal to PAC and approval July 2011 – completion of the move of BigCal from JLab to BNL February 2012 – run-11 stretch goal achieved and funding proposalrun-11 stretch goal March 2012 – BNL review of funding proposal Many thanks to C-A for excellent support for an ambitious project!

4/10/20124 Outcome of Review To: cc: Helmut Marsiske, Thomas Roser, Tom Ludlam, Edward O'Brien, Steven Vigdor From: Hank Crawford Fri Apr 6 09:37:49 EDT 2012 Hi - We have just come from a meeting with BNL management at which we were informed that AnDY will not be approved to go forward. We'll send the review committee report when we get it. - We disagree with management on most points discussed - we had assembled a great team and had a credible timeline but they disagree. We will continue analysis of the run11 data to uncover the jet signal. Thanks for all of your efforts. - Hank and Les

4/10/201252/6/20165 Run11 A N (Jet) arXiv: v1 200GeV Non-zero jet analyzing power essentially a prerequisite before proceeding to Drell Yan arXiv: jet A N measurements are required to clarify signs of quark/gluon correlators related to Sivers functions. from p  +p  “old” Sivers function “new” Sivers function  s=200 GeV Siver’s effect only (no collin’s effect contribution) Need A N (Jet) measurements before DY With ~10/pb & P=50%, AnDY run11 can measure A N (Jet)

4/10/20126 Jet Trigger Events Select from jet-trigger events for HCal “high-tower” to be centered in module Display for each detector of each module the ADC count as color scale (black=greatest count  yellow=lowest count) Events look “jetty”, as expected

4/10/20127 Towards Forward Jets (a) Distribution of summed energy in HCal modules from the jet trigger. (b) Distribution of fraction of energy in the jet as a function of distance in  -  space from the jet center (jet shape). (c) Jet energy from simulations versus reconstructed response in ECal+HCal arXiv: (a)(b)(c)

4/10/20128 Are These Events Jets? Reconstructions of full simulation, as generated by PYTHIA with detector response simulated by GEANT  max is the larger of the scattered parton pseudorapidity from PYTHIA 2  2 processes  Run-11 A N DY jet trigger primarily selects jets

4/10/20129 Jet Spin Effects Evidence for non-zero jet analyzing power Jet clustering, energy scales, trigger bias (from ECal), HCal compensation systematic effects still to be done i.e., standard spin-sorted cross ratio analysis applied to run-11 jet-triggered events All jet triggered runs 56<day<107

4/10/ Requests Complete end-of-store measurements to tune-up IP2 bump removal and collimation optimization to reduce backgrounds when IP2 goes into collisions. Bare minimum request is >2 fills with IP2 collisions. 1 fill needed for final timing checks of separated-beam tuneup of run-12 apparatus. 2 fills needed with ECal in its out position to establish from measurement effects from trigger bias on run-11 jets.

4/10/ Ideal Collide at IP2 and acquire 10 pb -1 of polarized proton collisions at  s=500 GeV with ECal moved to its out position, meaning no shadow cast on HCal. This fully eliminates trigger-bias from run-11 jet sample. The annular HCal will eliminate “sculpted combinatorics” as a background issue for      ,       or         calibration of hadronic response of HCal. Demonstration of 10 pb-1 / week delivered to 3 rd IP could be useful to others in possible future endeavors at RHIC.

4/10/ Backup

4/10/ Critical Run-12 Tests … proposed... (1) Finish HCal calibration with new annulus: correction for hadronic response (2) Test operation of GEM prototype (3) Demonstrate 10 pb -1 /week at  s=500 GeV, as required for runs 13,14 A N DY Comments: Corrections to run-11 HCal calibration for hadron showers expected to be ~20% GEMs improve position resolution from ~5cm (run-11)  ~0.1mm for calorimeter/preshower association required for background discrimination and other trackings Data from run-12 IP2 tests will improve run-11 J/ , enable B  J/  +K and start on concurrent  s=500 GeV A N   measurement required to determine sign of DY A N With run-12 test, becomes “measured to be”

4/10/ Dileptons from Run 11 Data A N DY profiling methods were applied to a limited data sample (L int =0.5 / pb) of run-11 ECal triggered data. Dominant backgrounds are now from , and are suppressed by using MIP response of beam-beam counters to tag clusters. Individual detector    calibration for HCal was an essential step to reconstruct J/  Limited granularity of BBC and poor position resolution of HCal-EM cluster results in less photon suppression than expected for final A N DY apparatus (project ~100x better suppression) Hadron suppression is not yet required, but will be in going from dileptons to DY J/  e+e- peak has ~120 events with 5.4  statistical significance. PYTHIA with NRQCD expects 420 events in the run-11 acceptance, approximately consistent with observation after crude efficiency correction. From PYTHIA 6.425, DY with M>4 GeV/c 2 is 170x smaller in this acceptance. J/  is a window to heavy flavor via B  J/  K and  b  J/  p  that would help quantify intrinsic b from proton backgrounds to DY Run-11 data absolutely compared to fast-simulator used for DY estimates

4/10/ Schematic of detector for Run-11 Polarized proton collisions at  s=500 GeV from February to April 2011 Beam-beam counter (BBC) for minimum-bias trigger and luminosity measurement from PHOBOS [NIM A474 (2001) 38] Zero-degree calorimeter and shower maximum detector for luminosity measurement and local polarimetry (ZDC/ZDC-SMD, not shown) Hadron calorimeter modules (HCal) are 9x12 modules from AGS-E864 (NIM406,227) Small (~120 cells) ECal loaned from BigCal at JLab Pre-shower detector

4/10/ Impact of Collisions at IP2 The anatomy of initiating collisions at IP2 Early after a RHIC store is set up, beams are colliding at IP6 (STAR) and IP8 (PHENIX). Beams are transversely separated at IP2 (A N DY). The arrow indicates when collisions begin at IP2 After the beam intensity decays to a threshold (here, 1.3  ions/bunch), collisions begin at IP2. There is loss of beam in the Yellow ring. The beam loss is monitored. The spikes in the Blue ring are due to insertions of carbon ribbons for measuring the beam polarization. Beam- beam tune shift causes loss of ions in Yellow when collisions begin at IP2. This loss typically decays with time, as shown. Luminosity at IP6 (STAR) and IP8 (PHENIX) is mostly constant when collisions are initiated at IP2 (A N DY).

4/10/ IP2 collisions have begun <3 hours after physics ON with minimal impact on IP6,IP8. Adequate luminosity for A N DY (10 pb -1 /week for  s=500 GeV polarized proton collisions) is projected for subsequent runs (to be demonstrated in run 12) IP2 collisions have begun <3 hours after physics ON with minimal impact on IP6,IP8. ~2mr crossing angle ~1.6mr crossing angle ~0mr crossing angle systematically increased thresholds for IP2 collisions Most of run-11 integrated luminosity was devoted to the HCal-based jet trigger Minimal impact on STAR,PHENIX Fri. 8 April 1.50  /bunch Impact of IP2 Collisions