ria summer school 2006 exotic beam production and facilities ii brad sherrill, michigan state...
TRANSCRIPT
RIA Summer School 2006
Exotic Beam Production and Facilities II
Brad Sherrill, Michigan State University
Lecture I• The Rare Isotope Accelerator Concept• Some history and background• The status of exotic beam plans in the USA
Lecture II• Methods of exotic beam production• Production mechanisms (e.g. fragmentation)• Current world situation for exotic beams
Brad Sherrill, Michigan State University
Lecture I• The Rare Isotope Accelerator Concept• Some history and background• The status of exotic beam plans in the USA
Lecture II• Methods of exotic beam production• Production mechanisms (e.g. fragmentation)• Current world situation for exotic beams
RIA Summer School 2006
Production Mechanisms
• In-flight Separation
• ISOL – Isotope Separation On-Line
• Neutron induced fission (2-step target)
• In-flight Separation
• ISOL – Isotope Separation On-Line
• Neutron induced fission (2-step target)
Post Acceleration
Driver AcceleratorFragment Separator
beam
Gas cell catcher/ion source
Driver
DriverTarget/Ion Source
Neutrons
Post Acceleration
Post Acceleration
Beams used without stopping
RIA Summer School 2006
• Good Beam quality ( mm-mr vs. 30 mm-mr transverse)
• Small beam energy spread for fusion studies
• Can use chemistry (or atomic physics) to limit the elements released
• 2-step targets provide a path to MW targets
• High beam intensity leads to 100x gain in secondary ions
• Good Beam quality ( mm-mr vs. 30 mm-mr transverse)
• Small beam energy spread for fusion studies
• Can use chemistry (or atomic physics) to limit the elements released
• 2-step targets provide a path to MW targets
• High beam intensity leads to 100x gain in secondary ions
Advantages/Disadvantages of ISOL/In-Flight
• Provides beams with energy near that of the primary beam
– For experiments that use high energy reaction mechanisms
– Luminosity (intensity x target thickness) gain of 10,000
– Individual ions can be identified
• Efficient, Fast (100 ns), chemically independent separation
• Production target is relatively simple
• Provides beams with energy near that of the primary beam
– For experiments that use high energy reaction mechanisms
– Luminosity (intensity x target thickness) gain of 10,000
– Individual ions can be identified
• Efficient, Fast (100 ns), chemically independent separation
• Production target is relatively simple
In-flight:GSIRIKENNSCLGANIL
ISOL:HRIBFISACSPIRALISOLDE
400kW protons at 1 GeV is 2.4x1015 protons/s
RIA Summer School 2006
• (p,n) (p,nn) etc. o Ep < 50 MeV
o Used for the production of medical isotopes. o Selective, large production cross sections (100 mb), and
intense (500 A) primary beams.o Used at HRIBF(ISOL), LLN (ISOL), ANL (in-flight) and
Notre Dame (in-flight), Texas A&M (in-flight)
• Fusiono Low energy 5-15 MeV/A and “thin” targetso Selective with fairly large production cross sections.o Used at ANL(in-flight), JYFL (Jyväskylä)
• (p,n) (p,nn) etc. o Ep < 50 MeV
o Used for the production of medical isotopes. o Selective, large production cross sections (100 mb), and
intense (500 A) primary beams.o Used at HRIBF(ISOL), LLN (ISOL), ANL (in-flight) and
Notre Dame (in-flight), Texas A&M (in-flight)
• Fusiono Low energy 5-15 MeV/A and “thin” targetso Selective with fairly large production cross sections.o Used at ANL(in-flight), JYFL (Jyväskylä)
Production Methods – Low Energy
RIA Summer School 2006
• High, specific production cross sections
• Example: 58Ni(3He,n)60Zn, EHe = 100 MeV
o Production cross section from ALICE: 100 bo 4 g/cm2 targeto Yield of 60Zn is 3x107/pA (LBL 88-inch has 10 pA of
3He)o Heavier beams can have larger cross sections, but require
thinner targets.
• High, specific production cross sections
• Example: 58Ni(3He,n)60Zn, EHe = 100 MeV
o Production cross section from ALICE: 100 bo 4 g/cm2 targeto Yield of 60Zn is 3x107/pA (LBL 88-inch has 10 pA of
3He)o Heavier beams can have larger cross sections, but require
thinner targets.
Example of production by fusion
RIA Summer School 2006
• Transfer reactionso Significant cross section between 10 - 50 MeV/A (this energy
range implies thin targets, mg/cm2)o High production of nuclei near stability.o Multi-nucleon reactions can be used to produce rare or more
neutron rich nuclei, e.g. GSI mass separator had a program to study neutron rich f-p shell nuclei using neutron transfer.
• Deeply inelastic reactionso Deep inelastic - much of the KE of the beam is deposited in the
target.o Was used to first produce many of the light neutron rich nucleio Is used to study neutron rich nuclei since the products are
“cooler” and fewer neutrons are evaporated than in fusion reactions.
• Transfer reactionso Significant cross section between 10 - 50 MeV/A (this energy
range implies thin targets, mg/cm2)o High production of nuclei near stability.o Multi-nucleon reactions can be used to produce rare or more
neutron rich nuclei, e.g. GSI mass separator had a program to study neutron rich f-p shell nuclei using neutron transfer.
• Deeply inelastic reactionso Deep inelastic - much of the KE of the beam is deposited in the
target.o Was used to first produce many of the light neutron rich nucleio Is used to study neutron rich nuclei since the products are
“cooler” and fewer neutrons are evaporated than in fusion reactions.
Low Energy - Continued
RIA Summer School 2006
• Fragmentation (NSCL, GSI, RIKEN, GANIL)o Projectile fragmentation of high energy (>50 MeV/A) heavy ionso Target fragmentation of a target with high energy protons or light HIs. In
the heavy ion reaction mechanism community these are called intermediate mass fragments.
• Spallation (ISOLDE, TRIUMF-ISAC)o Name comes from spalling or cracking-off of target pieces.o One of the major ISOLDE mechanisms, e.g. 11Li made from spallation of
Uranium.• Fission (technically not only high energy)
o There is a variety of ways to induce fission (photons, protons, neutrons (thermal, low, high energy)
o The fissioning nuclei can be the target (HRIBF) or the beam (GSI/MSU/RIKEN).
• Coulomb Breakupo At beam velocities of 1 GeV/n the equivalent photon flux as an ion passes
a target is so high the GDR excitation cross section is many barns.
• Fragmentation (NSCL, GSI, RIKEN, GANIL)o Projectile fragmentation of high energy (>50 MeV/A) heavy ionso Target fragmentation of a target with high energy protons or light HIs. In
the heavy ion reaction mechanism community these are called intermediate mass fragments.
• Spallation (ISOLDE, TRIUMF-ISAC)o Name comes from spalling or cracking-off of target pieces.o One of the major ISOLDE mechanisms, e.g. 11Li made from spallation of
Uranium.• Fission (technically not only high energy)
o There is a variety of ways to induce fission (photons, protons, neutrons (thermal, low, high energy)
o The fissioning nuclei can be the target (HRIBF) or the beam (GSI/MSU/RIKEN).
• Coulomb Breakupo At beam velocities of 1 GeV/n the equivalent photon flux as an ion passes
a target is so high the GDR excitation cross section is many barns.
Production Mechanisms – High Energy
RIA Summer School 2006
Fission Cross Sections
Low energy fission can lead to higher yields for certain nuclides.
This is the basis of the electron driver upgrade of the HRIBF.
Low energy fission can lead to higher yields for certain nuclides.
This is the basis of the electron driver upgrade of the HRIBF.
RIA Summer School 2006
HRIBF eBeam Upgrade
• Bremsstrahlung from the electron beam induces photo-fission in a uranium carbide target system with a thickness of ~35 g/cm2
• A 50 kW, 100 MeV electron beam incident on such a target would generate a total uranium fission rate 25 times greater than a 20 μA, 50 MeV proton beam.
• In addition, the yield of neutron-rich species is shifted much farther from stability than for proton induced fission.
• This would result in a factor of 1,000 to 10,000 increase in beam intensities at HRIBF
• Bremsstrahlung from the electron beam induces photo-fission in a uranium carbide target system with a thickness of ~35 g/cm2
• A 50 kW, 100 MeV electron beam incident on such a target would generate a total uranium fission rate 25 times greater than a 20 μA, 50 MeV proton beam.
• In addition, the yield of neutron-rich species is shifted much farther from stability than for proton induced fission.
• This would result in a factor of 1,000 to 10,000 increase in beam intensities at HRIBF
http://www.phy.ornl.gov/hribf/initiatives/electrons/
RIA Summer School 2006
Projectile Fragment
SpallationProduct
Intermediate Mass Fragment/ Target Fragment
Terminology for High Energy Reactions
The fragment could emit nucleons (fragmentation) and/or fission
The fragment could emit nucleons (fragmentation) and/or fission
See the lectures of D BazinSee the lectures of D Bazin
ABRABLA - A. R. Junghans, K.-H. Schmidt et al, Nucl. Phys. A 629 (1998) 635ABRABLA - A. R. Junghans, K.-H. Schmidt et al, Nucl. Phys. A 629 (1998) 635
RIA Summer School 2006
Overview of the In-Flight Technique
Wedge location
D = 5 cm/%
R = 2500 p/p
100 pnA 86Kr
5 kW Beam power
8 msr
p = 5%
Example: The NSCL Coupled Cyclotron FacilityExample: The NSCL Coupled Cyclotron Facility
65% of the 78Ni is transmitted
Morrissey and Sherrill: Euroschool LecturesMorrissey and Sherrill: Euroschool Lectures
RIA Summer School 2006
Multiple stages of separation
Z
N
P re-S eparator M ain-S eparator
S n132S n132S n132
H. Geissel et al. NIM B
Higher energy provides cleaner separation.
Higher energy provides cleaner separation.
RIA Summer School 2006
LISE++ Simulation Code
The code operates under Windows and provides a highly user-friendly interface. It can be downloaded freely from the following internet address: http://www.nscl.msu.edu/lise
O. Tarasov et al.
RIA Summer School 2006
0
1
2
3
4
5
0 5 10 15 20 25
Momentum Acceptance [%]
Yie
ld [
pps/
pA
] 100 MeV/u
200 MeV/u
400 MeV/u
600 MeV/u
1000 MeV/u
0
1
2
3
4
5
0 5 10 15 20 25
Momentum Acceptance [%]
Yie
ld [
pps/
pA
] 100 MeV/u
200 MeV/u
400 MeV/u
600 MeV/u
1000 MeV/u
Facility Specifications
78Ni from 86Kr
No secondary reactions
Tony Nettleton
RIA Summer School 2006
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50
dp/p in %-10 0 10
800
1200
400
0
1600
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50
dp/p in %-10 0 10
800
1200
400
0
1600
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
400
300
200
100
0
500
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
400
300
200
100
0
500
Fragmentation at 400MeV/u
• Angles ≤ ± 20 mrad
• Momentum ± 3 - 8 %
Relatively ‘easy’ due to small phase space
Momentum distrib.
100Sn
200W
M. Hausmann, T. Nettleton
RIA Summer School 2006
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
600500400300200100
0
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
600500400300200100
0
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
0
100
200
300
400
b/m
rad
-40-20
-60
0204060
a/mrad-50 0 50 -10 0 10
dp/p in %
0
100
200
300
400
In-Flight Fission at 400 MeV/u
•Angles ± 40 - 60 mrad
• Rigidity ± 6 - 10 %
• Plus correlations due to fission kinematics
More challenging due to larger phase space
132Sn
76Ni
M. Hausmann, T. Nettleton
RIA Summer School 2006
NSCL Coupled Cyclotron Project
Experimental Areas
Cyclotrons – up to MeV/uCyclotrons – up to MeV/u
ECR
Operational – will study N=82 nuclei and nuclei along the neutron drip line up to mass 30.
Operational – will study N=82 nuclei and nuclei along the neutron drip line up to mass 30.
RIA Summer School 2006
Particle Identification
RIA Summer School 2006
Beams Produced with CCF/A1900
RIA Summer School 2006
GSI Current RNB Facility
• Production of 100Sn and 78Ni
• Hundreds of new masses and isotopes, …
RIA Summer School 2006
Cold Fragmentation Studied at GSI
197Au + Be at 950 A MeV
J. Benlliure, K.-H. Schmidt, et al. Nuclear Physics A 660 (1999) 87
5
RIA Summer School 2006
The GSI FAIR Facility Layout
from J. Nolen ANL
RIA Summer School 2006
RIKEN Radioactive Ion Beam Factory
from J. Nolen ANL
RIA Summer School 2006
RIKEN RIBF Heavy-ion accelerator system
An ion source current of 32 p-μamps is required to reach uranium beam goal. An ion source current of 32 p-μamps is required to reach uranium beam goal.
RIA Summer School 2006
Targets and Production Mechanisms
from J. Nolen ANL
RIA Summer School 2006
I = Ib Tuseable diff des eff is_eff accel_effI = Ib Tuseable diff des eff is_eff accel_eff
H. Ravn
- production cross section
· Ib - beam intensity
· Tuseable - usable target
thickness diff – diffusion efficiency des – desorption efficiency eff – effusion efficiency is_eff - ionization efficiency accel_eff - acceleration
efficiency
- production cross section
· Ib - beam intensity
· Tuseable - usable target
thickness diff – diffusion efficiency des – desorption efficiency eff – effusion efficiency is_eff - ionization efficiency accel_eff - acceleration
efficiency
Production is only one part of the equation
target
RIA Summer School 2006
ISOLDE
http://isolde.web.cern.ch/ISOLDE/
CERN
PSB
1 GeV protons
2 mA
Intensities up to 1011 pps
CERN
PSB
1 GeV protons
2 mA
Intensities up to 1011 pps
Accelerate to 3.0 MeV/u
RIA Summer School 2006
SPIRAL at GANIL
http://www.ganil.fr/spiral/index.html
RIA Summer School 2006
GANIL SPIRAL-2
Completion
~2011
Completion
~2011
RIA Summer School 2006
ISAC Radioactive Beam Facility - ISOL
Beams are produced by 500 MeV protons from TRIUMF cyclotron.Beams are produced by 500 MeV protons from TRIUMF cyclotron.
2x109 22Na/s
ISAC-II underway
ISAC-II underway
RIA Summer School 2006
ISAC-2 overview
ISAC has a fixed 500-MeV proton beam driver with 50-kW power.
ISAC has a fixed 500-MeV proton beam driver with 50-kW power.
RIA Summer School 2006
Texas A&M Upgrade Project
http://cyclotron.tamu.edu/• Radioactive beams to 50 MeV/u• Difficult isotopes from the ion-guide
• Radioactive beams to 50 MeV/u• Difficult isotopes from the ion-guide
RIA Summer School 2006
EURISOL
5 MW Proton LINAC
http://www.ganil.fr/eurisol/index.html
RIA Summer School 2006
Overview of the RIA Concept
RIA Summer School 2006
A combination of forces working together is required to obtain
•Fast extraction times over the full volume
•High efficiency over the full volume
•Tolerance to high intensity
A combination of forces working together is required to obtain
•Fast extraction times over the full volume
•High efficiency over the full volume
•Tolerance to high intensity
Forces in gas catcher system
from J. Nolen ANL
RIA Summer School 2006
Momentum Compensation
Diagram: H. Weick et al., NIM B 164-165 (2000) 168
FWHM = 32 atm-m 4He
FWHM = 0.93 atm-m 4He
Above: Range compression of 350 Mev/u 130Cd produced from 500 MeV/u 136Xe(MOCADI simulation)
130Cd
0
0.5
1
1.5
2
0 500 1000 1500 2000 2500
0
0.5
1
1.5
2
0 500 1000 1500 2000 2500
Ran
ge F
WH
M (
atm
-m)
Resolving Power
350 MeV/u 130Cd range width
M. Amthor
RIA Summer School 2006
beam from A1900
9.4 T Penningtrap system
mass measurements
Many systematic studies:
L. Weissman et al., NIM A522 (2004) 212, NIM A531 (2004)
416, Nucl. Phys. A746 (2004) 655c, NIM A540 (2005) 245.
P/P 0.5 %, gas_cell_1.2_50
0.000
0.005
0.010
0.015
0.020
0.025
0.030
0.035
0.040
0.045
1650 1670 1690 1710 1730 1750 1770 1790
18 k pps
6 k pps
2 k pps
0.4 k pps
0.04 k pps
gas-equivalent
stopping /10
-10 -5 0 5 10
18
19
20
21
22
23
24
TO
F [
s]
fRF
[Hz] - 7595522
38Ca++
T1/2 = 440 ms
R = 2106
m/m < 10-8
First nuclear physics experiment with thermalized beams from fast beam fragmentation
LEBIT project
92 MeV/U 38Ca/37K
Degrader thickness m
effi
ciency
Gas Stopping in use at the NSCL
RIA Summer School 2006
<Normalized background substracted Si counts>
0
0.001
0.002
0.003
0.004
0.005
0.006
0.007
2150 2200 2250 2300 2350 2400 2450 2500 2550
Degrader Thickness [mg/cm2]
<Si /
Sci
41 -
bck
g>
17. Feb 05
0
5
10
15
20
1900 2000 2100 2200 2300 2400 2500
degrader thickness [mg/cm^2]
co
un
ts O
TO
F /
MU
SIC
GSI experiment S258
Savard(ANL), Scheidenberger (GSI) et al.
GSI experiment S258
Savard(ANL), Scheidenberger (GSI) et al.
Bragg peak from 56Ni beamBragg peak from 54Co beamBragg peak from 52Fe beam
54Co52Fe
~ 50 % of radioactive ions stopped in the gas catcher were extracted as
a radioactive ion beam!
ANL, GSI, KUL, MSU, RIKEN, …
RIA prototype gas catcher tested at GSI
RIA Summer School 2006
ANL Upgrade based on 252Cf Fission
Guy Savard, ANL
RIA Summer School 2006
ANL ATLAS upgrade: CARIBU
RIA Summer School 2006
Yields from the ANL Upgrade
Guy Savard, ANL
RIA Summer School 2006
SRIM & PIC calculation by M.Facina
0 100 200 300 400 500
60
80
100
120
140
160
radi
al d
ime
nsi
on
(mm
)
axial dimension (mm)
He+
Stopping volume Stopping volume 75 cm 75 cm33
Ionization Ionization 1.7 x 10 1.7 x 1066 IP/ionIP/ion
Extraction of He+
1.00E-04
1.00E-03
1.00E-02
1.00E-01
1.00E+00
0 100 200 300 400 500 600 700
time (ms)
effi
cien
cy
1e0/s
1e1/s
1e2/s
1e3/s
1e4/s
1e5/s
1e6/s
~0.53%
~2.15 %
~4.55%
~8.80%
~14.5%
~0.054%
HeHe+ + created by a 100 pps created by a 100 pps 3838Ca beam in 760 TorrCa beam in 760 Torr
RIA Summer School 2006
Cyclotron Gas Stopper Concept
RFQ Ion Guide
RF Carpet
Charge Collection Electrodes
Test (Fission) Source
2Tesla Magnet
Pumping
10 mbar He
Entrance window/degrader
extracted beam
injectedbeam
Gas-filled weakly-focusing cyclotron magnet w/ RF guiding techniques at end-of-range
Low gas pressure
long stopping path
fast drift & extraction
Separate He+ from rare ions
minimal space-charge
Exotic atom studies in a cyclotron trap for antiprotons, pions, and muons
L.M. Simons, Hyperfine Interactions 81 (1993) 253
Proposal for a cyclotron ion guide with RF carpet
I. Katayama, M. Wada, Hyperfine Interactions 115 (1998) 165
A Study of Gas-Stopping of Intense Energetic Rare Isotope Beams
G. Bollen, D.J. Morrissey, S. Schwarz, NIM A550 (2005) 27
Features/Expectations:
RIA Summer School 2006
Initial Stopping Calculations
degrader
100 MeV/A Br [ 2.6 mm Al ] 610 MeV Br
Field Bmax = 2 T, n = 0.2
10 mbar He
Beam simulations of ions in gas-filled weak-focusing magnet by Bollen
Beam simulations of ions in gas-filled weak-focusing magnet by Bollen
High space-charge and stopped-ion regions are separated ! Intensity limits > 108/s
High space-charge and stopped-ion regions are separated ! Intensity limits > 108/s
Energy loss or Ionization density
Energy loss or Ionization density
Stopped-ion distribution lies inside dashed circle
Top view
RIA Summer School 2006
NSCL Stopping Cyclotron (Under Design)
Superconducting magnet system Bmax = 2 T, n = 0.2, rinj = 0.7 m
High EnergyBeam
D.Lawton, A.Zeller (NSCL)
RIA Summer School 2006
Beam Simulation including Injection
One Trajectory in ‘real’ field
Energy vs. Position
degrader
100 MeV/A 79Br on 2.6mm Al 610 MeV 78Br
F. Marti (NSCL)
RIA Summer School 2006
Minimizing extraction time
Simulations of ion motion on RF carpets in 2 Tesla field
Low gas pressure (10 mbar compared to 200 - 1000 mbar in present systems) Time for collection onto carpet and transport out of gas stopper < 5 ms !
Low gas pressure (10 mbar compared to 200 - 1000 mbar in present systems) Time for collection onto carpet and transport out of gas stopper < 5 ms !
RF 400V; 1.5MHzDC gradient 20V/cmSpacing 1 mm, 0.5 mm thick
RFQ Ion Guide
RF Carpet
Charge Collection Electrodes
Test (Fission) Source
2Tesla Magnet
Pumping
10 mbar He
Entrance window/degrader
extracted beam
injectedbeam
RIA Summer School 2006
NSCL Reacceleration Stage Options
Reaccelerated beam area
Reaccelerated beam area
Stage I: 3 MeV/uStage I: 3 MeV/u
Stage II: 12 MeV/uStage II: 12 MeV/u
RIA Summer School 2006
You ask: Should I switch fields?
• Construction of a 1 B$ facility in the US in the next 5 years is unlikely
• There are positive signs (3rd on the DOE list of facility priorities; congressional mandate of RIA; highest NSAC priority) that something on the scale of 600 M$ will happen
• This is a very active field world-wide
• NSCL, TRIUMF, HRIBF, ANL, T A&M, etc.
• Upgrades at NSCL, ANL, HRIBF
• Large scale international facilities: FAIR, RIBF, SPRIRAL II, EURISOL, …
• There are exciting, important questions to answer
• Construction of a 1 B$ facility in the US in the next 5 years is unlikely
• There are positive signs (3rd on the DOE list of facility priorities; congressional mandate of RIA; highest NSAC priority) that something on the scale of 600 M$ will happen
• This is a very active field world-wide
• NSCL, TRIUMF, HRIBF, ANL, T A&M, etc.
• Upgrades at NSCL, ANL, HRIBF
• Large scale international facilities: FAIR, RIBF, SPRIRAL II, EURISOL, …
• There are exciting, important questions to answer
RIA Summer School 2006
Additional Material
RIA Summer School 2006
RIA White Papers
One of the best places to find out more information regarding RIA is the RIA users web site.
Overall info:
http://www.orau.org/ria/
White papers:
http://www.orau.org/ria/pubs.htm
One of the best places to find out more information regarding RIA is the RIA users web site.
Overall info:
http://www.orau.org/ria/
White papers:
http://www.orau.org/ria/pubs.htm
RIA Summer School 2006
Universality of Production Cross Sections
Na isotopesNa isotopes
RIA Summer School 2006
The production yield of residues saturates with a total beam energy of a few GeV. Limiting Fragmentaton
H. Ravn - “The saturation cross-section for more exotic species may well first be reached beyond 5 GeV.”
Kaufman and Steinberg, PRC 22 (80) 167.
Limiting Fragmentation
RIA Summer School 2006
Moretto and Wozniak, Ann. Rev. 45 (93)
Moretto and Wozniak, Ann. Rev. 45 (93)
p + Xeat 48.5 degrees
Limiting Fragmentation continues to high energy