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).

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

Narrow Hadronic States

Günther Rosner MESON2012, Krakow, 4/6/12 7

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

Günther Rosner MESON2012, Krakow, 4/6/12

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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

Günther Rosner MESON2012, Krakow, 4/6/12 31