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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)
4
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 intensitiesExtremely high vacuum ~10-13 mbar
Accelerator Challenges
Günther Rosner MESON2012, Krakow, 4/6/12
Brain Twister INo free quarks observed. They are confined in pairs or triplets in strongly interacting particles (hadrons).
Günther Rosner MESON2012, Krakow, 4/6/12 6
u d
u
Proton (p)938 MeV/c2
u d
d
Neutron (n)939 MeV/c2
ud
π- 140 MeV/c2
Baryons Mesons
Brain Twister IINormal (heavy) matter consists of pointlike, nearly massless quarks.
99% of the mass of the visible universe is, strictly speaking, energy!
Günther Rosner MESON2012, Krakow, 4/6/12 8
11
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
MESON2012, Krakow, 4/6/12 12
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+
16
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
APPA: Parity-Violation
Günther Rosner MESON2012, Krakow, 4/6/12 19
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
g NN
ee
Zee
NN
Select case with small splitting!
Large EM Fields
Günther Rosner MESON2012, Krakow, 4/6/12 20
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
Günther Rosner MESON2012, Krakow, 4/6/12 21
Particles / cm-3
Tem
per
atu
re [
eV]
Jupiter
LaserHeating
Sun Surface
Magnetic Fusion
solid statedensity
PHELIX
Sun Core
Inertial Fusion Energy
XFEL
SIS 18
Ion BeamHeating
SIS 100
Strongly coupled
plasmasIdeal plasmas
FLASH
ESA @ GSI & FAIR
Günther Rosner MESON2012, Krakow, 4/6/12 22
GCR Charge Contributions
Charge Number
0 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)
MESON2012, Krakow, 4/6/12 23
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
MESON2012, Krakow, 4/6/12 24
Modularised Start Version
Günther Rosner
APPA
CBM/HADES
NuSTAR
PANDAExperiments
M1: APPAM1: CBM/HADESM2: NuSTARM3: PANDA
M0
M1
M2M3
M3
MESON2012, Krakow, 4/6/12 25
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)
MESON2012, Krakow, 4/6/12 26
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€)
MESON2012, Krakow, 4/6/12 27
Timelines
Günther Rosner
20122011 2013 201620152014
6
Submission building permits
Site preparation
Civil construction contracts
Building of accelerator & detector components
Completion of civil construction work
Installation & commissioning of accelerators and detectors
Data taking
7 108
2017 2018 2019
12
6
7
8
9
11
12
10
119