Facility for Antiproton and Ion Research FAIR GSI

  • Slides: 22
Download presentation
Facility for Antiproton and Ion Research FAIR @ GSI Guenther Rosner BEACH 2006, Lancaster

Facility for Antiproton and Ion Research FAIR @ GSI Guenther Rosner BEACH 2006, Lancaster Univ. 1

GSI Darmstadt n -Ion y v a e otro r h c n Sy

GSI Darmstadt n -Ion y v a e otro r h c n Sy H ing R e rag to n. S o I y av He tor a r e l e r Acc Linea Present GSI facility in Darmstadt/Germany Guenther Rosner BEACH 2006, Lancaster Univ. 2

FAIR GSI today Future Facility SIS 100/300 SIS 18 UNILAC ESR 100 m Super

FAIR GSI today Future Facility SIS 100/300 SIS 18 UNILAC ESR 100 m Super FRS HESR Beams in the future: RESR Beams now: Z = 1 – 92 (Protons to Uranium) ≤ 2 Ge. V/nucleon some beam cooling Guenther Rosner CR NESR Intensity: primary 100 -fold secondary 10 000 -fold Species: Z = -1 to 92 (Anti-protons to Uranium) Energies: ≤ 35 - 45 Ge. V/u Precision: full beam cooling BEACH 2006, Lancaster Univ. 3

Six research areas at FAIR Nuclear Structure & Astrophysics with beams of short-lived nuclei

Six research areas at FAIR Nuclear Structure & Astrophysics with beams of short-lived nuclei 100 m Hadron Physics with antiproton beams Nuclear Matter Physics with 35 -45 Ge. V/u HI beams Plasma Physics with compressed ion beams & highintensity petawatt-laser Ultra-high electromagnetic fields & quantum electrodynamics with highly stripped ions and antimatter Solid state and biological applications with ion beams Guenther Rosner BEACH 2006, Lancaster Univ. 5

Accelerator chain Highly Parallel Operation: High Energy operation SIS 300 Guenther Rosner BEACH 2006,

Accelerator chain Highly Parallel Operation: High Energy operation SIS 300 Guenther Rosner BEACH 2006, Lancaster Univ. 6

Rare isotope beams (0 -1. 5 A Ge. V in flight) § § §

Rare isotope beams (0 -1. 5 A Ge. V in flight) § § § Superconducting FRagment Separator High-Energy Reaction Setup Multi-Storage Rings (CR, NESR, e. A) Energy-Bunched Stopped Beams 20 Tm fr SI om S 1 00 § from SIS 18 Guenther Rosner Key characteristics : - all elements, H to U - intensity > 1012 ions/sec. - high and low energies - pulsed and CW beams BEACH 2006, Lancaster Univ. 7

Heavy ion production rate Guenther Rosner BEACH 2006, Lancaster Univ. 8

Heavy ion production rate Guenther Rosner BEACH 2006, Lancaster Univ. 8

Compressed baryonic matter (CBM) SPS RHIC g, p-, p - beams Proton beams LHC

Compressed baryonic matter (CBM) SPS RHIC g, p-, p - beams Proton beams LHC SIS 18 SIS 200 300 T [Me. V] 300 Guenther Rosner BEACH 2006, Lancaster Univ. 9

Phase diagram of strongly interacting matter n SPS, RHIC, LHC: q n SIS 300:

Phase diagram of strongly interacting matter n SPS, RHIC, LHC: q n SIS 300: q Guenther Rosner high temperature, low baryon density moderate temperature, high baryon density BEACH 2006, Lancaster Univ. 10

Mapping the QCD phase diagram SI S 1 00 /3 00 Hadron gas EOS:

Mapping the QCD phase diagram SI S 1 00 /3 00 Hadron gas EOS: V. Toneev, Y. Ivanov et al. nucl-th/0309008 Critical end-point: Z. Fodor, S. Katz, hep-lat/0402006, S. Ejiri et al. , hep-lat/0312006 Guenther Rosner BEACH 2006, Lancaster Univ. 11

CBM Experiment - Objectives n In-medium modifications of hadrons q onset of chiral symmetry

CBM Experiment - Objectives n In-medium modifications of hadrons q onset of chiral symmetry restoration at high ρB q measure: ρ, ω, ф e+e- and open charm (D mesons) n Strangeness in matter (strange matter? ) q enhanced strangeness production? q measure: K, Λ, Σ, Ξ, Ω n Indications for deconfinement at high ρB q anomalous charmonium suppression? q measure: J/ψ, D n Critical point q event-by-event fluctuations n Color superconductivity q precursor effects? Guenther Rosner BEACH 2006, Lancaster Univ. 12

CBM setup n Radiation hard Silicon (pixel/strip) Tracking System q n Electron detectors: RICH

CBM setup n Radiation hard Silicon (pixel/strip) Tracking System q n Electron detectors: RICH & TRD & ECAL: q pion suppression better 104 n Hadron identification: TOF-RPC n Measurement of photons, π, η, and muons: q n Guenther Rosner in a magnetic dipole field electromagnetic calorimeter (ECAL) High speed data acquisition and trigger system BEACH 2006, Lancaster Univ. 13

PANDA physics programme Charmonium spectroscopy Exotics: charmed hybrids & heavy glueballs Time-like form factors

PANDA physics programme Charmonium spectroscopy Exotics: charmed hybrids & heavy glueballs Time-like form factors Medium modifications of charmed mesons Drell-Yan processes Hard exclusive processes CP-violation (D & - sector) Hypernuclei Guenther Rosner BEACH 2006, Lancaster Univ. 14

(Exotic) hadron spectroscopy Guenther Rosner BEACH 2006, Lancaster Univ. 15

(Exotic) hadron spectroscopy Guenther Rosner BEACH 2006, Lancaster Univ. 15

Charmonium spectroscopy – a high-precision testing ground for confinement Guenther Rosner n Direct formation

Charmonium spectroscopy – a high-precision testing ground for confinement Guenther Rosner n Direct formation of charmonium in pbarp n Experimental issues e. g. q measure hc(11 P 1) width q find c‘ (21 S 0) q measure transition rates q identify states above DDbar threshold n Refine confinement potential (spin dependence? ) n Challenge for lattice QCD BEACH 2006, Lancaster Univ. 16

Search for heavy glueballs n Heavy glueballs q q q n flavour blind decay

Search for heavy glueballs n Heavy glueballs q q q n flavour blind decay charmed final states! Probably small widths only a few charmed mesons around 3 -4 Me. V/c 2 : less mixing! Exotic heavy glueballs: no mixing! q q m(2+-) = 4140(50)(200) Me. V m(0+-) = 4740(70)(230) Me. V Morningstar & Peardon, PRD 60(1999)34509 Morningstar & Peardon, PRD 56(1997)4043 Guenther Rosner BEACH 2006, Lancaster Univ. 17

What is needed experimentally? n n Gluon-rich environment q Proton-antiproton annihilation Precision resonance scan

What is needed experimentally? n n Gluon-rich environment q Proton-antiproton annihilation Precision resonance scan q Cooled antiproton beam q High luminosity All quantum numbers measured q Large acceptance detector High statistics samples q Large cross sections q Several years of beamtime Guenther Rosner Crystal Barrel f 0(1500) BEACH 2006, Lancaster Univ. E 835: 240 ke. V PANDA: 20 ke. V 18

Antiproton accelerator HESR Guenther Rosner BEACH 2006, Lancaster Univ. 19

Antiproton accelerator HESR Guenther Rosner BEACH 2006, Lancaster Univ. 19

Target generator Muon counters TOF stop Solenoid EM and hadron calorimeters Dipole RICH Interaction

Target generator Muon counters TOF stop Solenoid EM and hadron calorimeters Dipole RICH Interaction point Drift or wire chambers Ø Tracking of charged particles Ø Identification of γ, e±, μ±, π±, K±, p, anti-p Ø High rate capability Ø Fast trigger scheme Guenther Rosner BEACH 2006, Lancaster Univ. 20

Charmonium Production in pp * for selected decay mode ** L = 2 x

Charmonium Production in pp * for selected decay mode ** L = 2 x 1032 cm– 2 s– 1, 50% accelerator and detector efficiency, integrated luminosity = 8 pb– 1/day *** 1% B. R. for this decay mode Guenther Rosner BEACH 2006, Lancaster Univ. 21

PANDA production rates (1 -2 Final State Cross section -1 fb /y) # reconstr.

PANDA production rates (1 -2 Final State Cross section -1 fb /y) # reconstr. events/y Common feature : Low multiplicity events, moderate particle energies For pairs : Charge symmetry condition - trigger on one, investigate the other Guenther Rosner BEACH 2006, Lancaster Univ. 22

Timelines n 2006: contract signed by participating countries n 2007/8: begin of construction n

Timelines n 2006: contract signed by participating countries n 2007/8: begin of construction n Phase I n n n q SIS 18 upgrade, CR, NESR, Super. FRS (RIB intensity factor 100 ) q NUSTAR, Plasma Physics (density factor 200 ) Phase II q SIS 100, RESR, HESR (stochastic cooling) q PANDA Phase III q SIS 300, HESR (electron cooling) q NUSTAR (RIB intensity factor 104 ), Plasma Physics (dens. fact. 2500 ) q PANDA high resolution, CBM Start of data taking (phase I, III) 2010 -15 Guenther Rosner BEACH 2006, Lancaster Univ. 23