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UNIVERSITY OF CALIFORNIA
NSD NUCLEAR SCIENCE DIVISION
Experimental capabilities for applied nuclear science at
the 88-Inch CyclotronLarry Phair
Questions1. What are the capabilities at your lab?
particle microamp most anything on the periodic table Facilities: BGS, gamma decay counting, BASE
2. Are there specific limitations in the types of experiments that can be run at your lab?
E/A=5-10 MeV for heavyE/A = 14 MeV for mediumE/A = 32 MeV for lighter heavy-ion beams
protons: up to 55 MeVdeuterons: up to 65 MeVHe3: up to 170 MeValphas: up to 130 MeVneutron beams: 8-30 MeV
3. What is required to run an experiment at your lab?
Local Cyclotron Advisory Committee (CAC) $1400/hrRad worker 1 training online, Bldg OJT (20 min. onsite)
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3
88-Inch Cyclotron Dual Mission
Conduct world-class science: Berkeley Gas-filled Separator (BGS), super-heavy element program
Support national security and other US space programs in the area of radiation effects testing: Berkeley Accelerator Space Effects (BASE) Facility
BGS
BASE Facility Cave 1: BGS
Users: ~ 350 Light Ions: Protons up to 55 MeV 3He up to 170 MeV Heavy Ions: 5 To 32 AMeV
Caves 4A & B
4
Ion Sources
Cyclotron
BASE Test Shack
Experimental Caves
BASE Facility and mission
BASE = Berkeley Accelerator Space Effects
Mission: Support national security and other US space programs in the area of radiation effects testing.
protons: 1-55 MeV
Standard Cocktail Beams: 4.5, 10, and 16 AMeV
BASE Cocktails
What is a “Cocktail”?• Multiple ions injected in to the
Cyclotron, which we can then select and separate by simply changing the frequency of the cyclotron.
Why do BASE users want “Cocktails”?
• Typically, to obtain data correlating event cross sections to linear energy transfer (LET).
5
Large ion selection combined with 3-minute ion changes saves users a significant amount of time.
88-inch accelerator
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6.4 GHz ECR VENUS: 18+28 GHz
AECR: 10+14 GHz
High Intensity Light Ions Protons to 55 MeV3He to 170 MeV
Heavy Ions 5 To 32 MeV/nucleon0.2 ≤ Q/M ≤ 0.5
Mass Resolution 1/3000
Medium to very high charge states of every element from H to U
E
M=
✓Q
M
◆2
⇥K
World-leading ECR ion source group
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Ion Chg state
Intensity (eµA)
4He 2+ 11,00016Ο 6+ 3,00040Αr 11+ 860209Bi 31+ 300209Bi 50+ 5.3238U 33+ 440238U 50+ 1340Ca 11+ 400
VENUS records
Why these records are important...
BASE community can use the tails for higher LET in the cocktail • Xe in the 16 AMeV cocktail• Bi or Au in the 10 AMeV
cocktail8
1
10
100
1000
104
4 6 8 10 12 14 16 18Ext
ract
ed b
eam
from
the
Cyc
lotro
n [e
nA]
MeV/nuc
Xe28+
Xe42+
Xe43+Xe34+
Xe28+
VENUS
AECR
Beams not available with the AECR
Xe44+
Xe42+
Xe34+
Collaboration with MSU238U33+ : 430 μA
FRIB needs very high intensity high-charge-state beams.
Low emittance beams for high intensity transmission (super heavy studies)
Engineering NSD AFRD
Future heavy ion accelerators begin here: Next generation ECRIS for intense heavy ion beams
Current state of the art: VENUS
VENUS MARS
B on axis (T) 4 3.6
B radial (T) 2.2 3.3
Frequency (GHz) 28 18-28
A path forward: MARS (Mixed Axial and Radial field System)
Prototype ion source for FRIB
Recent milestone: 238U33+ : 430 eμA
MARS will bridge to next generation ECRIS technologies with a novel closed-loop super-conducting coil. This scheme for generating higher magnetic fields will be tested in MARS and will ultimately allow for new ion source designs with improved performance far beyond that of VENUS.
MARS: proof of principle of the new magnetic structure for next generation ECRIS
Superconducting Electron Cyclotron Resonance ion sources (ECRIS) are being developed at LBNL that provide improved performance and significant cost savings for accelerator facilities in the US and around the world. Significant gains can be made for radioactive beam facilities, high density physics research, and super-heavy element studies with more intense, higher charge state beams.
Goal: emA of high charge state Bi & U beams
MARS windings: a test
Field maps
Test potting techniques
Wind with NbTi to build a MARS demonstrator, up to 45 GHz
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Beam time distribution in FY12
46 experiments for BASE (~300 customer visits)9 experiments for NSD:48Ca for GRETINA@BGS
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5425 hours of 10/4 operation Availability: 94%
BASERechargeBeam developmentNuclear Science
FY12 beam usage
6%8%
4%
11%
2%4%
26%
22%
2%
15%
Ar ArHI ArHiH Ca Cr other HMg NeHIH Ti
Ar
10 AMeV
Ca
protons
Ti
Mg
Cr
16 AMeV
Aerospace Corp.Aeroflex
Micro-RDCHoneywell Microsemi
MIT – LincolnSilicon Space
TechnologyXilinx
Situs LogicUltracommMoog, Inc.
International Rectifier
LBNLLLNL
Sandia National Lab
National Semiconductor
BAECypress
SemiconductorIntersil
Texas InstrumentsSpace Micro
ZephyrITT Exelis
BroadcomLinear Technology
Georgia TechASIC Advantage
Rochester Inst. of Tech.
NASA JohnsonNASA Goddard
NASA AmesNASA Jet
Propulsion LabUnited Launch
AllianceNorthrup Grumman
Vanderbilt U.Boeing
Ball AerospaceNRL
Users
Neutron beamStopped d beams in the vault. Break-up neutrons at zero degrees in to Cave 0.
• Intensities: 106 n/cm2/sec
• Energies: 8-30 MeV
• Beam sweeper
Use light-ion reactions, 7Li(p,n)7Be and d(d,n)3He, to produce nearly monoenergetic neutrons
Darren Bleuel’s talk Friday12
Lunar Reconnaissance Orbiter
Characterize new neutron scintillator materials for basic and applied research (LLNL)
Cyclotron capabilities (now)
10’s of microamps of light ions (H, D, He3, alphas)
• protons: 3-55 MeV
• deuterons: 2-65 MeV
• He3: up to 170 MeV
• alphas: up to 130 MeV
• neutrons: 8-30 MeV
Particle microamps of heavy ions (up to 32 MeV/nucleon)
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Cyclotron capabilities (future & past)
Cyclotron started as an internal target machine:
• Few mA of beam
If we need to extract intense light ion beams: negative ions and stripping
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Cave Door
Cave Door
OOS Cave DoorVault Door
Cave Door
Vau
lt D
oor
Deflector Power
Supplies
Cave Door
Cave Door
Cave Door
Vault
Cave 5
Cave 4
Cave 2
Cave 4B
Cave 4A
Cave 3
Cave Door
Cave Door
Cave
5
Bea
m P
lugs
BL1
GV
1M
C 1
1
G-1
Cave
4A
B
eam
Pl
ug
Cave
4B
B
eam
Pl
ug
So
lid
Sta
te D
ete
cto
r
CyclotronR
F Ta
nk
Dee
PH 1
1
General Research Facility
G - 2
Coff
inLaser Trap
Deflector Niche
20o
Swit
chin
g M
agn
et40o59o
-35o
10o
-110o
110o
-7.5o
14.5o
42o
Cave 4C
Heavy Ion Facility
Light Ion Facility
RF
Tank
FPABerkeley Accelerator
Space Effects (BASE)Facility
Berkeley Accelerator
Space Effects (BASE)Facility
-20o
Fast
FC
- V
D
0o
TMV
6
Stee
lSt
eel
Cave 1
BL1
GV
2
PH 1
2
FC 1
1
BGS 88-Inch Cyclotron88-Inch Cyclotron Cave
01/02
Q01 A & B
G-0
Wobbler
MC 01
Cave 01/02Beam Plug
49o
VA 0
PH 01
FC 01Coll. 01
FC/Neutron Tgt
Sand
Bag
s
HLC
CUSP
D
etec
tor
Cyclotron: internal targets
15
Questions1. What are the capabilities at your lab?
particle microamp most anything on the periodic table Facilities: BGS, gamma decay counting, BASE
2. Are there specific limitations in the types of experiments that can be run at your lab?
E/A=5-10 MeV for heavyE/A = 14 MeV for mediumE/A = 32 MeV for lighter heavy-ion beams
protons: up to 55 MeVdeuterons: up to 65 MeVHe3: up to 170 MeValphas: up to 130 MeVneutron beams: 8-30 MeV
3. What is required to run an experiment at your lab?
Local Cyclotron Advisory Committee (CAC) $1400/hrRad worker 1 training online, Bldg OJT (20 min. onsite)
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