APS-DNP Fall20041 Design Studies for RIA Fragment Separators A.M. Amthor National Superconducting...
-
date post
21-Dec-2015 -
Category
Documents
-
view
216 -
download
3
Transcript of APS-DNP Fall20041 Design Studies for RIA Fragment Separators A.M. Amthor National Superconducting...
APS-DNP Fall2004
1
Design Studies for RIA Fragment Separators
A.M. Amthor
National Superconducting Cyclotron Laboratory, Michigan State UniversityDepartment of Physics and Astronomy, Michigan State University
APS-DNP Fall2004
2AMA
RIA Concept
High-Resolution Separator
Large-Acceptance Separator
APS-DNP Fall2004
3AMA
Motivation: ISOL and Gas Stopping
Optimum productionmethod for low-energy beams
Standard ISOL technique
Two-step fission
In-flight fission + gas cell
Fragmentation + gas cell
ISOL Committee Task Force Report (1999)
APS-DNP Fall2004
4AMA
Motivation: Beam Energy and Momentum Acceptance
Above: Fragment beam of 78Ni produced from 86Kr. At the RIA energy of 400MeV/u the acceptance should be greater than 10%.
Left: Production of various fragments for fixed current and acceptance. Acceptance determines energy of turnover point (here 10% dp/p)
J. Nolen ANL
0 100 200 300 400 500 600 700 800 900 100011001200
E/A ( MeV/u )
1
10
100
FragmentationISOLIn-flight fission
211Fr
132Sn,96Kr
110Zr
80Zr
11Li
138Sn
78Ni
114Zr
159Nd
Δp/p = 10%
Re
lativ
e M
ass
Se
pa
rate
d Y
ield
s
0
1
2
3
4
5
6
7
8
9
0 5 10 15 20
600 MeV/u
400 MeV/u
200 MeV/u
100 MeV/uYiel
d (p
ps/p
μA)
Momentum Acceptance (%)
APS-DNP Fall2004
5AMA
Fragment Separators
N
Z
N
Z
N
Z
Fragments after target
Fragments at wedge
Fragments after FP
SpecificationsBρmax = 6Tm
Δp/p = 5%Δθ = ±40mrΔφ = ±50mrCompensated to 3rd orderLargest acceptance of current facilities
Note: Isotope yield diagrams are from 86Kr78Ni simulation with primary beam of 140MeV/u
APS-DNP Fall2004
6AMA
Thick Wedges andTwo-stage Fragment Separation
CAARI 2004 talk by A. Stolz
Al 450 mg/cm2
Al 300 mg/cm2
Al 190 mg/cm2
APS-DNP Fall2004
7AMA
RIA Separators
Preseparator
• Maximized production rate
• 100 mr in horizontal and vertical
• 12% momentum acceptance
• low optical aberrations (< 2 mm)
High-Resolution Separator
• Maximized quality and purity
• Two-stage fragment separation
• 80 mr in horizontal and vertical angular acceptance
• 6% momentum acceptance
• d/M = 2.5m
The RIA concept makes use of two fragment separators.
PreseparatorMomentum Compensator
Gas-Stopping Cell
Beam
PreseparatorHigh-Resolution Separator
High-Energy Area
Beam(up to 400 kW)
Target
APS-DNP Fall2004
8AMA
PreseparatorThe compensated third order system passes approximately 73% of fragments uniformly distributed in a 6-D phase space ellipse with a and b from ±50mr and with δ distributed over a full width of 12%.
Target
NSCL
Beam
WedgeIsotope
Slits
Beam
Dump
Additional wedge at beam Additional wedge at beam dump?dump?
Additional stage of separation Additional stage of separation for gas cell separator?for gas cell separator?
• Significant higher order aberrations (>3rd order)
• Up to 200kW power on beam dump
• Primary beam often within momentum acceptance and sometimes with |δBρ|< 1%
• Higher energy and greater neutron excess of fragment beams increases magnetic rigidity (10Tm)
• Range compressed fragments to be stopped in 0.5 atm-m gas cell, requires aberrations < 2mm
APS-DNP Fall2004
9AMA
Momentum Compensator
Specifications:
• Full angular and momentum acceptance from preseparator
• Momentum resolving power R>1000
• d/M = 2.5m
Diagram: H. Weick et al., NIM B 164-165 (2000) 168
FWHM = 32 atm-m 4He
FWHM = 0.93 atm-m 4He
Ion
Gui
de,
Coo
ler a
ndB
unch
er
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
Rang
e FW
HM (a
tm-m
)
Resolving Power
350 MeV/u 130Cd range width
Gas
Cel
l &
Noz
zle
Mon
oene
rget
ic
Deg
rade
r
Dis
pers
ive
Ele
men
ts
APS-DNP Fall2004
10AMA
Simulation Methods& Needed Improvements
(x|θδ) aberration – angled wedges
Dispersive focal plane
A. Stolz, CAARI 2004
Fragment production in thick wedges
Profile wedge degrader
APS-DNP Fall2004
11AMA
Acknowledgements
Additional thanks to:
RIA R&D is funded in part by the U.S. Department of Energy (Grant No. DE-FG03-03ER41265) and Michigan State University.
The NSCL is funded in part by the National Science Foundation (Grant No. PHY-01-10253) and Michigan State University.
Collaborators:
B.M. Sherrill 1,2
D.J. Morrissey 1,3
A. Nettleton 1,2
A. Stolz 1
O. Tarasov 1
1National Superconducting Cyclotron Laboratory, Michigan State University2Department of Physics and Astronomy, Michigan State University 3Department of Chemistry, Michigan State University
Ion Optical Program GICOa combination of GIOS and COSY 5.0 written at University of Giessen, 1986 - 1998 by Martin Berz, Bernd Hartmann, Klaus Lindemann, Achim Magel, Helmut Weick
The MOCADI program was developed in PL/I by T. Schwab, H. Geissel, and A. Magel at Giessen University in Germany.
N. Iwasa translated MOCADI 1.34 into C on a DEC VMS operating system and developed it further.