Year- 1 (Heavy- Ion) Physics with CMS at the LHC

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Year- 1 (Heavy- Ion) Physics with CMS at the LHC Edwin Norbeck and Yasar Onel (for the CMS collaboration) University of Iowa For the 26 th Winter Workshop on Nuclear Dynamics Ocho Rios, Jamaica 8 January 2010

Outline LHC (Large Hadron Collider) CMS (Mostly about forward angles) December results and future projections Ed Norbeck Univ. of Iowa 8 Jan 2010 2

What is New at LHC? AGS SPS RHIC LHC s NN (GeV) 5 20 200 5500 Increasing factor x4 x10 x28 1.6 3.0 5.3 8.6 LHC energies are far exceeding previous heavy-ion accelerators - A hotter, denser, and longer lived partonic matter For central collisions, T Bjorken 0 d ~ with 0 1 de 2 ( R ) 1fm/c ~ 10 GeV/fm 3 Ed Norbeck Univ. of Iowa 8 Jan 2010 3

Production Rate at LHC - Large rates of various hard probes over a larger kinematic range - Plenty of heavy quarks (b & c) - Weakly interacting probes are available (W ± & Z 0 ) d 3 /dyd 2 p T [mb GeV -2 ] SPS RHIC LHC p T [GeV] Ed Norbeck Univ. of Iowa 8 Jan 2010 4

The Quark Gluon Plasma Hard probes are abundant at the LHC Allow quantitative measurements of e.g. temperature, density, transport coefficients of the QGP Ed Norbeck Univ. of Iowa 8 Jan 2010 5

Note from C hamonix meeting: Early Pb Beam will have lower energy. 10TeV pp corresponds to 4 TeV in Pb+Pb (1.97 Te V/nucleon) Pb+Pb Coll. Energy Max. Coll. Rate Ave. Coll. rate CPU Budget /Event Year-1 ~ 4 TeV ~150Hz ~100Hz ~60s Nominal 5.5 TeV ~8kHz ~3kHz ~2s During Year- 1 run no selection will be applied in the HLT and all events will be written to tape Ed Norbeck Univ. of Iowa 8 Jan 2010 6

The three LHC heavy- ion experiments ALICE: dedicated HI experiment Largest HI community (~1000) Tracking ( <1-2): TPC + ITS + TRD 0.5 T solenoid magnet EMCal under discussion Forward muon spectrometer Strongest capabilities: low- p T, light- quark PID,... ATLAS & CMS: multipurpose (pp) + HI program People: ~50/2000 (ATLAS), ~70/2300 (CMS) <2.5: Full tracking, muons <5: Calorimetry 4 T (CMS), 2 T (ATLAS) mag. field Forward detectors (CMS) Strongest capabilities: hard-probes, Y, full jet reco, heavy-q jet PID, jet-z, Ed Norbeck Univ. of Iowa 8 Jan 2010 7

Large Hadron Collider (LHC) @ CERN 1 ring: 26.66 km circumference 8.33 T superconducting coils 25 ns crossing time LHCb CMS ATLAS ALICE Ed Norbeck Univ. of Iowa 8 Jan 2010 8

The CMS Detector (Pixel) Large Range of Hermetic Coverage: Tracker, muons ECAL + HCAL Forward HCAL ZDC 8.3< Ed Norbeck Univ. of Iowa 8 Jan 2010 9

Innermost Endcap Disk 10

Compact Muon Solenoid Ed Norbeck Univ. of Iowa 8 Jan 2010 11

Some of CMS capabilities CMS excels at high p T measurements in Pb+Pb Fast, flexible DAQ + Trigger Jet, photon, muon trigger High resolution, large acceptance calorimeters Jets, photons High resolution, large acceptance tracker Charged hadrons from 100 MeV to 100 of GeV The excellent capabilities CMS give the unique possibility of measuring both soft and hard probes of the dense medium state: Multiplicity Soft and hard spectra of charged particles Fragmentation Function from Jet correlations Photons Jets Quarkonia Ed Norbeck Univ. of Iowa 8 Jan 2010 12

Excellent resolution for upsilon states I expect the second excited state to melt in the hot QGP. If so, the third peak would be only from excited upsilons formed at the surface. Study details by looking at the amplitude of the third peak as a function of centrality and angle wrt the reaction plane and of other variables. Ed Norbeck Univ. of Iowa 8 Jan 2010 13

Tungsten stops beam. Kinetic energy of n, produces showers of charged particles, which make light in fibers. N, EM has 5 horizontal towers HAD section has 4 longitudinal towers

Measuring Reaction Centrality ZDC measures spectator neutrons 15

Other measures of impact parameter In forward calorimeter HF 3 < < 5.2 In CASTOR 5.2 < < 6.7 Ed Norbeck Univ. of Iowa 8 Jan 2010 16

New, useful physics from p- p collisions in December dn ch /d at 2.36 TeV Allows for better extrapolation to energies used in heavy- ion calculations. Expect to get dn ch /d at 7 TeV (3.5 TeV beams) in February. This will bracket 4 and 5.5 TeV/nucleon heavy ion runs. >10 µb - 1 at 900 GeV (injection energy) gave dn ch /d values that agree with other measurements (Tevatron). CMS is working well. Measurements agree with MC. Ed Norbeck Univ. of Iowa 8 Jan 2010 17

The present plan Resume proton experiments in mid February at 7 TeV. Some increase in energy during the year. Pb beam setup during last two weeks of October. Pb- Pb experiments during November at some energy well under 5.5 TeV/nucleon, 4 Tev/nucleon likely. Ed Norbeck Univ. of Iowa 8 Jan 2010 18

Search for Stranglets Edwin Norbeck and Yasar Onel University of Iowa (not submitted to the 3000 people in the CMS collaboration) For the 26 th Winter Workshop on Nuclear Dynamics Ocho Rios, Jamaica 8 January 2010

Stranglets observations Defined here as light nuclei with enough strange quarks to reduce Z/A below that of lead. Thought to be a common object seen in the core of cosmic ray showers (in mountain top detectors). Typical reaction: cosmic iron on nitrogen. How could such a reaction produce a stranglet? Ed Norbeck Univ. of Iowa 8 Jan 2010

Cosmic ray stranglets Cannot be formed from hot quark- gluon plasma. Nucleons (P, N, o ) from hot QGP do not stick together to form nuclei. [J. Ellis et al J. Phys. G 35 (2008) 115004] Suggest formed by Ks, etc. from QGP getting into the spectators. For Fe on N there is always much spectator matter. Would like to make them with Pb- Pb and see them in the Zero Degree Calorimeter. Ed Norbeck Univ. of Iowa 8 Jan 2010

Lifetimes Lifetimes of hyper nuclei with two o is similar to that of a single o, 200-300 ps. Assuming the lifetime of a strange quark in a strangelet is 300 ps, the mean distance to decay, c, is 9.6 m at 100 GeV/nucleon (RHIC) 260 m at 2.75 TeV/nucleon (LHC) 96 km at 1000 TeV/nucleon (cosmic rays) With many strange quarks, the lifetime of the stranglet may be shorter. Look for stranglets in a zero degree calorimeter. Distance from IP to ZDC is 18 m for STAR and 140 m for CMS. For CMS, 84 m gets stranglet beyond last magnet. Ed Norbeck Univ. of Iowa 8 Jan 2010

STAR stranglet search Looked at 4% most central collisions and found none [Phys. Rev. C 76 (2007) 011901(R)] neutrons. But stranglets would only be produced in peripheral collisions. Ed Norbeck Univ. of Iowa 8 Jan 2010

CMS stranglet search Look for large signal in hadronic part of ZDC. Determine impact parameter from HF (3 < < 5). Look for signals larger than for expected number of neutrons. STAR already has such data. Can we search STAR data for strangelet events? Ed Norbeck Univ. of Iowa 8 Jan 2010

Energy dependence RHIC vs LHC LHC energy more like cosmic rays More Ks at the higher energy Mechanism K - more likely to react with spectator than K + Ed Norbeck Univ. of Iowa 8 Jan 2010

stranglets Spectator nuclei with reduced Z/A likely produced in suitably non- central collisions, particularly at LHC. Need some good quantitative calculations. Short lived stranglets that could reach mountain- top cosmic ray detectors may not live long enough to reach ZDCs. Ed Norbeck Univ. of Iowa 8 Jan 2010