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ANNALES

UNIVERSITATIS MARIAE CURIE-SKŁODOWSKA LUBLIN —POLONIA

VOL. XL/XLI, 22 SECTIO AAA 1985/1986

Instytut Fizyki UMCS

W. A. KAMINSKI, J. WAWRYSZCZUK

The Extended Core-coupling Scheme with Example for the “’Gd

Rozszerzony schemat sprzężenia rdzenia z cząstką na przykładzie H’Gd Расширен. в ..я схема сопряженного остова с применением к 14,Gd

Dedicated to Professor Stanisław Szpikowski on occasion

of his 60th birthday

1. INTRODUCTION

The core-coupling model of Thankappan and True [l], which is in fact extending de'Shalit’s ideas [21, has been applied to a wide range of atomic nuclei. The early papers (e.g.[5], [4].[5]) demonstrated the utility of this model for the interpretation of energy levels, reduced transition probabilities and spectroscopic factors in the lighter nuclei: copper, strontium, ytterbium. The core states were coupled to the possible single-particle states of the outermost-odd nucleon in all these cases. The Hamiltonian contained both the dipole-dipole and the quadrupole-quadrupole

forces.

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284 W. A. Kamiński, J. Wawryszcxuk

In the present paper we try to apply the core-coupling model to the interesting region of A ''•150. The results have preliminary character and further studies of the model are continued.

In the model there is a plethora of parameters. As the first order of approximation we took their values accepted in the neigh­

bouring regions and then investigated the effect of a variation of the parameters. There were nine parameters in our calculation and some of them, in general, did not have strong effects on levels splitting. Thus, although we paid attention to the computation of the right values of the parameters, there can appear some ambigui ­ ties.

A number of experimental works have been done lately on the 147gd (e.g.[6], [7], [81 ,[9} ). It was found that in this nucleus the strong single-character spectra and many members of multiplets connected with the 3~ and 2+ core states were populated.

Liany of the published theoretical works, however, have not shown a good agreement with the basic features of energy schemes and specially with reduced transition probability and magnetic mo­

ment values [1O1. A more phenomenological investigation [111,[12J could be useful, in such a situation, for a systematic study of the general behavior of the core-odd particle interaction para ­ meters.

2. THEORY

The Hamiltonian for an odd-A nucleus near closed shells can be taken in the model as

H = Я с + Hgp + Hint (1 )

where Hc is the core Hamiltonian, - the Hamiltonian of the single particle outside the even-even core, and t is the Kami 1 - tonian of the interaction between the particle and core excitations

(collective vibrations, rotational or multi-quasiparticle excita­

tions). A ground foundation is the weakness of the odd-particle- -core force in comparison with the interaction of nucleons of the core. Then, H^^ may be formally expanded as a series of mil t-i pni p -

-multipole interactions

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The Extended Core-coupling Scheme 285

H int = • æiP (2)

In eq. (2) is an unknown strength for the к-range multipole- -multipole force, and T^k^ * means a scalar product of the core multipole tensor

= Ёл A-1 Yk^i ’ fi) <5>

and the odd-particle multipole operator

к ft,

^sp = r sp Y k9€^sp ’ ^sp)

The sum in eq. (3) is extended on all nucleons in the core.

In all the reported applications of the model the authors had taken into account two terms of eq. (2) only. Ke included, additionally, the third term which is necessary for the right interpretation of spectroscopic characteristics of the ^^Gd.

We have therefore, in the form

fe у (3) (3)

Hint = -5 Jc- sp "7%-%p "He • T SP (5)

named nextended". J c j sp eq (5 ) are the angular mo- mentum operators for the core and the odd nucleon respectively, Q c and Qs p are quadrupole and T^p\ octupole operators.

Only an explicit form of the single-particle operators will be needed. The matrix element of the Q c and T^) are parametrized in the manner of paper [l].

The eigenstates |(jSpJ c )i M of tb e Hamiltonian (1) can be

taken as a linear combination of the angular momentum coupled

eigenfunctions of the HQ + Hsp part.

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286 W. A. Kamiński, J. Wawryszczuk

E % j |i Sp>lJ o> “ >

W.

I is the total angular momentum for a system of the core (with the angular momentum J ) and the odd particle (with angular mo- mentum J 8 p)' æhe c j are » 'thus, the probability amplitudes describing the states (6) in terms of the simpler basis functions

The ordinaiy procedure for finding energy levels involves diagonalization of the Hamiltonian (1) to compute its eigenvalues.

The single particle energies of H__ sp are treated as further para- meters of the model. Their initial values are taken to be equal to the experimental single particle energies £13].

In the calculations we adopt the harmonic-oscillator wave functions with h6i= 41 A-1^ ag the single-particle functions.

Further details of the model are straightforward and the final forms of the needed matrix elements can be obtained by the standard methods of the angular momentum technique [141.

The computer code allows for a self-acting fit of the energy levels and transition probabilities to the experimental ones. As a result we obtain the coefficients cï T and, therefore, the

“ sp J c structure of the eigenfunctions (6).

This information is sufficient for an extraction of some ad ­ ditional interesting nuclear properties of the A+1 nucleus! e.g.

quadrupole moments, magnetic moments, spectroscopic factors for the transfer of a single nucleon to the core can be calculated.

All these quantities are good- tests for the utility of the model.

The core-coupling model is of the feature that very little assumption is made about core states. The reduced matrix elements of multipole operators are taken to be parameters fitted to the experiment. In the model they are not derived from any model.

The approximation in the model arises from the assumed anti ­ symmetry of the wave function. The states | (. . gM S in eq. (6)

^sp “ c '

are taken as vector-coupling states. The states [ Jo> , however,

contain an amplitude from single nucleon in the jq p orbit and

thus, strictly speaking the state |3sp^> is partially blocked

according to the Pauli principle. Our approximation will, in con ­

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The Extended Core-coupling Scheme ... 287 sequence, be working well only if the blocking effects are rela­

tively small.

3. RESULTS AND DISCUSSION

The preliminary results we have reported concern the ^^Gd nucleons, which belongs to the interesting region A ~ 150. In the presented calculation we demonstrate the possibility of the ex­

tended core-coupling model application to the nucleus under dis ­ cussion.

The 147gd has 64 protons and 83 neutrons. The even-even core is taken to be active by only collective excitations (in the sense we wrote about in the THEORY). The eighty-third neutron is treated as single nucleon which is distributed between single particle states: f?/2 » * 13/2 ’ h 9/2 ’ p3/2 pl/2 ’ Hi8her configurations are not included in the model space because of their large exci ­ tation energy. In the paper we adopted single-particle energies

[13] as a first step of the fit procedure and the core excitations shown in Table 1.

Table 1.

! ^°Gd J ! Energy (keV)

j 3" ; 1579

J 2 + } 1972

! 5" ! 2658 J L--- L____________J

This choice provides as set of parameters the matrix elements of the core multipole operators:

,Х02=г<° + KU 2+>;

X22=^<2+ 4 M 2+>

^55 = 5‘ (I * 0 U

X33 3'hJ 3' >i

35 HUO *

03 =$< o+ K 5) !l 3“> -,

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288 W. A. Kamiński, J. Wawryszczuk

Y 23 = 5 ->» Х25 = ï <2 + 11 т 0 (5) |1 5’>.

The best fit of level scheme was attained for the parameter values presented in Table 2. The energies of the calculated states are

Values of parameters

Г--- --- --- -,--- --- MeV • fm z ii MeV • fm ' u MeV

--- ---.--- --- --- J--- --- #— —.

Table 2.

b---

1________ 02 55 35 22 55 !! 03 II

1 II 25 1 25 !!

1

li

1 1

! 0.000 L______ J

-0.139 0.097 0.049

II II 0.114

*

1 0.009

It li

II - .. J

1 li

1 il

0.009 ! 0.014 il 0.017

1 il

1

li

_______ i_______ U________

reproduced well (Table 3). The 1/2+ (1292 keV), 2+ (1412 keV),

?/2+ (1628), $/2+ (1642), V2 + (1701) states are members of the (3" ® 7/2 “) multiplet. Two of these states ( 1 /2~ and V2 + ) are other spectroscopic characteristics in the literature £l31. Our results were confirmed on the grounds of the transition probabi­

lities and magnetic moments analyses. The levels: 2~ (g.s.),

^/2“ (1.152 keV), 1 /2“ (1.847) have a strong single-particle cha racter and we obtain their "unperturbed" energies: f7/ 2~ keV) p 3/2~ keV)> S9/2“ keV), P.|/2 “ (18 42 keV) which are very closed to those deduced from experiment [13].

More detailed analyses based on the reduced transition pro­

babilities and quadrupole and magnetic moments are not possible in the wider scale because of very limited data on the 1 ^^Gd nuc ­ leus. In the case of the best fit we can calculate only the value listed in Table 4. Comparison of the E3 reduced transition proba­

bility proves that the state 1 ’/2+ (998 keV) has very strong col ­ lective admixture. Л coherent interpretation of the experimental data needs to place the i-jj/g * sinsbe^particle state about 2116 keV above the f?/ 2.

Concluding, we can confirm the utility of the model as a way of data interpretation (energy levels, spectroscopic factors, re­

duced probability transitions). 17e are able to reproduce the

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The Extended Core-Coupling Scheme 289

Table 3.

1 --- [ State J i i

Energy (keV ) 1 Theoiy j Experiment t

! 7 /2- g.s. -0.08 0.0

1 _ _ _ J

! 15/2 + 1014 998

1 ....

3 /2-

1 ' 1151

1 1

! 1152 j

1 .

! 1/2+ 1273 1292

! 9 /2- 1401 1398 J

! ’ /2 * 1402 1412

! 7 /2 * 1645 1 1

162E

9/2 + 1656 1643

! 11 /2 + 1664

I I

I 1701 J 9 /2" 1799

I I

1797

! 1/2" 1842 1847

! 17/2+ 2480

I I

! 2488

1 ____________ __ t________ _________ I Table 4.

Theory " Experiment ■ -'J n'si Quadrupole moment

13/ 2 + (998 keV) (b)

-0.70 a ) ±(0.73 * 7)

B(E3: 15 /2 +--- 7/2~g.s.

(e2 fm6 ) 55 10 5 b>

(56±4 )•105

Magnetic moment ( u^ ) i ____________________ ‘______

-0.24 C)

_________________

(-0.24±0.07) -1 a) effective charge e^2= 1.99e

b) effective charge = 2.5e

C) gc = Z/A = 0.44-, gl = O.Oj g®ff = 0.&g * ree = -2.29/^

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290 W. A. Kamiński, J. Wawryezczuk

strength of the core-odd particle interaction and unpeturbed single-particle energies.

We have not discussed, however, higher power effects in the core-single nucleon interaction and its influence on the change of the core structure. All these problems may be included in the model in a simple way.

Some other extensions of the core-particle scheme are easy to reach [16] . Especially, an. addition of more than one particle

and a definition of a structure of the core Hamiltonian are pro­

mising cases. We develop the searches with the IBM-r1 Hamiltonian for the A=148 core.

REFERENCES

[Ü. T h a n k a p p a n V. K. and True W. W.: Phys. Rev.

1965, 157B, 795.

[^.Shalit de, A.: Phys. Rev. 1961, 122, 1530.

[$Hoffuann-Pinther P. and A d a m s J. L.:

Nucl. Phys. A, 1974, 229, 365.

(4 D a 1 t o n B. J. and Robson D.: Nucl. Phys. A, 1973, 210, 1.

A dam a J. L.: Phys. Rev. 1979, 20C. 1542.

[^.Kleinheiz P.: Phys. Scr. 1981, 24, 236.

[4 B a k a n d e r 0. et al.: Nucl. Phys.A,1982, 389, 93.

P i i p a r i n e n M. et al.: Z. Phys. 1982, 309, 87.

H. W a r d D. et al.: Nucl. Phys. A, 1983, 397, 161.

fl cj. Liotta R.J.,Pomar C., Silvestre Brae B. A.: Lett. Nuovo Cimento 1980, 27, ser. 2, p. 100

fl 4. Bossing T., Neergard K., Sagawa H.:

J. Phys. Colloq. 1980, 410, 79.

[l2j. 17 a n g M. C. Hsieh S. T.: Lett. Nuovo Cimento 1982, 34, ser. 2, p. 370.

[l3j. K d m p p a T. et al.: Z. Phys. A, 1983, 314, 33.

[Ц. Kamiński W. A. and Wawryszczuk J.: Jader- naya Fizika (in Russian) - to be published

[1^. Hàusser O. et al.: Nucl. Phys. A, 1982, 379, 287.

[16]. Broglia R., Maglione F. and V i t t u r i A.:

Nucl. Phys. A, 1982, 376, 45.

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Rozszerzony schemat sprzężenia rdzenia ... 291

STRESZCZENIE

W pracy dyskutuje się hamiltonian oddziaływania cząstka- -rdzeń z siłami multipolowymi zawierającymi człony do rzędu TL < 3. Dzięki zastosowaniu parametryzacji elementów macierzo­

wych operatorów charakteryzujących rdzeń nie wymagana jest zna­

jomość jawnej ich postaci. W teorii traktuje się je jako swo­

bodne parametry dopasowywane do eksperymentalnych danych.

Model został zastosowany w jąderze atomowym 1^^Gd. Poka­

zano użyteczność wprowadzonych przybliżeń, a w szczególności niezbędność włączenia do hamiltonianu członów zawierających od­

działywanie oktupol-oktupol.

РЕЗЮМЕ

В работе рассматривается гамильтониан взаимодействия час­

тица-остов с мультипольными силами содержащими члены ранга X ( 3. Благодаря применению параметризации матричных элемен­

тов операторов описывающих остов - не требуется их явной формы.

В теории рассматривается их как свободные параметры подгоняе­

мые к экспериментальным данным.

Эта модель применяется к атомному ядру 147 g < i . Демонстри­

руется применимость введенных приближений, а в частности необ­

ходимость включить в гамильтониан членов учитивающие октуполь-

-октупольное взаимодействие.

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