Facility for Antiproton and Ions Research Saudi Arabia FAIR

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Facility for Antiproton and Ions Research
Saudi Arabia
FAIR project Roadmap to FAIR GmbH foundation

• Facility - new scenario of the project
  realization
• Research program at the Modularized Start
  Version
• Roadmap to FAIR GmbH foundation

Helmholtz Centre for Ion Research
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• Late 1990s
• GSI researchers began discussion with the 1200
  outside users

• 2001
• GSI had drawn up the Conceptual Design Report for
  a new facility

• Spring 2006
• STI presented FAIR Baseline Technical Report -
  2400 authors 45 countries

http//www.gsi.de/fair/reports/btr.html
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(No Transcript)
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New accelerator systems to be constructed
10 000 x For radioactive ion beams
1000 x For primary HI beams
Synchrotrons SIS100 SIS300
FAIR multi-purposes, state of the art
facility
p - LINAC
Highest quality and intensity beams!
High-Energy Storage Ring HESR
Superconducting large-acceptance Fragment
Separator Super-FRS
100 x For cooled antiprotons
Collector Ring CR
New Experimental Storage Ring NESR
Recycled Exp. Storage Ring RESR
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From Summary Record of 8th ISC Meeting, July 24,
2006, Berlin To the FAIR core facility
belong the experiments of the 14 approved
technical proposals (see table).
The main research thrust of FAIR focuses on the
structure and evolution of matter on both a
microscopic and a cosmic scale
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FAIR Research
George Gamov
Fred Hoyle
Quar-gluon soup lept., neutr., fot., graw.,
The evolution of the universe
TK 1 TeV 1016 1 GeV 1013 1 MeV
1010 1 KeV 107 1 eV 104 1 meV 10
Nuclei
Parlicles
Atoms
10-12 10-6 1
106 1012
1018 ts
Today 13.7 bln y. later
FAIR QCD research programs
(Quantum Chromodynamics
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QCD Research Program
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FAIR Research -NuSTAR
Quar-gluon soup lept., neutr., fot., graw.,
TK 1 TeV 1016 1 GeV 1013 1 MeV
1010 1 KeV 107 1 eV 104 1 meV 10
Nuclei
Parlicles
Atoms
Sun 5 bln y. ago
10-12 10-6 1
106 1012
1018 ts
Today 15 bln y. later
FAIR NUSTAR research programs (Nuclear
Structure, Astrophysics and Reactions
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Nuclear Structure, Astrophysics and Reactions -
NuSTAR
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FAIR Research - APPA
Quar-gluon soup lept., neutr., fot., graw.,
TK 1 TeV 1016 1 GeV 1013 1 MeV
1010 1 KeV 107 1 eV 104 1 meV 10
Nuclei
Parlicles
Atoms
Sun 5 bln y. ago
10-12 10-6 1
106 1012
1018 ts
Today 15 bln y. later
FAIR APPA research programs(Atomic ,Plasma
Physics and Applications)
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Atomic Physics, Plasma Physics and Applications
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Construction Period, Cost, Users

• Construction until 2018
• Total cost 1.2 B (2005 prices)
• Scientific users 2500 - 3000 per year

Financing

• up to 65 Federal Government of Germany
• 10 State of Hessen
• 25 Partner Countries

FAIR GmbH with International Shareholders
Project Costs scrutinized by CORE, TAC, STI as
basis how to account in-kind contributions
Operation cost will be negotiated in 3
years after FAIR GmbH will be established
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New cost estimates in 2009

• Detailed cost estimate for CC presented by
  architects
• New cost estimate for the accelerator complex
  presented by TD
• Detailed list of site related construction
  costs was worked out

• Germany and State of Hesse announced to cover
  "site-dependent
• construction costs outside FAIR project budget
  110 M !

Firm commitments of FAIR Member States
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Development of Project Staging
The Modularized Start Version
Outstanding research opportunities should be
offered to all four scientific pillars of FAIR by
the Modularized Start Version
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Module 0 SIS100 and connection to existing GSI
accel.
APPA
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CBM/HADES
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 1 Experimental areas for CBM/HADES and
APPA
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CBM/HADES
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 1 Experimental areasfor CBM/HADES and
APPA
Module 2 Super-FRS, fixed target branch
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CBM/HADES
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 1 Experimental areas for CBM/HADES and
APPA
Module 2 Super-FRS , fixed target branch
Module 3 High-energy antiprotons (p-linac,
pbar-target, CR, HESR)
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CBM/HADES
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 4 Low energy RIB and low energy
antiprotons
Module 1 Experimental areas for CBM/HADES and
APPA
Module 2 Super-FRS , fixed target branch
Module 3 High-energy antiprotons (p-linac,
pbar-target, CR, HESR)
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CBM/HADES
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 4 Low energy RIB and low energy
antiprotons
Module 1 Experimental areas for CBM/HADES and
APPA
Module 5 RESR storage ring
Module 2 Super-FRS , fixed target branch
Module 3 High-energy antiprotons (p-linac,
pbar-target, CR, HESR)
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CBM/HADES
Modularized Start Version
Module 0 SIS100 and connection to existing GSI
accel.
APPA
Module 4 Low energy RIB and low energy
antiprotons
Module 1 Experimental areas for CBM/HADES and
APPA
Module 5 RESR storage ring
Module 2 Super-FRS , fixed target branch
Module 3 High-energy antiprotons (p-linac,
pbar-target, CR, HESR)
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The Modularized Start Version should
enablerealization of research program of all
scientific FAIR communities.
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Science with the Modularized Start Version
APPA
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Construction Roadmap
Coasting aspects
Total cost of modules 0, 1, 2 and 3
1.027.000
Firm commitments from FAIR partners 1.038.660

• Start of construction activities 2010/11
• Schedule is driven by civil construction
• Aim for earliest commissioning of accelerators
• and respective experiments

Ready for installation
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Summary CBM/HADES at FAIR

• Physics program with large discovery potential
  at Module 0,1
• Exploring the equation-of-state of nuclear
  matter at neutron star densities
• with multistrange hyperons.
• First measurements of lepton pairs at SIS100
  energies to study the modification
• of hadron properties in dense nuclear matter,
  and the electromagnetic structure
• of dense nuclear matter.
• Searching for strange matter.
• First measurement of charm production and
  propagation at threshold energies.
• Full version of FAIR
• Mapping the QCD phase diagram, and searching for
• the deconfinement and chiral phase transitions,

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Module 0-3 p-bar induced reactions studied with
FAIR have an enormous impact in particle physics
Summary PANDA Collaboration
All qq states can be formed directly (not only
1--) - discovery potential pp cross section is
high - precision studies 1st time High
probability for production of exotic states - 2
states 1- are predicted Low final state
multiplicities - allows complete PWA Nucleon
structure can be studied - via electromagnetic

processes

Module 5 additional research opportunities
Higher luminosity Maximizes the yield, and then
rare phenomena can be studied
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Module 0-3 Unique Research Opportunities to
Study Nuclear Structure and Dynamics and Nuclear
Astrophysics
Summary NuSTAR Collaboration
R3B full program, reactions at relativistic
energies, complete
kinematics ILIMA unique measurements of masses
and half-lives in the CR HISPEC,DESPEC in-beam
(50-100 AMeV) decay spectroscopy MATS, LASPEC
precision ground state properties

Modules 4 and 5 Additional Research Opportunities
ILIMA cooled beams, unique decay modes, isomeric
beams in NESR EXL elastic and inelastic
scattering on internal H, He target in
NESR HISPEC energy buncher access to heavier
nuclei, low-energy beams MATS, LASPEC energy
buncher faster extraction, cleaner beams
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Module 1Unique research opportunities for
atomic-, bio-, and plasma-physics as well as
applied sciences(BIOMAT, HEDgeHOB/WDM, SPARC)
Summary APPA Collaborations
Highest Charge States Extreme static
fieldsRelativistic Energies Extreme
dynamical fields and ultrashort pulsesHighest
Intensities Very high energy densities and
pressures
Modules 4 and 5 Additional Research Opportunities
SPARC Precision studies using cooled, stored and
trapped ions
FLAIR Most intense source of low-energy
antiprotons will be accessible
HEDgeHOB/WDM Diagnostic tools of high power
laser and of proton radiography
are optional
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FAIR Science Review Committee

Siegfried Grossmann
Nigel Lockyer

Alex Mueller
Guenther Rosner

Robert Rosner (chair)
Committee met on 16 October, 2009 at
GSI/Darmstadt having received its charge from
Dr. Beatrix Vierkorn-Rudolph (BMBF/Germany).
The oral statement of the Committee says The
panel's belief that a realization of modules 0
3 will provide a facility that offers a broad
and excellent scientific program with a strong
potential for all four scientific pillars of FAIR
from early on.
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Reported by Arne Jungstand
The cost estimates performed in 2009 are
realistic and form a reliable basis for further
evolution the FAIR project.
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FAIR ISC met on 29nd October 2009.Based on
statements by AFI and STI, ISC adopted the
following resolutionThe construction of FAIR
shall start with the Modularized Start Version as
described in the White Paper.
FAIR STI Working group met on 22nd October 2009
and evaluated in depth the White
Paper. Conclusions STI has evaluated the
FAIR Modularized Start Version including science
case, costing and roadmap as defined in the White
Paper. It considers the project scientifically
exciting and financially mature. STI suggests to
implement it expeditiously.
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Construction of FAIR
The Modularized Start Version secures a swift
start of FAIR construction.
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History of FAIR Site Building Activities
1998 2001 Discussions on the future of GSI
2002 FAIR CDR evaluated by
Wissenschaftsrat 2005 Preparations
for a international large scale project
International Steering Committee
(ISC) 2005 B-Plan changes approved
by city of Darmstadt 2006 Project
definition by ISC (FBTR) 2007 Approval by
GSI-AR to start pre-planning, i.e.
EU-call for tender on steerer, engineers
and architects together with
CC hbm Fulda 2007 ISC task to plan
for the full version of FAIR
Antrag auf Einleitung ZBau-Verfahren
2008 BMBF approves Raumprogramm for full
version with identifying
Start Version buildings. 2009 Working
out pre-planning documents (HUBau)
handed over to hbm in September.
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Civil Construction Documents for the Full Version
120 folders of planning documents handed to hbm
for approval
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Birds Eye View on FAIR Full-Version
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Where do we Stand?

• Pre-planning of full FAIR building now with hbm
  for approval
• Dec. 2009
• New room-program for Modules 0 3 incl.
  APPA-hall ?
• Have it approved by BMBF
• Start with new pre-planning of Modules 0 3
  (April 2010)
• Hand documents as textures to hbm
  (July 2010)
• Start approval documents
  (Sept 2010)
• Apply for building permit
  (Dec 2010/Jan 2011)

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New GSI structure presented by H. Stöcker and B.
Vierkorn-Rudolph in the co-workers assembly 19
January 2010.

• FAIR structure will be established within GSI
  GmbH as the
• dedicated FAIR division (present preparatory
  phase)

• Boris Sharkov will head the division as 4th GSI
  Managing Director
• (with specific responsibility for all
  FAIR-related issues)

• FAIR Division will later be separated from GSI
  and
• will form the FAIR GmbH

• It is foreseen that the existing personnel in
  the FAIR Division will
• be transferred from GSI to FAIR GmbH.

• Distribution of Work Packages between GSI and
  FAIR is in progress
• (Joint (GSIFAIR) preparation of the
  Business Management Contract
• draft with the aim to deliver it to AFI by
  mid of April 2010.)

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Responsible for all civil construction
matters FAIR will have direct control of
significant budget fraction
Employment of APPA, CBM, NuSTAR and PANDA
technical and resource coordinators
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Roadmap to FAIR GmbH foundation

• The status of the translation process of the
  founding documents
• BMBF is now harmonized the German and English
  versions of the texts
• The documents are expected to be sent out to the
  other countries which
• require own language versions (France, Russia,
  Spain) by the German
• Foreign Office.
• At the same time the English version will be
  provided to all the Delegations.

The translations might be formally agreed on by
end of March, leading to a translation\initialing
conference end of April 2010
If this works out, the FAIR signing ceremony
could finally take place eight weeks later,
i.e., end of June or beginning of July 2010.
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What limps - moves
Co kuleje - idzie.
Stanislaw Lec (1909-1966) Baron Stanislaw Jerzy
de Tusch-Letz