September 19, 2006I. Augustin, GSI at PHIBADE 2006 Status of the FAIR Project I. Augustin FAIR Coordination Group GSI

September 19, 2006 I. Augustin, GSI at PHIBADE 2006

Status of the FAIR ProjectStatus of the FAIR Project

I. Augustin

FAIR Coordination Group

GSI

September 19, 2006 I. Augustin, GSI at PHIBADE 2006, Strasbourg

CDR Layout at pre-FAIR times

2001

700 authors

PANDA

Atom.Phys.

CBM

Plasma Phys. Low En. RIB Expt.

High En. RIB Expt.


Primary Beams

• All elements up to Uranium • Factor 100-1000 over present intensity• 50ns bunching

Secondary Beams

• Rare isotope beams up to a factor of 10 000 in intensity over present • Low and high energy antiprotons

• Beam cooling • Rapidly cycling superconducting magnets• Narrow bunching of beams

Key Technologies

Storage and Cooler Rings

• Rare isotope beams• e-– Rare Isotope collider

• 1011 stored and cooled antiprotons for Antimatter creation

International FAIR Project: the Intensity Frontier

Rare Isotope Production Target

AntiprotonProduction Target


Radioactive Ion Beam Programme Anti Proton Beam Programme

Relat. Ion Beam ProgrammePlasma Physics Beam Programme


Up to 4 fold Parallel Operation at FAIR !


PAC QCD E. Chiavassa

PAC NUSTAR R. Casten

PAC APPA D. Schwalm

TAC Y. Cho

Observers:

FAIR Project

CORECost Review Groups

D. Plane, W. Bartel

FCIFull Cost Issues

B. Brandt

AFI Working GroupAdministrative + Funding Issues

Ö. Skeppstedt

LFILegal Framework Issues

U.B. Jahn

STI Working GroupScientific + Technical Issues

H. Wenninger / S. Gales

ISCInternational Steering Committee

H. Schunck

The International Committee Structure of FAIRThe International Committee Structure of FAIR

MiniTACs• Cryogenics• Warm and Cold magnets• Power Supplies• Beam Instrumentation• p-Linac


Milestones 2003 Milestones 2003 –– 2006 2006


Baseline Technical Report Baseline Technical Report (April 2006)(April 2006)

> 3500 pages

Contributors:~ 2200 expt. scientists~ 400 accel. scientists

Investment costs:~ 1000 M€

Personnel needed:~ 2400 MY


FAIR

LAYOUT


What has changed?What has changed?

• readjusting of the beam rigidity (SIS300)

• optimizations injection and extraction of the synchrotrons

• rearrangement high energy beam transport system

• add storage ring (RESR) to achieve the accumulation and cooling performance

• antiproton injection into HESR at an energy of 3 GeV • accelerate/decelerate in HESR allowing direct injection from RESR


FLAIR@FAIR: Facility for Low energy Antiprotons and Ion Research

Originates from

CERN-AD program

100x more intensity than at CERN AD


STI Recommendations on STI Recommendations on ExperimentsExperiments

Experiment PAC Base Program Core Facility Comments

R3B NUSTAR yes yes

HISPEC/DESPEC NUSTAR yes yes

ILIMA NUSTAR yes yes

LASPEC NUSTAR yes yes

MATS NUSTAR yes yes

AIC NUSTAR no no open scientific & techn. issues

ELISe NUSTAR yes yes

EXL NUSTAR yes yes

NCAP NUSTAR no no request beam-time

EXO-pbar NUSTAR no no

PANDA QCD yes yes

CBM QCD yes yes

PAX QCD no no Strong scientific merit; could become part of base program

ASSIA QCD no no Consider joining PAX

LAPLACE/HIHEX/WDM APPA yes yes should merge under one umbrella

FLAIR APPA no yes not part of the initial CDR

SPARC APPA yes yes

BIOMAT APPA yes yes


Accelerator Physics and Technology for FAIRAccelerator Physics and Technology for FAIRMain R&D challengesMain R&D challenges

Superconducting, fast ramping synchrotron magnets

High gradient, low frequency RF cavities

Fast stochastic and electron cooling

Novel lattice/collimation design: Beam optics studies

Control of collective effects:Large scale simulation studies

Ultra high vacuumfor intense beams

HESR e-cooler

SIS 100 dipole magnet

CR compressor cavity

control of stripping losses

Desorption test-stand Working pointdiagram:Stabilityof intensebeams


Critical Path IssuesCritical Path Issues

Negotiations and agreements with FAIR partners:

• Decisions on NESR, RESR magnet technology (warm or cold) in autumn of 2006 Spain• If decision for NESR and RESR superconducting, prototype for end of 2008 Spain • CR and Super FRS sc-dipole prototypes in 2008 China• SIS 300 decision for or against curved magnets probably end of 2006 Italy, Russia• SIS 300 sc magnets prototype a) straight magnets 2008, b) curved magnets 2008/9 Italy,

Russia• SIS 300 sc quadrupoles prototype 2008/9 France, CEA and

IN2P3• SIS 100 sc magnet prototype 2008 Russia, Industry,

GSI• HESR curved sc magnets, feasibility study end 2006, prototype in 2008 Industry, Jülich• Design Super FRS Triplets 2007 Industry, GSI• Prototype Super FRS Triplet 2008 Industry, GSI• SUPER FRS Energy Buncher dipoles, delivery end of 2009 India


Scope of CNI: FAIR injector SIS18intensity upgrade (HADES, R3B)

Scope of Design Study: secondary beams (RIB and Antiprotons)

I3 programmes in the 6th FP I3HP, EURONS,

R&D funding issues: FAIR - EU support

SIS100/SIS300

HESR

PANDA

(I3HP)

CR

GSIAcceleratorFacilities

NESR

Super- FRS

HADES* / CBM I3HP

NUSTAR EURONS

HADES*

R3B

R3B

SIS18

EU R&D funding FAIR related amounts to 32 M€


FAIR Master Schedule

Adapted to Civil Construction Schedule

Critical Path:Availability of buildings to start installations(Subjected for further optimization)

Actual planning allows for: First experiments at sFRS 2011/2012 Project end 2014/2015


Stage 1

(2007- 2011)

Civil Construction Activity

Radioactive beam physics

•Nuclear structure and nuclear astrophysics•Atomic physics studies with highly charged/radioactive ions & plasma physics


Stage 2

(2011- 2013)

Civil Construction Activity

Proton-antiproton physics•QCD studies with protons and antiprotons•Precision studies with antiproton beams addressing fundamental symmetries and interactions•FLAIR

Relat. Heavy Ions•1-10AGeV relat. heavy ion beams for atomic and nuclear collision studies, e.g. with HADES


Stage 3

(2013- 2015)

No Civil Construction Activity anymore

Full facility capability & all research programs

•Full parallel operation of up to four research programs •Full energy and luminosity for nuclear collisions program at CBM•Precision QCD Studies at PANDA up to 15 GeV/c •Plasma research (full gain factor in power density: ~400)•Atomic reaction studies with fast beams

September 19, 2006 I. Augustin, GSI at PHIBADE 2006

Proposed FAIR – Roadmap: Establishment of FAIR GmbH

Contracting Parties

Share-holders (SH)

Bylaw Subgroup

AFI

ISC

STI

IKAB

Joint Core-Team

07/06 08 09 10 11 12 01/07 02 03 04 05 06

Nomination of Shareholders + Completion

of negotiations

Completion of draft Bylaws

Signature of Convention

and Final Act

Signature AoA

STI

AFI AFI

joint meeting ISC/SHISC ISC

Bylaws, draft FAIR GmbH structure and

kick-off staffing

Convention, Final Act, AoA;

Joint Core Team

Technical evaluation of potential in-kind contributions (ongoing process up to the formation of FAIR GmbH)

Mandate for IKAB

Monitoring of technical planning and project costs (ongoing process up to the formation of FAIR GmbH)

Elaboration of the Bylaws (ongoing)

ConventionFinal Act AoA

First meeting: start senior

staffing

Constitutive Meeting of the

Council

Convention, Final Act, AoA;

Bylaws (first draft)

Bylaws, draft FAIR structure

Technical project decisions (follow up design changes) / FAIR preparation tasks (ongoing process up to the foundation of FAIR GmbH)

Formation FAIR GmbH

Negotiations (ongoing, 'till end of 2006)

meetings


Thank you for your attention!


Parameters for end of commissioning / start of operation (I)


Parameters for end of commissioning / start of operation (II)


There are other IN-FLIGHT and ISOL facilities availabe - WHY FAIR ?

The FAIR accelerators will provide beams with the following characteristics:

Full range of ion beam species plus antiprotons: The facility will accelerate all ions from protons (and also antiprotons) up to heaviest elements, uranium. This will provide the necessary broad basis for the multi-disciplinary research program for FAIR.

Highest beam intensities: Intensities of primary heavy-ion beams will increase by a factor of 100, secondary radioactive beams by a factor of up to 10,000 over the present GSI facility, pushing forwards the sensitivity of experiments

Substantial increase in beam energy: An increase by about a factor of 20 in energy is foreseen for beams as heavy as uranium. In this energy regime nucleus-nucleus collisions are expected to generate hadronic matter at the highest densities This enables unique studies of charm production in highly compressed matter.

Generation of precision beams: These will be stochastic and electron cooling of ion beams, in particular also applicable to the secondary radioactive and antiproton beams. Together with the statistical precision and high sensitivity that results from high beam intensities and interaction rates, the precision-quality beams will allow entering totally new areas of research in all of the FAIR science fields.

Synchrotrons and storage rings as accelerator structures of choice: For ion beams, ranging from protons to uranium, synchrotrons provide the most economical solution to generate very high beam energies. Even more important for the FAIR research program, accelerator rings are unique in their capability to store, cool, bunch, and stretch beams.


Five Research Communities at Five Research Communities at FAIRFAIR

100 m

High EM Field (HI) _Fundamental Studies (HI & p)Applications (HI)

Plasma Physics: x600 higher target energy density 600kJ/g

Nuclear Matter Physics with35-45 GeV/u HI beams, x1000

Hadron Physicswith antiprotons of 0 - 15 GeV

SIS 100/300

HESR

SuperFRS

NESR

CBMHADES

FLAIRCR- RESR

Rare Isotope Production Target

AntiprotonProduction Target

Nuclear Structure & Astrophysicswith radioactive beams, x10 000and excellent cooling

Documents

September 19, 2006I. Augustin, GSI at PHIBADE 2006 Status of the FAIR Project I. Augustin FAIR Coordination Group GSI