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Measurement of 4 He( 12 C, 16 O) reaction in Inverse Kinematics Kunihiro FUJITA K. Sagara, T....
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Transcript of Measurement of 4 He( 12 C, 16 O) reaction in Inverse Kinematics Kunihiro FUJITA K. Sagara, T....
![Page 1: Measurement of 4 He( 12 C, 16 O) reaction in Inverse Kinematics Kunihiro FUJITA K. Sagara, T. Teranishi, M. Iwasaki, D. Kodama, S. Liu, S. Matsuda, T.](https://reader036.fdocument.pub/reader036/viewer/2022062314/56649e3f5503460f94b2f8a1/html5/thumbnails/1.jpg)
Measurement of 4He(12C,16O)g reaction in Inverse Kinematics
Kunihiro FUJITAK. Sagara, T. Teranishi, M. Iwasaki, D. Kodama, S. Liu, S.
Matsuda, T. Mitsuzumi, J.Y. Moon, M.T. Rosary and H. Yamaguchi
Department of Physics, Kyushu University, Japan
Kyushu University Tandem Laboratory (KUTL)
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Evolution of Stars
12C/16O abundance is determined
→ affects all of the posterior processes
H-burning
4p → 4Hevia
p-p chain &CNO cycle
He-burning
3 4He → 12C4He+12C → 16O+g
C-burning
O-burning Si-burning
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Introduction• 12C/ 16O ratio after helium burning process
– evolution of heavy stars – supernova or white dwarf?– abundance of element of universe
• Cross Section of 4He(12C,16O) g– very small (~10-8 nb) – coulomb barrier – varies drastically around stellar energy(0.3MeV)
• Extrapolation with experimental data
Ecm (MeV) s (nbarn)2.4 601.5 1
1.15 0.11.0 3x10-2
0.85 10-2
0.7 10-3
0.3 10-8
our experiment( 10% accuracy)
extrapolation
stellar energy
E1
E2
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16O measurement① 4He beam + g measurement
② 16N decay measurement
③ direct 16O measurement with 12C beam and 4He target– high efficiency (~ 40%: charge fraction)– total S-factor can be obtained
• necessary components for Ecm=0.7MeV experiment– background separation system: NBG/N12C ratio of 10-19
– thick gas target : ~25 Torr x 3 cm– high intensity beam: ~ 10 pmA
• Y(16O) ~ 5 counts/day
→ 1 month experiment for 10% error
Cross section (S=const.)
10-5
10-5
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Experimental Setup• Layout of Kyushu University Tandem Laboratory (KUTL)
Detector (Si-SSD)
Sputterion source
12C beam
Tandem Accelerator
Final focal plane(mass separation)
Blow in windowless4He gas target
Long-time chopper
chopperbuncher
16O
12C
Recoil Mass Separator(RMS)
Ecm = 2.4~0.7 MeVE(12C)=9.6~2.8 MeVE(16O)=7.2~2.1 MeV
Tandem
RMS
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Windowless Gas Target
RMS
TMP3
TMP4MBP2TMP2TMP5
MBP1
beam
TMP1
DP
1500 l/s
3000 l/s330 l/s
330 l/s520 l/s 520 l/s
520 l/s
350 l/s
Differential pumping system (side view)
• center pressure: 24 Torr - post stripper is not necessary• effective length: 3.98 0.12 cm (measured by p+a elastic scattering)
→ target thickness is sufficient for our experiment (limited by energy loss of 12C beam)
24Torr
SSD: beam monitor4.5cm
• Blow-In Gas Target (BIGT)– windowless & high confinement capability
beam
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BG Reduction and 16O Detection Recoil Mass Separator
– 12C/16O separation : ratio of 10-11
– angular acceptance: 1.9deg
100% 16O can be observed
• Background 12C– charge exchange– multiple scattering
• Background reduction① RF deflector (Long-Time Chopper)
– background reduction ~10-3
② movable slits– combination with trajectory analysis
v dispersionm dispersion
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Ecm=1.5 MeV experiment
• beam: 12C1+, frequency: 3.620MHz– energy: 6.0MeV, intensity: 60pnA
• target: 4He gas 15.0 Torr x 3.98 cm• observable: 16O3+, 4.5 ± 0.3 MeV– abundance = 40.9 ± 2.1 % = efficiency
95 hours data
16O
208 counts
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Charge State Distribution of 16O
• Charge state after gas target– 16O has different charge state
• Our target is very thick
• Equilibrium charge distribution was measured• Comparison with theoretical calculation
2 4 6 8 10 12 140
10
20
30
40
50
60
70
14MeV
12MeV9.4MeV7.2MeVF
ract
ion
(%)
Energy(MeV)
4.5MeV
Line: the empirical formuladot: our data and triumf data
7+
6+5+
4+3+2+
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Cross Section and S-factor
• 2.4MeV: • 1.5MeV:
• Background ratio NBG/N12C = 10-16
• Next experiment is Ecm=1.20 MeV
future plan D. Schurmann et al.Eur. Phys. J. A 26, 301-305 (2005)
Our data (2009, 2010)
, 2010
stellar energy
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Development of Ionization Chamber• BG reduction by 10-3 is necessary for
Ecm=0.7MeV measurement
Particle Identification by E-DE information → Ionization Chamber
• Gas: PR-Gas, 10~30 Torr• Effective area: 40Hx40Wx50tmm2
• Entrance Window: PET foil, 0.5mm, f45mm
• Voltage:– Cathode: GND, Grid: 100V, Anode: 150V
• Timing resolution of1ns is necessary
→ install Si-SSD at the end
f45mm
cathode
frish grid
anode
SSD
PETfoil
50mm
40mm
50mm
particle
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Performance test by 12C+a
• Test experiment by Ecm=1.5MeV setting
– 6.0MeV, 12C beam: ~100nA– Pilot 16O - spontaneity generating from tandem acc.
– 16O(4.5MeV) and12C(3~6MeV) was separated by the ratio of 10-3(99.9%)– Energy resolution of Ionization Chamber was DE/E=9%(FWHM)
projection
12C
16O
Total E [MeV]
DE [
MeV
]
DE [MeV]
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Test Experiment of Ecm=1.2MeV
• Update of Tandem acc. ~Accelerate Decelerate mode– successfully incremented for beam intensity
• Beam: 4.8MeV(1.2MV), 12C2+
• Observable: 3.6MeV, 16O3+ 5 hours data
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Summary
• Direct 16O measurement via 4He(12C,16O)g reaction was proposed to determine 12C/16O abundance ratio in stars
• Blow-in type windowless gas target was developed, and thickness of 24 Torr x 3.98 cm was achieved
• Background reduction was performed by using RMS, RF-deflector and movable slits
• Ecm= 2.4 MeV experiment
– s= 64.6 nb, S-factor = 89.0keV b• Ecm= 1.5 MeV experiment
– s= 0.900 nb, S-factor = 26.6 keV b• Now we start measurement at Ecm=1.2MeV
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15
BACKUP
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16
Charge State Fraction of 16O
0
10
20
30
40
50
60
70
2 4 6 8 10 12 14
Frac
tion
[%]
Energy [MeV]
5+4+3+ 6+2+
7+
Our dataW. Liu et al. / Nucl. Instr. and Meth. A 496 (2003) 198–214
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pass only reaction products (16O) which are spread in time.
f2=3×f1
V2=V1/9
f1=6.1MHzV1=±24.7kV
V3=23.7kV
reject BG
pass reaction products
+
Flat-bottom voltage
RF-Deflector (Long Time Chopper)
BG(12C)16O5+
500events
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Trajectory Analysis• 12C backgrounds were rejected by slit
control based on trajectory analysis
16O3+ 4.5MeV (Ecm=1.5MeV)
12C3+ 6.0MeV
12C2+ 3.0MeVslits
target
ED D1 D2final focal plane(detector)
v dispersion
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19
Ecm=2.4MeV experiment
• beam: 12C2+, frequency: 6.063MHz– energy: 9.6MeV , intensity: ~35pnA
• target: 4He gas ~ 23.9 Torr x 3.98 cm• observable: 16O5+ 7.2 ± 0.3 MeV
– abundance = 36.9 ± 2.1 % = efficiency
29hours data
941 counts
16O
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Development of Ionization Chamber• BG reduction by 10-3 is necessary for Ecm=0.7MeV measurement
• Additional electric deflector? Or Wien-Filter?
→ difficult due to space boundary• Upgrade detector
DE information by Ionization Chamber
Simulation plot of E-DE
Ar Gas: 20Torrx5cm
16O (4.5MeV)
12C (1~6MeV)
Total E [MeV]
DE [
MeV
]
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Resolution of Ionization Chamber
16O beam
Ionization Chamber
θ12 C,1
6 O
7μg/cm2 C-foil• Detector setting
– PR-gas: 20 Torr– Cathode: -150V, Grid: -50V
• Measurement of 16O+12C elastic scattering– Beam: 16O2+, 9.6MeV– Target: 12C(7 mg/cm2)
12C: 5.91MeV
16O: 4.75MeV
– Clearly separated for 16O(4.75MeV) and 12C(4.7MeV)
– Energy Resolution: DE/E=6%(FWHM)
Total E [ch]
DE [
ch]
45.0°37.5°
12C: 4.70MeV
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Normal operation of tandem accelerator.
Accel-decel operation of tandem accelerator.
At low acceleration voltage, focusing becomes weak, and beam transmission decreases.
By alternative focus-defocus, Focusing becomes strong, and Beam transmission increases.
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By the accel-decel operation, ・ 10 times higher beam transmission is obtained by strong focusing. ・ 17.5 times more intense beam can be injected, due to higher electric power
necessary for accel-decel operation.By a large aperture (12f) gas stripper, spread in beam energy and angle is
decreased, and beam transport to the target is ~3 times increased.
Totally, beam intensity is 300-500 times increased.
normal operation
accel-deceloperation
Al shorting bars for accel-decel operation