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The CBM Experiment at FAIR - An Update -

Volker Friese. v.friese@gsi.de. The CBM Experiment at FAIR - An Update -. Workshop on The Physics of Compressed Baryonic Matter Trento, May 28 – June 2, 2006. Baseline Detector Setup. Tracking: STS, TRD Vertexing: STS Hadron ID : TOF Electron ID: RICH, TRD, ECAL γ , n: ECAL.

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The CBM Experiment at FAIR - An Update -

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  1. Volker Friese v.friese@gsi.de The CBM Experiment at FAIR- An Update - Workshop on The Physics of Compressed Baryonic Matter Trento, May 28 – June 2, 2006

  2. Baseline Detector Setup Tracking: STS, TRD Vertexing: STS Hadron ID : TOF Electron ID: RICH, TRD, ECAL γ, n: ECAL Volker Friese Workshop on The Physics of CBM, Trento, May 2006 2

  3. D0→π+K-(D±→ππK) J/ψ→e+e- J/ψ→μ+μ- ρ,ω,φ→e+e- Λ→π-p, Ξ-→Λπ-, Ω-→ΛK- K/πfluctuations CBM Feasibility Studies • Simulation levels: • pure Monte-Carlo (principal feasibility; acceptance, estimated yields) • anticipated detector response, track and vertex reconstruction • full detector simulation including global tracking and PID Volker Friese Workshop on The Physics of CBM, Trento, May 2006 3

  4. Performance of STS for D0 Mesons invariant π+K- mass vertex resolution without PID similar studies for D± (larger cτ, better vertex, 3-particle combinatorics) Volker Friese Workshop on The Physics of CBM, Trento, May 2006 4

  5. Optimisation of the STS Volker Friese Workshop on The Physics of CBM, Trento, May 2006 5

  6. Optimisation of STS: open charm Volker Friese Workshop on The Physics of CBM, Trento, May 2006 6

  7. Open Charm: Questions What should me measure: yields, spectra, flow? How close to threshold do we have to go? What about charmed baryons? (Λc, τ = 60 μm, very challenging!) Huge impact on design of STS! Volker Friese Workshop on The Physics of CBM, Trento, May 2006 7

  8. 7 6 tracking 5 4 pixel detectors strip detectors vertexing 3 2 1 vacuum z = 5,10,(20) cm z = (20),40,60,80,100 cm The Silicon Tracking System Main Tracker (hybrid pixel + strip) Vertex tracker: MAPS in-vacuo operation removable, for open charm only (not maximum intensity) Volker Friese Workshop on The Physics of CBM, Trento, May 2006 8

  9. Fe absorbers  C absorber (cm) 5 10 20 30 120 16 detector layers ~190 cm 247 cm 170cm Electrons or Muons? Concept of an active absorber setup for muon identification Volker Friese Workshop on The Physics of CBM, Trento, May 2006 9

  10. CERES (1997) arXiv:nucl-ex/9712008 v1 23Dec 1997 Electrons vs muons: physics difference Scomparini (NA60), QM 05 Volker Friese Workshop on The Physics of CBM, Trento, May 2006 10

  11. Electrons vs. muons: physics difference (2) Both dielectrons and dimuons measure LVM and charmonium Muon measurements exclude mass range below 2 mμ ≈ 200 MeV Relevant physics: (modified ρ) : 200 – 600 MeV → close to edge of phase space. No π Dalitz peak in spectrum (efficiency control, normalisation of cocktail) Volker Friese Workshop on The Physics of CBM, Trento, May 2006 11

  12. electron identification is complicated: cherenkov, TRneeds dedicated detectors, but: established technologies muon identification: simple in principle: absorber details are tedious: optimisation of absorber material / thickness usually optimised to one beam energy, not well suited for energy scan problem: matching of track before and after absorber Electrons vs muons: Identification Volker Friese Workshop on The Physics of CBM, Trento, May 2006 12

  13. Electrons: abundant background from conversion and π Dalitz conversion: can be reduced by target thickness Dalitz: requires sophisticated suppression strategy misidentified hadrons: performance of eID detectors Muons: main background from charged pion decay reduced by minimising distance of muID from target detection of decay topology (kink) misidenified hadrons: performance of muID detector Electrons vs muons: Background Volker Friese Workshop on The Physics of CBM, Trento, May 2006 13

  14. CBM performance: Charmonium Muons Electrons Both feasible; muons seem to work better What about higher-mass states? Volker Friese Workshop on The Physics of CBM, Trento, May 2006 14

  15. CBM performance: Low-mass vector mesons Dimuons Dielectrons Volker Friese Workshop on The Physics of CBM, Trento, May 2006 15

  16. Dielectrons MC only, perfect tracking, perfect PID more realistic simulation started, first look: performance decreases detector concepts available, R&D under way not expected to be very sensitive to beam energy Dimuons Tracking and PID already included detector concept under development (GEM / MWPC) for one beam energy only (might be very sensitive) "Level of reality" Volker Friese Workshop on The Physics of CBM, Trento, May 2006 16

  17. Options for setup with muID "Minimal setup" already accesses a big part of CBM physics "Minimal change" : Replace RICH by MUID Volker Friese Workshop on The Physics of CBM, Trento, May 2006 17

  18. Decision aspects Volker Friese Workshop on The Physics of CBM, Trento, May 2006 18

  19. Dielectron simulations perform simulations with realistic tracking and electron ID study ψ' Dimuon simulations implement realistic detector response study energy dependence of performance make code available Open charm simulations D0 possible without TOF? Low-mass vector mesons Develop quality criterion of measurement (e.g. power to discriminate in-medium scenarios) MUID detector develop detector concept (tracking stations) cost estimate Theory how important is ψ' (higher states?) limitations in low-mass spectrum due to 2μ threshold? relative importance of physics observables to be potentially skipped prioritised observable list Input needed Volker Friese Workshop on The Physics of CBM, Trento, May 2006 19

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