Status of the FAIR Project Status of the FAIR Project I. Augustin - - PowerPoint PPT Presentation

status of the fair project status of the fair project
SMART_READER_LITE
LIVE PREVIEW

Status of the FAIR Project Status of the FAIR Project I. Augustin - - PowerPoint PPT Presentation

Status of the FAIR Project Status of the FAIR Project I. Augustin FAIR Coordination Group GSI September 19, 2006 I. Augustin, GSI at PHIBADE 2006 CDR Layout at pre-FAIR times 2001 700 authors PANDA Low En. RIB Expt. Plasma Phys. High


slide-1
SLIDE 1

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006

Status of the FAIR Project Status of the FAIR Project

  • I. Augustin

FAIR Coordination Group GSI

slide-2
SLIDE 2

CDR Layout at pre-FAIR times 2001 700 authors

PANDA Atom.Phys. CBM Plasma Phys. Low En. RIB Expt. High En. RIB Expt.

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-3
SLIDE 3

International FAIR Project: the Intensity Frontier

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

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

  • ver 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 Rare Isotope Production Target Antiproton Production Target

slide-4
SLIDE 4

Radioactive Ion Beam Programme Anti Proton Beam Programme Plasma Physics Beam Programme

  • Relat. Ion Beam Programme

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-5
SLIDE 5

Up to 4 fold Parallel Operation at FAIR !

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-6
SLIDE 6

The International Committee Structure of FAIR The International Committee Structure of FAIR

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

PAC QCD E. Chiavassa PAC NUSTAR R. Casten PAC APPA D. Schwalm TAC Y. Cho

Observers:

FAIR Project

CORE

Cost Review Groups

  • D. Plane, W. Bartel

FCI

Full Cost Issues

  • B. Brandt

AFI Working Group

Administrative + Funding Issues

Ö. Skeppstedt

LFI

Legal Framework Issues

U.B. Jahn

STI Working Group

Scientific + Technical Issues

  • H. Wenninger / S. Gales

ISC

International Steering Committee

  • H. Schunck

MiniTACs

  • Cryogenics
  • Warm and Cold magnets
  • Power Supplies
  • Beam Instrumentation
  • p-Linac
slide-7
SLIDE 7

Milestones 2003 Milestones 2003 – – 2006 2006

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-8
SLIDE 8

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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-9
SLIDE 9

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

FAIR LAYOUT

slide-10
SLIDE 10

What has changed? What has changed?

  • readjusting of the beam rigidity (SIS300)
  • ptimizations 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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-11
SLIDE 11

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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

Originates from CERN-AD program

100x more intensity than at CERN AD

slide-12
SLIDE 12

STI Recommendations on STI Recommendations on Experiments Experiments

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

  • pen 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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-13
SLIDE 13

Accelerator Physics and Technology for FAIR Accelerator Physics and Technology for FAIR

Main R&D challenges Main R&D challenges

Novel lattice/collimation design: Beam optics studies High gradient, low frequency RF cavities Superconducting, fast ramping synchrotron magnets

control of stripping losses SIS 100 dipole magnet CR compressor cavity September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

Control of collective effects: Large scale simulation studies Ultra high vacuum for intense beams Fast stochastic and electron cooling

Working point diagram: Stability

  • f intense

beams Desorption test-stand HESR e-cooler

slide-14
SLIDE 14

Critical Path Issues Critical 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 September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-15
SLIDE 15

R&D funding issues: FAIR - EU support

Scope of CNI: FAIR injector SIS18 intensity upgrade (HADES, R3B) Scope of Design Study: secondary beams (RIB and Antiprotons) I3 programmes in the 6th FP I3HP, EURONS,

SIS100/SIS300

HESR

PANDA (I3HP)

CR

GSI Accelerator Facilities

NESR

Super- FRS

HADES* / CBM I3HP NUSTAR EURONS HADES* R3B R3B

SIS18

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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-16
SLIDE 16

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

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

slide-17
SLIDE 17

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

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

slide-18
SLIDE 18

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

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

slide-19
SLIDE 19

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg

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

slide-20
SLIDE 20

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006

Proposed FAIR – Roadmap: Establishment of FAIR GmbH

07/06 08 09 10 11 12 01/07 02 03 04 05 06 Nomination of Shareholders + Completion

  • f negotiations

Completion

  • f draft

Bylaws Signature of Convention and Final Act Signature AoA

STI AFI AFI joint meeting ISC/SH ISC 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) Convention Final 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

Contracting Parties Share- holders (SH) ISC AFI STI Bylaw Subgroup Joint Core- Team IKAB

slide-21
SLIDE 21

Thank you for your attention!

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-22
SLIDE 22

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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-23
SLIDE 23

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

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-24
SLIDE 24

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.

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg
slide-25
SLIDE 25

Five Research Communities at Five Research Communities at FAIR FAIR

100 m

High EM Field (HI) _ Fundamental Studies (HI & p) Applications (HI) Plasma Physics: x600 higher target energy density 600kJ/g Nuclear Matter Physics with 35-45 GeV/u HI beams, x1000 Hadron Physics with antiprotons

  • f 0 - 15 GeV

SIS 100/300

HESR Super FRS NESR CBM HADES FLAIR CR- RESR

Rare Isotope Production Target Antiproton Production Target

Nuclear Structure & Astrophysics with radioactive beams, x10 000 and excellent cooling

September 19, 2006

  • I. Augustin, GSI at PHIBADE 2006, Strasbourg