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The Facility for Antiprotonand Ion Research in Europe
Günther Rosner MESON2012, Krakow, 4/6/12 1
FAIR @ Darmstadt
Günther Rosner MESON2012, Krakow, 4/6/12 2
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Facility for Antiproton & Ion Research
Günther Rosner MESON2012, Krakow, 4/6/12
Dense Bulk Plasmas (Ion-beam bunch compression& petawatt-laser)
Materials Science & Radiation Biology (Ion & antiproton beams) Accelerator Physics
UNILAC
SIS18 SIS100/300p-Linac
HESR
CR &RESR
NESR
Cryring
Rare-IsotopeProduction Target
Anti-ProtonProduction Target
100 m
QCD-Phase Diagram(HI beams 2 to 45 GeV/u)
Hadron Physics (Stored and cooled14 GeV/c anti-protons)
Nuclear Structure & Astrophysics(Rare-isotope beams)
Fundamental Symmetries& Ultra-High EM Fields(Antiprotons & highly stripped ions)
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Fast accelerationHigh gradient, variable frequency
Ferrite & MA loaded cavities
Compact & cost effective acceleratorsFast cycling superconducting magnets
dB/dt ~ 4T/s
Precision beamsElectron & stochastic cooling XHV @ high beam intensities
Extremely high vacuum ~10-13 mbar
Accelerator Challenges
Günther Rosner MESON2012, Krakow, 4/6/12
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FAIR Experiments
Günther Rosner MESON2012, Krakow, 4/6/12
CBM
PANDANuSTAR
Super-FRS
APPA
Brain Twister INo free quarks observed. They are confined in pairs or triplets in strongly interacting particles (hadrons).
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u d
u
Proton (p)938 MeV/c2
u d
d
Neutron (n)939 MeV/c2
ud
π- 140 MeV/c2
Baryons Mesons
Narrow Hadronic States
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PANDA @ FAIR
Brain Twister IINormal (heavy) matter consists of pointlike, nearly massless quarks.
99% of the mass of the visible universe is, strictly speaking, energy!
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Anti-Proton Annihilation @ DA
Günther Rosner MESON2012, Krakow, 4/6/12
PANDA
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Gluonic excitations
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Search for Heavy Glueballs• “Charmed” glueballs
– flavour blind decays• charmed final states!
– only a few charmed mesons around 3 - 4 MeV/c2
• less mixing!
• Exotic glueballs (oddballs), no mixing!– m(2+-) = 4140(50)(200) MeV– m(0+-) = 4740(70)(230) MeV– decay modes , , J/, J/ – Narrow widths predicted
Günther Rosner MESON2012, Krakow, 4/6/12
Morningstar & Peardon, PRD60(1999)34509Morningstar & Peardon, PRD56(1997)4043
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PANDA & CBM: Hadrons in Nuclei• Partial restoration of chiral
symmetry in nuclear matter Light current quarks sensitive to
quark condensate• Charmonium states
Sensitive to gluon condensate Significant mass shifts expected for
c, ’, (3770): 40, 100, 140 MeV/c2 resp.
• D mesons: the QCD analogue of an H-atom Chiral symmetry to be studied on a
single light quark Theoretical calculations disagree in
size and sign of mass shift (50 MeV/c2 attractive vs. 160 MeV/c2 repulsive)
Günther Rosner
Vacuum Nuclearmedium
p
K
25 MeV
100 MeV
K+
K-
p-
p+
Hayaski, PLB 487 (2000) 96Morath, Lee, Weise, priv. Comm.
D-50 MeV
D
D+
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Compressed Baryonic Matter
Günther Rosner
SIS100/300
CBM @ FAIR
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High Baryon Density @ CBM
Günther Rosner
Probes of Dense Phase
No data so far FAIR Range
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NuSTAR
Günther Rosner MESON2012, Krakow, 4/6/12
NuSTAR
Super-FRS
Secondary Beams: Broad range of radioactive ion beams ≤ 2 GeV/u RI- Intensities up to 10 000 over present
Primary HI Beams:• 40Ar18+ 2x1012/s @ 1 – 2 GeV/u• 238U28+: 5x1011/s @ 1 – 2 GeV/u• 40Ar18+ 2x1010/s @ 1 – 45 GeV/u• 238U92+: 1x1010/s @ 1 – 35 GeV/u100 x 1000 times current intensity
GSI FRS FAIR Super-FRS
Günther Rosner MESON2012, Krakow, 4/6/12 171000 7500
Super-FRS
FRS
NuSTAR
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APPA: Parity-Violation
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PS
PNWFS
EE
QG
-
522/
Mixing coefficient for states with opposite parities:
Energy levels of He-like uranium
2E1 (PNC)
To “compete” with spontaneous decay channels one needs to induce a two-
photon PNC transition by polarised light with intensity 1020 W/cm2
NN
ee
Zee
NN
Select case with small splitting!
Large EM Fields
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Sub-fs pulses
Lasers
(adapted from Mourou, Tajima, Bulanov, RMP 78, 2006)
Heavy ions
Large EM fields, zs pulses
Equivalent toI ≥ 1028 W/cm2
Plasmas
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Particles / cm-3
Tem
pera
ture
[eV
]
Jupiter
LaserHeating
Sun Surface
Magnetic Fusion
solid statedensity
PHELIXSun Core
Inertial Fusion Energy
XFEL
SIS 18
Ion BeamHeating
SIS 100
Strongly coupled
plasmasIdeal plasmas
FLASH
ESA @ GSI & FAIR
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GCR Charge Contributions
Charge Number0 5 10 15 20 25 30
% C
ontr
ibut
ion
0.001
0.01
0.1
1
10
100
FluenceDoseDose Eq.
Free Space
Durante & Cucinotta, Nature Rev. Cancer (2008)
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Staging
Günther Rosner
Start Version Phase A(SIS100) Phase B
(SIS300)
Modularised Start Version
Module 0 Module 1 Module 2 Module 3 Module 4 Module 5
SIS100 Exp. halls CBM & APPA
Super-FRS NuSTAR
Antiproton FacilityPANDA & options NuSTAR
LEB, NESR, FLAIR
NuSTAR & APPA
RESRPANDA,
NuSTAR & APPA
2017/18
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Modularised Start Version
Günther Rosner
APPA
CBM/HADES
NuSTAR
PANDAExperiments
M1: APPAM1: CBM/HADESM2: NuSTARM3: PANDA
M0
M1
M2M3
M3
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Costs MSV
Günther Rosner
Accelerators and personnel (including Super-FRS) 502 M€
Civil construction (excluding site related costs) 400 M€
FAIR contribution to experimental end stations * 78 M€
FAIR GmbH personnel & running until 2018 (>8 years) 47 M€
Grand Total MSV, Modules 0 - 3 1027 M€
in 2005 € (inflation escalation until 2018: ca. +50%)
* Total experimental end stations (excluding Super-FRS): ca. 210 M€ (2005) = 315 M€ (2018)
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Funding Modules 0-3Contracting Party Contribution
(in 2005 M€)Finland 5.00
France 27.00
Germany 705.00
India 36.00
Poland 23.74
Romania 11.87
Russia 178.05
Slovenia 12.00
Sweden 10.00
Total 1.008,66
Günther Rosner
• All numbers in 2005 €(escalation until 2018 ca. +50%)
• Spain expected to join soon (with 11.87 M€)
• China and the UK are potential Associate FAIR Members and will contribute to the experiments (6.6 M€)
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Timelines
Günther Rosner
20122011 2013 201620152014
6
Submission building permitsSite preparationCivil construction contractsBuilding of accelerator & detector componentsCompletion of civil construction workInstallation & commissioning of accelerators and detectorsData taking
7 108
2017 2018 2019
12
6
7
89
11
12
10
119
Civil Construction
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Start Clearing 6/12/2011
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Test Drilling 31/8/2011
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Thank you very much
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