Nuclear moment studies with spin polarized radioactive beams from - - PowerPoint PPT Presentation
Nuclear moment studies with spin polarized radioactive beams from - - PowerPoint PPT Presentation
Nuclear moment studies with spin polarized radioactive beams from fragmentation reaction Daisuke Kameda Department of Physics, Tokyo Institute of Technology Plan of the talk 1. Introduction of the nuclear-moment measurement g factor
Nuclear-moments measurement around light mass region by using the spin-polarized Radio Isotope (RI) beam
- H. Ogawa et al.,
Phys.Rev. C 67 (2003) 064308
µ l, j of the valence orbital Q effective charge, deformation
The principle of β-NMR experiment
Aβ : Asymmetry factor of β-ray emission P : Polarization
The principle of production for spin polarized RI beam from fragmentation reaction
p||
Emission angle Momentum distribution of projectile fragments The projectile fragment should be selected 1, in the momentum distribution 2, in the emission angle
= P0
Production of spin polarized RI beam
RIKEN Projectile-fragment Separator (RIPS)
RRC
Detector setup to detect the spin polarization of RI
22Ne, 110 MeV/u
Confirmation of the spin polarization
Beam pulsing & β -ray counting
Spin- rotation
Adiabatic Field Rotation Method
17C,T1/2 = 193(13)ms 19N,T1/2=0.27(6) s
Primary Beam Ne, 110 MeV/u Ne, 110 MeV/u Target Nb, 778 mg/cm2
natC, 546 mg/cm2
Bz 370 Gauss 420 Gauss Aβ P (net)
- 1.2 ±0.4 %
0.28 ±0.09 % Emission angle 2.3°~ 5.3° 2.6°~ 6.0° Momentum Accep. 7.21~7.66 GeV/c 8.18~8.69 GeV/c Stopper Pt ( at 75 K ) Pt ( at 15 K ) Spin-pol. RI beam Momentum Acceptance
17C : 1.00 P0 ± 3 % 19N : 1.03 P0 ± 3 %
The β-NMR experiment for 17C
Effective Field Nuclear spin ω0 − ∆ω ω0 + ∆ω
ω0 Adiabatic Fast Passage method ω0 = γ Β0 ( γ = µN g / h )
RF coil
40 ms
Time
The β-NMR spectrum of 17C
|g (17Cg.s.) |= 0.5054(24)
Spin parity assignment of 17C I π (17C) = 3/2+
This experimental result
E.K. Warburton and D.J. Millener,
- Phys. Rev. C39 (1989) 1120
MK MK3 J.P. Dufour, et al., Z. Phys. A 324 (1986) 487
I π =(1/2+, 3/2+, 5/2+)
PSDWBT 35% | π(p1/2)-2 ν(d5/2)2(2s1/2)1 > + 31% | π(p1/2)-2 ν(d5/2)3 > + …… PSDMK Similar result to PSDWBT
3/2[211] 5/2[202] 1/2[220] 1/2[211]
10
ε 2 : Quad. Deformation
parameter
ε 2 ~ 0.95 β 2
17C 19O 21Ne 23Mg
ε2 ∼ 0.4 ε2 ∼ 0.4
Spin parity of isotone N=11
Although I π(15C, 19C)=1/2+ ,
Nilsson diagram in prolate deformation region
16C : deformed nucleus
β 2 = 0.93(21)
Recently reported by N. Imai in RIKEN
- Phys. Rev. Lett. In print
(2004) Deformation ?
Further research of 17C will be needed.
Ref. NPA193(1972)372 for 21Ne NPA140(1970)333 for 23Mg
Deformation parameter (ε2 ) Magnetic moment (n.m.) B A C D
A : Bare g factor , κ = 0.08 B : Bare g factor, κ = 0.10 C : Effective g factor, κ=0.08 D : Effective g factor, κ=0.10 Effective g factor for 1d orbit gs = -3.339, gl = -0.0749
The β-NMR experiment for 19N
Experimental Condition
- Graphite stopper at room
temperature
– This material was used in g-factor measurement for 17N.
- Pulsing time : 50ms for beam
700ms for β counting
- Beam Intensity : 5 kpps
- β-ray yield : 500 cps
- RF magnetic field : 10.0 [Gauss]
Beam
0 100 200 300 400 500 600 700
Time for β-ray count (ms) Counts / 2ms (log scale) T1/2 = 298 ± 13 ms
g = 0.58~0.64 (3.3 σ )
Magnetic moments of odd-mass Nitrogen Isotopes
Conditions for 19N in the calc.
- Model Space : p, sd shell
core : 4He p-shell : 10~11 nucleons sd-shell : 4~5 nucleons
- Bare gp, gn factor
Future perspective
x 10 2 x 10 3 x 10 4 x 10 5 pps
95 MeV/nucleon 60 pnA
Beam Intensity for spin-polarized RI Beam Program code : intensity_34 Target : Nb Island of Inversion
Summary
- Confirmed Polarization for 17C and 19N produced from fragmentation reaction
by using the new spin-flip method (Adiabatic Field Rotation) as
17C : - 1.2 ±0.4 % in Pt stopper at 75 K 19N : 0.28 ±0.09 % in Pt stopper at 15 K
- The g factor for 17C and 19Ng.s. by using the b-NMR method as
17Cg.s. : |g | = 0.5054 ±0.0024 19Ng.s. : |g | = 0.58 ~ 0.64 (preliminary)
- The assignment of spin parity for 17C : I π (17C) = 3/2+
Indication of the large deformation of 17C
- Anomalous change of the g factor for 19N compared with the shell
model predictions
Acknowledgements
- K. Asahi, H. Ogawa, H. Miyoshi, K. Shimada, G. Kato, S. Emori,
- G. Kijima, T. Suga, K. Ohno, K. Yogo, K. Sakai
Department of Physics, Tokyo Institute of Technology
- H. Ueno, A. Yoshimi, H. Watanabe, T. Haseyama, Y. Kobayashi,
- W. Sato, K. Yoneda, J. Murata, A. Yoshida, T. Kubo,
and M. Ishihara The Institute of Physical / Chemical Research, RIKEN
- N. Imai
Department of Physics, The University of Tokyo
The time spectrum of β-ray count
Fitting function : N exp( -t/τ ) + Const. Result : χ2 = 1.002 T1/2 = 298 ± 13 ms S/N = 4.5
The β-rays form daughter nuclei,
19 O(T1/2=26.91s), were treated as
constant-background noise.
The observed half life is consistent with the value reported by P.L.Reeder in 1991. Half life of 19N
Time (ms) This exp.
1. J.P. Dufour, et al,. Z. Phys. A324 (1986) 487 2.
- M. Samuel, et al., PRC37 (1988) 1314
3. J.P. Dufour, et al., AIP Conf. Proc. (1988) 344 4. P.L. Reeder, et al., PRC44 (1991) 1435 5. Table of isotope 8th edition
1. 2. 3. 4. 5.
0 100 200 300 400 500 600 700
Time for β-ray count (ms) Counts / 2ms (log scale)
Shell model calculations
- Model Space : p, sd shell
p-shell : 11 nucleons sd-shell : 4 nucleons
- Interaction : PSDMK, PSDWBT
- gp, gn factor : bare