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D-STATE PARAMETER DETERMINATIONS FOR 3He AND 4He

E. Ludwig, C. Bhat, T. Clegg, E. Crosson, H. Karwowski, G. Graw, P.

Schiemenz, R. Hertenberger, H. Kader, D. Hofer, et al.

To cite this version:

E. Ludwig, C. Bhat, T. Clegg, E. Crosson, H. Karwowski, et al.. D-STATE PARAMETER DETER- MINATIONS FOR 3He AND 4He. Journal de Physique Colloques, 1990, 51 (C6), pp.C6-439-C6-442.

�10.1051/jphyscol:1990647�. �jpa-00230917�

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D - S T A T E P A R A M E T E R D E T E R M I N A T I O N S F O R 3 ~ e A N D 4 ~ e

E.J. LUDWIG, C.M. BHAT'~', T.B. CLEGG, E.R. CROSSON, H.J. KARWOWSKI, G. GRAW* , P. SCHIEMENZ* , R. HERTENBERGER*, H. KADER*, D. HOFER* ,, M. BISENBERGER* , A.M. EIRO*" and F.D. SANTOS* *

U n i v e r s i t y o f North Carolina a t Chapel H i l l and T U N L ' ~ ) , Durham, NC 77706, U.S.A

Sektion Physik der UniversitEit Miinchen, 0-8046 Garching. P . R . G .

* Centro de F i s i c a Nuclear da Universidade de Lisboa, P-1699 Lisboa, Portugal

Nous avons r6alis6 des determinations du rapport asymptotique D/S dans 3 ~ e par reaction ( d , 3 ~ e ) et dans '~e par reaction (d.a)

.

Nous avons essay6 d'extraire l'information sur 1'6tat D par des calculs DWBA en port6e finie (traitement exact) avec peu de parametres libres, et nous avons examine la sensibilite des calculs aux parami?tres du mod&le optique, a la fonction de recouvrement et au choix de la transition. Nous discutons des cas 3 2 ~ ( d , 3 ~ e ) 3 1 ~ a E,=16 MeV et 5 8 ~ i ( d , ~ c ) ~ ~ ~ o ti E,=22 MeV.

Abstract

-

Determinations of the asymptotic D/S-state ratio for 3He (q(3He) using the (d, 3He) reaction and ~ ~ ( 4 ~ e ) using the (d,a) reaction are being conducted. An attempt is made to extract D- state information using exact finite-range DWBA calculations with few free parameters. The sensitivity of calculations to factors such as optical model parameters, overlap function and choice of transition is examined. Cases discussed are the 32s polarized (d,%e)31~ reaction at Ed = 16 MeV and 58Ni polarized (d,a)56Co at Ed = 22 MeV.

1 - INTRODUCTION

Our work concentrates on the extraction of parameters, (e.g., q and D2) /I/ dependent on the D state of 3He and 4He using polarized (d,3He) and polarized (d,a) transfer reactions. Finite-range DWBA calculations have shown that the tensor analyzing powers Ax,@) and Ayy(8) are serisitive to small s = 312, L = 2 components of the d+ p cluster in 3He and s = 2, L = 2 components of the d

+

d cluster in 4He.

Improved determinations of q(3He) are timely since recent experimental results 121 based on analytic- extrapolation methods and radiative-capture experiments yield q(t)/q(3~e) = 1.46

+

0.24 while theoretical calculations for 3H and 3He, assuming charge-symmetric nucleon-nucleon forces 131, predict q(t)h(3He) = 1.07

+

0.03. Unambiguous determinations of parameters such as q for 3He are considerably more difficult than for 3 ~ , since sub-Coulomb reactions have much lower yields and the analysis of analyzing-power measurements for higher-energy ( d , 3 ~ e ) reactions is sensitive to the choice of optical model potential (OMP) parameters.

Experimental determinations of D2 for 4He based on radiative capture and transfer reactions have resulted in a wide variety of values (- 0.31 fm2 < D2 < - 0.08 fm2). Analyses of 2~ polarized (d,y)4He reactions have been hampered by the complexity of the reaction mechanism, while previous (d,a) studies have involved uncertainties in the mixture of contributing L-transfer values. The most reliable value extracted to date, D2

=

-

0.19 st 0.04 fm2, is based on a case of appreciable L mixing 141.

2 - EXPERIMENTAL METHODS

Measurements of the 32S polarized (d?He)3IP reaction at Ed = 16 MeV were made with a vector and tensor polarized deuteron beam from the Lamb-shift polarized ion source at the Triangle Universities Nuclear Laboratory. Angular distributions of ~ ( 8 ) , Ay (8), Ayy (0) and Axx (8) were measured in an angular range

Present address: Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510

(2j Supported by the U.S. Department of Energy, Office of High Energy and Nuclear Physics

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1990647

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C6-440 COLLOQUE DE PHYSIQUE

of 15' 1 9 1 45' in 2.5' steps. The absolute cross sections were estimated to have an uncertainty of 5.4%.

Angular distributions of ~ ( 8 ) , Ay, Ayy and Ax, were measured for the 58Ni polarized (d,,u)56Co reaction at Ed = 22 MeV using the Lamb-shift polarized ion source at the Munich MP accelerator laboratory. The Q3D magnztic s-pectrograph was used to detect the exiting a particles over an angular range of 10' 1 9 5 65' in 5' steps with an experimental resolution of = 12 keV.

3 - ANALYSIS AND DISCUSSION

In the 32S(d,3He)31P reaction, the ground state (1129 and 2.23 MeV (5/2+) levels, known I51 to proceed by 2s1D and ld.512 proton pickup respectively, were strongly excited. Angular distributions of ~ ( 0 ) showed an G 0 shape for the ground state and L = 2 shape for the excited state. These transitions both represent cases of j = L

+

112 and should be especially sensitive to the presence of a D-state in 3 ~ e /6/. Figure 1 shows the measured ~ ( 0 ) , oAXx(9), oAyy(B) for these transitions. The latter quantities, called analyzing cross sections, are chosen for comparison with theory because of their insensitivity, relative to analyzing powers, to the choice of OMP parameters in DWBA calculations. They are also largest and most sensitive to q at angles where cross sections are large and such calculations are expected to most closely predict measured values.

Curves in fig. 1 are results of one-step exact finite-range DWBA calculations using the code TWOFNR with q(3He) =

-

0.048 (solid curve) and q(3He) = 0 (dashed curve). Cross section predictions have been adjusted by < 20% to match the measured cross section at forward angles for the ground state only. It has been shown for the 31p(d,3He)30Si g., transition at Ed = 16 MeV 161 that the predicted cross sections and analyzing powers are not very sensitive to the choice of three-body wave function provided similar values are used for D2 (77 is also the same to within 5% by the asymptotic ap roximation 171). Since this

S

insensitivity is also expected to appear in calculations for the 32S(d,3Re) IP at 16 MeV an overlap

9"

integral < d,p I 3He > derived from a Woods-Saxon potential consistent with the He separation energy was used in the present calculations.

3 2 ~ ( d , 3 ~ e ) 3 1 ~ Ec,=16MeV

1.2- I I 1 1 0.4

-

Z 0.8 -

\

13 0.2

E 0.4-

-

Fig. 1 - Angular distributions for 0(8), oAxx(9), c ~ A ~ ~ ( 0 ) for states excited in the 3 2 ~ ( d , 3 ~ e ) 3 1 ~ reaction at Ed = 16 MeV. The solid curve results from exact finite-range DWBA calculations assuming q ( 3 ~ e ) = - 0.048 while the dashed curve represents q ( 3 ~ e ) = 0.

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is the average of these determinations weighted by the individual uncertainties. We estimate an uncertainty in q of

+

0.006.

Our value of q is slightly larger in magnitude than obtained previously 161, however, it is consistent with the recent theoretical findings of Friar et al. 131 which predict a value of v ( ~ H ~ ) = - 0.043

+

0.001. These calculations have been made using a Faddeev equation formalism and incorporating the Coulomb interaction. When our value is combined with the average value for q(t) given in ref /2/ @jt = - 0.051

+

0.004), the ratio q(t)lq(3He) =: 1.1 1 f 0.15 is obtained, in agreement with expectations based on charge symmetry.

The 58~i(d,a)56Co reaction was chosen for a D-state parameter study since both the stretched state at 2.283 MeV having

F

= 7+ and the 5+ level at 0.576 MeV are expected to be populated with essentially pure L transfers. The (n,p) configuration expected to be transferred in populating the 7+ state is (lf7/2, lf712) leading to L = 6 transfer while the 5+ level is predicted 181 to be populated by an almost unmixed transfer of

-

.581L = 4>

-

.041L = 6> involving predominantly the (2~312 , l W 2 ) configuration. The assumption of a direct-pickup process works best for the states mentioned above since they are strongly populated. Finite- range DWBA calculations were carried out using realistic overlap functions generated by taking the Fourier transform of the d

+

d amplitudes in 4 ~ e generated from the variational wave functions of Schiavilla et al.

/I/ using the Argonne + Model VII interaction having D2 = -0.16 fm2 and the Urbana + Model VII interaction @2 = -0.24 fm2). These overlap functions for S- and D-states are shown in fig. 2.

A r g o n n e t Motlel VII

- - - - Urbana t Model VII

0 1 2 3 4 5 6 7 8

(fin

)

Fig. 2

-

S- and D- state overlap functions obtained from the Fourier transforms of fits to the d+d momentum distributions of ref. 111.

Angular distributions of Ay(8), Axx(B) and Ayy(B) for the two states in S6Co are shown in fig. 3 in comparison with our calculations employing the Argonne interaction (solid line), the Urbana interaction (dashed line) and a Woods-Saxon overlap function involving an S-state term only (dotted line). The comparisons with the 5+ state indicate that the shape of the angular distributions are reasonably well predicted with calc~llations using OMP parameters taken from ref. 181 and the predicted L-mixing amplitudes. There is not a great deal of variation in predictions using the Urbana and Argonne overlap functions, however. The DWBA calculations of tensor analyzing powers (TAP) for the 7+ state using the same OMP parameters, do show some variation with the choice of overlap function, especially for A,,. The comparisons with data indicate that the Argonne interaction provides a form factor which produces the closest comparison with experimental data. Other calculations indicate that overlap functions with the same D2, e.g., Argonne and Woods-Saxon both with D2 =

-

0.16 fm2 produce somewhat greater difference in shapes for the TAP calculatioris than observed in the 3lP(d,3He)3OSi study of ref. 161. Further calculations

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C6-442 COLLOQUE DE PHYSIQUE

will be performed using OMP parameters obtained from fits to (d,d) and (a,a) elastic scattering data. The effects of the form factor of the heavy particle system will also be investigated.

Fig. 3

-

Angular distributions of Ay(0), Ax,(%) and Ayy(0) for states populated in the 5 8 ~ i ( d , a ) 56Co reaction at Ed = 22 MeV. The curves represent exact finite-range DWBA calculations using overlap functions generated using the Argonne+Model VII inteaction (solid curve), the Urbana+Model VII interaction (dashed curve) and the Woods-Saxon potential (dotted curve).

1.0 0.6 0.2

In conclusion, TAP measurements for transfer reactions can be compared to exact finite-range DWBA calculations to test overlap functions derived from basic N-N interactions. For the 3 2 ~ ( d , 3 ~ e ) 3 1 ~ g . , . reaction, the D-state sensitivity is enhanced in oAxx(0) and oAyy(0) observables especially at forward angles fort= 0 transfers. Our analysis indicates that an overlap function with q =

-

0.048 provides a best fit in calculations of these observables. A preliminary analysis of the 58Ni(d,a)56Co reaction populating the 7+

state at 2.283 MeV indicates that of the two realistic overlap functions for the d

+

d system presented in ref.

111, the one based on the Argonne

+

VII interaction provides closest agreement with experimental TAP data.

~ ~ ~ l ~ l - ~ ~ l ~ ~ ~ , ~

: 5 8 ~ i ( d , a ) s G ~ o 7' 1 Ex= 2.283 McV

- -

REFERENCES

/I/ R. Schiavilla, V.R. Pandharipande and R.B. Wiringa, Nucl. Phys.

A449

(1986) 219.

121 B. Vuaridel et al., Nucl. Phys.

A499

(1989) 429.

131 J.L. Friar et al., Phys. Rev.

532

(1988) 2859.

141 F. Merz et al., Nucl. Phys.

A489

(1988) 399.

151 G . Th. Kaschl et al., Nucl. Phys. a ( 1 9 6 9 ) 286.

/6/ C. M. Rhat et al., Phys. Rev. C38 (1988) 1537.

/7/ A.M. Eiro and F.D. Santos, J. Phys. G; Nucl. Part. Phys.

16

(1990) in press.

181 M. Haller et al., Nucl. Phys.

A419

(1984) 45.

-0.2 - , *,

. . . . -

, . I . , . , . , .

l ~ l : l ' ~ ~ l ~ l ~ l '

0.6

, , , . 1 , ! , 1 . I . , .

I ' I ' I . I ~ I ' I ' I '

; -

\ / - \

\ ' \

, , \I

0.2 7.\\,,. -

:

I

' . .

. . . ...I . . _ _ . _ _ . . . . . .

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)

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-1.0 u

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Oc,,,(deg ) Ocm(deg )

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