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The quadrupole moment and strong interaction parameters

from muonic and pionic X-ray studies of 237Np

Citation for published version (APA):

Laat, de, C. T. A. M., Taal, A., Duinker, W., Konijn, J., Achard van Enschut, d', J. F. M., David, P., Hartfiel, J.,

Janszen, H., Mayer-Kuckuk, T., Mutius, von, R., Piller, C., Schaller, L. A., Schellenberg, L., Krogulski, T.,

Petitjean, C., Reist, H. W., & Müller, W. (1987). The quadrupole moment and strong interaction parameters from

muonic and pionic X-ray studies of 237Np. Physics Letters B, 189(1-2), 7-11.

https://doi.org/10.1016/0370-2693(87)91260-3

DOI:

10.1016/0370-2693(87)91260-3

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Published: 01/01/1987

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Volume 189, number 1,2 PHYSICS LETTERS B 30 April 1987

T H E Q U A D R U P O L E M O M E N T A N D S T R O N G I N T E R A C T I O N P A R A M E T E R S

FROM MUONIC AND PIONIC X-RAY S T U D I E S O F 237Np

C.T.A.M. D E L A A T a, A. T A A L a, W. D U I N K E R a, J. K O N I J N ~,

J.F.M. D ' A C H A R D V A N E N S C H U T b, p. D A V I D c, j. H A R T F I E L c, H. J A N S Z E N ¢, T. M A Y E R - K U C K U K c, R. V O N M U T I U S ¢, C. P I L L E R d, L.A. S C H A L L E R d,

L. S C H E L L E N B E R G d, T. K R O G U L S K I e, C. P E T I T J E A N f H.W. R E I S T f and W. M O L L E R g.h

" NIKHEF-K, NL-IO09 DB Amsterdam, The Netherlands

b Physics Department, Delft University o f Technology, NL-2629 JB Delft, The Netherlands c InstitutfurStrahlen- undKernphysikder UniversitlltBonn, D-5300Bonn, Fed. Rep. Germany d Institut de Physique, Universit~ de Fribourg, CH- 1700 Fribourg, Switzerland

e UniversityofWarsaw, Branch inBialystok, PL-15-424Bialystok, Poland f SIN, CH-5234 Villigen, Switzerland

European Institute for Transuranium Elements, JRC Karlsruhe, D- 7500 Karlsruhe, Fed. Rep. Germany h CBNM, Euratom, B-2440 Geel, Belgium

Received 17 December 1986

The X-ray spectrum of muonic and pionic

237Np

has been investigated with muons and pions stopped in a NpO2 target. The nuclear spectroscopic quadrupole moment was determined to be Q= 3.886 + 0.006 b from the splittings of the muonic 5g--,4f hyperfine complexes. The B( E2 ) J.-values for the first and second excited states were evaluated as 3.17 _+ 0.08 and 2.77 + 0.10 e2b 2, respectively. A comparison between the muonic and pionic 5g--,4f hyperfine complexes yields the strong interaction parameters for the pionic 4f state. For the first time a change of sign as function of Z for the strong interaction quadrupole shift ~2(4f) has been observed. The standard optical model predictions agree reasonably well with the measured strong interaction monopole shift, ~o(4f), and width, Fo(4f), while they disagree with the experimental value for ~2. A stronger s-wave repulsion in the optical potential could explain this effect.

F r o m the study o f m u o n i c and pionic atoms o f a deformed .heavy actinide, interesting aspects can be learnt about electromagnetic a n d strong interac- tions. The latter induces shifts, ~, and widths, F , on pionic X-ray transitions, the observation o f which has been used to construct a semiphenomenological optical potential [ 1 ]. This potential plays an impor- tant role, not only in pionic atoms but also in describing near-threshold photoproduction, radia- tive capture and in a slightly modified form low- energy p i o n - n u c l e u s scattering. The non-spherical part o f the strong and the electromagnetic interac- tion gives rise to a hyperfine splitting o f each pionic or m u o n i c level. Furthermore, by c o m p a r i n g the pionic and muonic hyperfine splitting patterns, strong interaction monopole and quadrupole parameters can be extracted. The results contribute to the investiga- tion on the earlier observed deviations between 0370-2693/87/$ 03.50 © Elsevier Science Publishers ( N o r t h - H o l l a n d Physics Publishing Division)

experiment and theory in pionic atoms [2]. As pointed out by D e y et al. [ 3 ], errors reflecting uncer- tainties in the calculation o f multi-electron systems and in estimating the electric field inhomogeneity at the nucleus and the effect o f the polarization o f the electron core do not exist in m u o n i c and pionic atoms. In the d o m a i n o f intermediate energy states for pionic and m u o n i c atoms, where the orbit size is large c o m p a r e d with nuclear dimensions and yet small c o m p a r e d with the orbits o f atomic electrons, the exotic a t o m is "hydrogen-like". The corrections for finite size, v a c u u m polarization, magnetic dipole, and electric hexadecapole effects applied to the quadrupole hfs are small for the 5 g ~ 4 f transitions. They add up to only a few percent.

The present experiment not only serves to meas- ure the nuclear spectroscopic quadrupole m o m e n t from m u o n i c and pionic 2STNp atoms but is also B.V.

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aimed at investigating the behaviour of strong inter- action parameters F0(4f) as well as ¢0(40 and ¢2(4f). In earlier studies a change in sign for ¢2 has been observed, when going from the 4f to the 3d level in the nuclei Ta and Re [ 4 ]. As the pionic states popu- lated in 237Np a r e much more bound than those in Ta, Re, Au, Pt, Pb and Bi [2,4], deviations in the strong interaction parameters such as a possible change of sign in ¢2 within the pionie 4f level, there- fore, are best looked for in the mass region of the heavy actinides.

The experiment was performed with muon and pion beams at SIN, Switzerland. The pion beam was tuned to 100 MeV/c, whereas the muons had a momentum of 50 MeV/c. Stop rates of approxi- mately 106 n -/s and 105 ix - / s were obtained in a 0.92 g/cm 2 thick NpO2 target, containing 9.981 g of 237Np. The experimental set-up includes a multidetector BGO Compton suppression spectrometer. The measuring technique has been described earlier [ 2 ]. The energy calibration was taken from accurately known energies of muonic X-rays and nuclear "t-ray transitions induced in the target and its aluminum encapsulation by the incident particle beam. The

neutron induced background transitions were well separated in time from the prompt X-rays, by using a time-of-flight path of about 60 cm between target and detector.

Regarding the muonic 2 p ~ Is, 3 d ~ 2 p and 4f--. 3d transitions one should note that several low-lying excited states belonging to the rotational band of the Nilsson ground state configuration ~ + [642] ~ in 237Np a r e mixed appreciably with the muonic 3d, 2p and Is states. Therefore, the spectroscopic nuclear quadrupole moment is derived by fitting the observed hyperfine splitting in both the muonic 6g--,4f and 5g~ 4f transitions, which have energies in the region of 0.86 and 0.55 MeV, respectively. This method has the advantage of not being sensitive to the finite nuclear size and the dynamical mixing of nuclear states. The K, L and M X-ray data were only used to determine approximate nuclear charge distribution parameters, namely the Fermi parameters c = 7.00 fm and t = 2 . 3 fro, respectively. In fig. 1 we present the hyperfine splitting of the 5g9/2~4f7/2 and 597/2--*4fs/2 muonic X-rays, the transitions of which occur with a much higher transition rate than the 6 g - , 4 f com- plexes. From the latter a moderately accurate value

i o 3 i o 2 , [ I I i I

~

't " i - - - _ _ I I I i I I I I . . . . I ' ' ' I ' ' 550 560 570 e n e r g y i n keV

Fig. 1. The muonic 5g~ 4f hyperfine complexes of 237Np are shown, the muonic 5g9/2-+ 4f7/2 complex to the left and the 597/2 ~ 4t"5/2 X-ray complex to the right. The hyperfine splitting of the two complexes is pronounced, the strongest two components of each complex being split by AE= 2.608 _+ 0.019 keV and AE= 2.863 +_ 0.021 keV, respectively. The solid line is the fit to the experimental data of the hyperfine complex, including some weak nuclear T-ray transitions from 236U and 237U.

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Volume 189, number 1,2 PHYSICS LETTERS B 30 April 1987 of Q = 3.864 + 0.055 b is obtained from the measured

energy splitting. The energy splitting of the two 5g-* 4f complexes is 10.864 + 0.022 keV between the main transitions. The splitting o f the two main compo- nents of each complex allows for two independent determinations of the quadrupole moment. From the energy splittings of 2.608 -+ 0.019 and 2.863 -+ 0.021 keY for the 5g9/2 ~ 41"7/2 and 5g7/2 ~ 4t"5/2 muonic com- plexes, respectively, a spectroscopic nuclear quadru- pole moment of Q = 3.886 + 0.006 b is derived.

Older results [ 5-8 ], though less accurate, agree well with the present result. The ground state of 241Am and the 59.537 keV state of 237Np have the same Nilsson quantum numbers: ~ - [ 5 2 3 ] $ . Therefore, within the framework of the collective model, the quadrupole moments o f these two Nilsson states should be equal, except for a small correction due to a change in nuclear deformation and a size correc- tion proportional to A 2/3. From nuclear 7-ray reso- nance measurements [ 9], the ratio of the quadrupole moment of excited state to that of the ground state and the results from muonic 241Am [ 10] one arrives at a value of Q = 3.9-+0.2 b, following the same pro- cedure as in ref. [8].

The present experimental result, Q = 3.886 + 0.006 b, is an improvement in accuracy of more than an order o f magnitude for the value o f the spectroscopic nuclear quadrupole moment. The B(E2) S-values from the first and the second excited states were evaluated, using the transition energies of the muonic 4 f ~ 3d, 6g--* 4f and 5g--,4f transitions. They amount to 3.17 -+ 0.08 e2b 2 and 2.77 _+ 0.10 e2b 2, respectively. These B(E2)$-values do confirm the old Coulomb excitation results, 3.1-+0.8 and 2.4-+0.4 e2b 2, respectively, as reported by Newton [ 6 ] but are much more precise.

In the analysis of the hfs of the pionic 5g-~4fcom- plex, i.e. the determination of the hyperfine splitting, lorentzian line width, energy and intensity, it is important to include the instrumental line shape of the photopeak, see ref. [4], since otherwise the obtained lorentzian line widths are not adequately represented by the fit. Subtracting from the fitted values the radiative widths of initial and final levels, we obtain a strong interaction monopole width of Fo(4f)=3.88_+0.26 keY and a monopole shift of co(4f)=5.26_+0.14 keV (with respect to the point Coulomb energy). These results have to be corn-

pared with the values predicted by the standard Kisslinger optical potential [ 11-13] g 0 ( 4 f ) t h = 4.16_+ 0.92 and C0(4f)th=4.54--+ 0.75, respectively. The present measurement on the pionic 4flevel and earlier results in other nuclei [ 2,4 ] agree reasonably well with the calculated values, contrary to those for the 3d level [ 2 ].

A quantity much more sensitive to the interplay between s- and p-waves in the rc-N interaction is the strong interaction quadrupole shift, C2(4f), about which very little information is available. Besides the strong interaction monopole shift and width, the observed hfs of the pionic 5g--,4f transition of the strongly deformed

237Np

nucleus also yields the effective electric quadrupole constant, A [ f f ( 4 f ) = 3.80_+0.08 keV. This quantity is directly propor- tional to the effective spectroscopic quadrupole moment, Qeff. From the difference between A [fr and the calculated electromagnetic quadrupole constant A2(4f) =4.295 keV in pionic

237Np,

the strong inter- action quadrupole shift, C2(4f ) = -I- 0.49 _+ 0.08 keV, is obtained (for the notation see ref. [ 14]). The for- mulae for calculating the quadrupole shift from experimental data for muonic and pionic atoms can be found in refs. [ 3,14 ]. In table 1 experimental val- ues are also presented calculated from other experiments.

The agreement of c 2 (4f) with standard optical cal- culations, c2 (41")th = 0.0 + 0.1, is rather poor. In addi- tion, there is a change of sign for both the calculated and experimental values for the strong interaction quadrupole shift c 2 as one goes from the 4 f t o the 3d level, whereas the monopole shift Co remains positive (i.e. attractive). In the case o f 237Np we observe, for the first time, that the sign of the experimental value of 42 (4f) is opposite to that o f the calculated one and to that of the other elements in the same pionic shell (see table 1 ). This effect is very similar to the change of sign of the strong interaction monopole shift Co observed in the pionic 2p level by Abela et al. [ 15 ]. The effect o f changing sign in both cases can be ascribed to the increasing importance of the repul- sive s-wave part in the strong interaction when the overlap between pion and nuclear wave functions becomes larger in deeper pionic orbits (see also the anomalous Fo in 3d and ls shells [2]). This change of sign is predicted to occur by theory for both Co [ 1 ] and c 2

[

14] the experimental values are not repro-

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Table 1

Strong interaction quadrupole shifts for the pionic 3d and 4f levels of some heavy deformed nuclei.

Nucleus A Set (exp) Re A2 eSxp e~heory Ref. (keY) (keY) (keY) (keV)

pionic 4f level ~65Ho 1.389+0.027 1.336 -0.053 +0.027 -0.020 [ 16] 165Ho 1.419+0.009 1 . 3 3 6 --0.083+0.009 --0.020 [ 17] 175Lu 1.688 + 0.032 1,609 -- 0.079 + 0.032 -- 0.028 [ 16 ] tSlTa 1.724+ 0.011 1.643 --0.081 +0.011 --0.031 [ 17] i SiTa 1.750 + 0.016 1.643 -- 0.107 + 0.016 -- 0.031 [4] Re 1.163+0.010 1 , 1 1 7 -0.046+0.010 -0.023 [4] 2°9Bi -0.37 +_0.05 -0.302 -0.07 +0.05 -0.009 [18] 237Np 3.80 +0.08 4.295 +0.49 +0.08 -0.018 thispaper pionic 3dlevel JS~Ta 9.1 +-0.5 9.610 +0.5 +-0.5 +4.55 [4]

Re 5.4 +_0.6 6.479 + 1.1 +0.6 +3.24 [4]

d u c e d correctly, however.

The i n d i v i d u a l contributions to the E2(4f) in 237Np for the p i o n i c 4 f state are c a l c u l a t e d to be: ~2(s) = +0.901 keV and e2(P) = - 0 . 9 1 9 keV *t. As p o i n t e d out b y K o c h a n d Scheck [ 14 ] the p - w a v e p a r t is less i m p o r t a n t in e2 as c o m p a r e d to Co. Therefore, w h e n going to h e a v i e r nuclei the p i o n i c 4 f level is m o r e d e e p l y b o u n d a n d the repulsive s-wave i n t e r a c t i o n will b e c o m e increasingly i m p o r t a n t , a change o f sign in E2 is expected before it occurs in Eo. A s i m i l a r can- cellation effect could also be the reason for the smaller theoretical values o f Eo(4f) in c o m p a r i s o n with the e x p e r i m e n t a l values for 238U a n d 237Np.

In conclusion the m u o n i c X - r a y s p e c t r u m o f 237Np p r o v i d e d us with a m o d e l i n d e p e n d e n t n u c l e a r struc- ture i n f o r m a t i o n regarding B ( E 2 ) , - v a l u e s a n d the nuclear s p e c t r o s c o p i c q u a d r u p o l e m o m e n t Q = 3.886 +_ 0.006 b, which could be d e t e r m i n e d from the hfs o f the m u o n i c 5g--,4f c o m p l e x e s to an accu- racy o f a b o u t 0.2%. T h e intrinsic q u a d r u p o l e m o m e n t s o f the n u c l e a r g r o u n d states show a s m o o t h systematic increase with increasing a t o m i c m a s s in the h e a v y actinides a n d the p r e s e n t result fits well into this regular t r e n d [ 19 ]. T h e p r e s e n t value for the i n t r i n s i c q u a d r u p o l e m o m e n t , Qo = 10.88 +_ 0.02 b, is also in g o o d a g r e e m e n t with t h e o r e t i c a l calcula-

st Unfortunately the sign definition [ 14] of the strong interac- tion quadrupole shift ~2,

A~fe=A2-~2,

yields a negative value of ~2 for an attractive interaction (p-wave), opposite to the definition of the monopole shift ~0.

tions [ 20 ]. The p i o n i c X - r a y s p e c t r u m p r o v i d e d val- ues for the strong i n t e r a c t i o n m o n o p o l e w i d t h a n d shift o f the p i o n i c 4 f level. F o r the first t i m e a change o f sign for the strong i n t e r a c t i o n q u a d r u p o l e shift E2(4f) was observed. T h e s t a n d a r d optical m o d e l calculations are in d i s a g r e e m e n t with the e x p e r i m e n - tal value for e2(4f), while the strong i n t e r a c t i o n m o n o p o l e p a r a m e t e r s F o ( 4 f ) a n d % ( 4 f ) agree rea- sonably well with these calculations.

This w o r k is p a r t o f the research p r o g r a m m e o f N I K H E F - K at A m s t e r d a m , m a d e possible b y finan- cial s u p p o r t f r o m the F o u n d a t i o n for F u n d a m e n t a l R e s e a r c h on M a t t e r ( F O M ) a n d the N e t h e r l a n d s ' O r g a n i z a t i o n for the A d v a n c e m e n t o f Pure Research ( Z W O ) . It was also s u p p o r t e d in p a r t b y the Swiss N a t i o n a l F o u n d a t i o n a n d b y the B u n d e s m i n i s t e r i u m f'tir F o r s c h u n g u n d Technologie o f the F e d e r a l R e p u b l i c o f G e r m a n y a n d b y the U n i v e r s i t y o f W a r - saw. F o r preparing the target we thank Mr.K. Richter a n d his coworkers at the E u r o p e a n I n s t i t u t e for T r a n s u r a n i u m Elements, J R C Karlsruhe, F e d . Rep. G e r m a n y .

References

[ 1 ] M. Ericson and T.E.O. Ericson, Ann. Phys. 36 (1966) 323. [2] C.T,A.M. de Laat et al., Phys. Lett. B 162 (1985) 81. [3] W. Dey et al., Nucl. Phys. A 326 (1979) 418. [4] J. Konijn et al., Nucl. Phys. A 360 (1981) 187. [5] A. Veyssi~re et al., Nucl. Phys. A 199 (1973) 45~

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Volume 189, n u m b e r 1,2 PHYSICS LETTERS B 30 April 1987 [6] J.O. Newton, Nucl. Phys. 5 (1958) 218.

[7] Y.A. Ellis, Nuclear Data Sheets 23 (1978) 71.

[8] B.D. Dunlap and G.M. Kalvius, Phys. Rev. 186 (1969) 1296.

[ 9 ] B.D. Dunlap et al., Phys. Rev. 171 (1968) 316;

J.A. Stone and W.L. Phillinger, Symp. Faraday Soc. 1 (1967) 77.

[ 10] M.W. Johnson et al., Phys. Lett. B 161 (1985) 75. [ 11 ] L. Tauscher, Proc. Intern. Seminar on ~r-meson nucleus

interaction (Strasbourg, 1971 ), Report CNRS-Strasbourg, p. 45.

[ 12] C.J. Batty et al., Nucl. Phys. A 402 (1983) 411. [13] R. Seki and K. Masutani, Phys. Rev. C 27 (1983) 2799. [ 14] J.H. Koch and F. Scheck, Nucl. Phys. A 340 (1980) 221. [ 15 ] R. Abela et al., Z. Phys. A 282 (1977) 93.

[ 16 ] P. Ebersold et al., Nucl. Phys. A 296 (1974) 493. [ 17 ] C.J. Batty et al., Nucl. Phys. A 355 (1981 ) 383. [ 18 ] R. Beetz et al., Z. Phys. A 286 (1978) 215. [ 19] J.D. Zumbro et al., Phys. Lett. B 167 (1986) 383. [20] M. Bracket al., Nucl. Phys. A 234 (1974) 185;

J. Libert and P. Quentin, Phys. Rev. C 25 (1982) 571.

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