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Submitted on 1 Jan 1975

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Nanosecond isomers in 186W

H. Karwowski, S. Majewski, B. Pietrzyk, L. Wencel, J. Jastrzebski

To cite this version:

H. Karwowski, S. Majewski, B. Pietrzyk, L. Wencel, J. Jastrzebski. Nanosecond isomers in 186W.

Journal de Physique, 1975, 36 (6), pp.471-474. �10.1051/jphys:01975003606047100�. �jpa-00208275�

(2)

NANOSECOND ISOMERS IN 186W

H.

KARWOWSKI,

S. MAJEWSKI

(*),

B. PIETRZYK

(*),

L. WENCEL

(*)

and J.

JASTRZEBSKI

Institute of Nuclear

Research, 015Awierk

near Warsaw, Poland

(Reçu

le 28 novembre

1974,

révisé le 30

janvier

1975,

accepté

le

7 février 1975)

Résumé. 2014 Les niveaux du 186W alimentés par la

désintégration

du 186Ta et par la capture électro- nique du 186Re ont été étudiés. Les spectres simples et les coincidences retardées ont été mesurés. Les temps de vie des trois isomères dans 186W ont été déterminés :

et la valeur limite supérieure de la vie moyenne du niveau à 1 463 keV,

T1/2 ~

0,1 ns, a été estimée. Les

énergies des états à deux

quasi-particules

ont été calculées et leur attribution aux niveaux observés

expérimentalement

est proposée.

Abstract. 2014 The levels of 186W fed in the

03B2-decay

of 186Ta and EC

decay

of 186Re were inves- tigated. The

single

spectrum and the delayed coincidence spectra were measured. The half-lives of

three isomers in 186W were determined :

and the upper limit of the 1463 keV level half-life

T1/2 ~

0.1 ns was estimated. Two-quasiparticle

excitations were calculated and their

assignment

to

experimentally

observed states is proposed.

Classification

Physics Abstracts

4.220 - 4.240 - 4.470

1. Introduction. - Levels of the heaviest stable tungsten

isotope 186W

have been

investigated by

several authors since 1955. Monnand et al.

[1],

Pathak

et al.

[2]

and

Gujrathi

and Mark

[3]

measured energy levels of

186W

in the

fl-decay

of

186Ta.

Coulomb

excitation methods were used

by

de Boer et al.

[4],

McGowan and Stelson

[5]

and Milner et al.

[6].

An

extensive

study

of 186W and

lighter tungsten

nuclei

were

performed by

Gunther et al.

[7].

The life-time of the first excited 122.3 keV level in

186W

has

already

been measured

by

different

methods. The data obtained

by

electronic measu-

rements

[8, 9, 10]

have the mean value

Experiments

based on the Môssbauer effect

[11, 12]

gave

Tl,2

= 1.39 ± 0.12 ns and a nuclear recoil

experiment [13]

gave

7B/2

= 1.30 ± 0.21 ns.

An indication that the 952.4 keV level has a life- time of about 0.2 ns was

given by

Monnand et al.

[1].

The aim of the present

investigation

was to deter-

mine the exact values of the lifetimes of the 122.3 keV and 952.4 keV levels.

Furthermore,

the half-life of

the 1 661 keV level was measured and an upper limit for the lifetime of the 1 463 keV level was estimated.

Single

gamma-ray spectra were also measured but

only slight

modifications to the

decay

scheme

proposed

in reference

[3]

were introduced

[14].

These modi- fications are not

important

for the present work.

Calculations of

two-quasiparticle

excitations in 186W and 184W were

performed

and the calculated confi-

gurations

were

assigned

to some

experimentally

observed states.

2.

Experimental procédure.

- The excited states of

186W

can be reached in

the p decay

of 1116 Ta

(T1/2

= 10.5

min)

and

by

EC

from 186Re (Tl/2

= 90

h).

Natural tungsten

samples

were irradiated with 14.5 MeV neutrons from a NE-246 type neutron

generator (typical

flux 5 x 109

n/s cm2)

and the

1116 Ta

activity

was obtained

by

the

(n, p)

reaction.

For the measurements of the half-life of the first excited state

samples

of natural rhenium were acti- vated

during

1 h in the flux of thermal neutrons of about

1014 n/s cm2

in the EWA reactor at Swierk.

(*) From the Institute of Expérimental Physics, Warsaw Uni-

versity, Polaud.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003606047100

(3)

472

The half-lives of the excited states were measured

using

the standard

time-to-pulse-height

converter

technique,

NaI

(Tl) crystals,

fast

plastic

scintillators connected with XP 1021

phototubes

and a true

coaxial 20

cm’ Ge(Li)

detector

[15]

were used as time

signal

generators.

3. Results. - Two

plastic

scintillators were used to determine the half-life of the 952.4 keV level

(cf. Fig. 1).

The

delayed

coincidence curve,

analyzed using

the convolution method

[16],

is shown in

figure

2.

The value

T1/2 (952.4 keV)

= 0.193 ± 0.015 ns was obtained. The lifetimes of the 396.5 keV and 737.5 keV levels do not influence the measured value since

T1/2 (737.5 keV)

= 9 ps

and, although T,12 (396.5 keV)

= 40 ps, this level is

weakly populated

in

the 186Ta decay.

Fie. l. - The simplified decay scheme of 186Ta (ref. [1, 3, 14]). The intensity limit of the 952.4 keV transition is taken from refe-

rence [14].

It was

proved

in an additional

experiment

that the

observed isomer

in 186W corresponds

to the 952.4 keV level and not to the 1 463 keV one

(cf. Fig. 1).

To avoid

registration

of the 198.0 keV and 214.9 keV transitions the energy windows in both

photomultipliers

were

chosen between 300 and 500 keV. The value

T1/2

= 0.200 ± 0.040 ns obtained in this measure-

ment is in

good agreement

with the

previous

expe- riment.

An

electron-gamma

quantum coincidence expe- riment was

performed

to determine the half-life of the 1 661 keV level. The results of one of the measure- ments are shown in

figure

3. The value of the half-

life obtained is

Tij2 (1. 661 keV)

= 4.92 + 0.10 ns.

FIG. 2. - The half-life of the 952.4 keV level. The dashed line indicates the normalized prompt curve. The full line indicates the fitted time distribution assuming the transition intensities shown

in figure 1.

FIG. 3. - The half-life of the 1661 keV level. The arrow indicates the beginning of the fitted area.

In these

experiments

the NE

111-Ge(Li) assembly

allowed a

unique

determination of the isomeric level.

On the basis of the

analysis

of the

delayed

coinci-

dence curves the upper limit of the lifetime of 1463 keV level was estimated to be 0.1 ns.

The half-life of the 122.3 keV level was measured

by Xk-Xk

coincidence.

X-rays accompanying

electron

capture and

X-rays produced

as a result of the conver-

sion of the 122.3 keV transition were measured

by

two Pb loaded

plastic

scintillators PILOT B and the value

T,12 (122.3 keV) =

1.036 ± 0.010 ns was _obtained. This result is in

good

agreement with the

previous

electronic measurements and is

substantially

lower than the one obtained in the

experiments

based

on the Môssbauer effect.

(4)

4. Discussion. - 4.1 GENERAL CONSIDERATIONS.

- The

simplified decay

scheme of 186Ta based on

references

[1, 3, 14]

is shown in

figure

1. The

1116 Ta ground

state

configuration

can be

1/2 -(510), 7/2+(404)

with W = 3 - or

3/2-(512), 7/2 + (404)

with Kn = 5 - .

Both

configurations

were

previously proposed [1, 3]

and are consistent with the

experimental

data.

The low

log ft

value of

the f3

transition

leading

to

the 1661 keV level

(ah

or 1 u

transition)

indicates that this level should be

mainly

of a

two-quasiparticle

nature with one

particle

in the same orbital as in 186Ta

ground

state.

The 1 661 keV level

decays preferentially

to the

1 463 keV state. The 198.0 keV transition has a retar- dation factor

FsP

= 2.1 x

105, typical

for the one

particle

El transition in deformed nuclei.

Therefore, although

a two

phonon interpretation

was

proposed

for the 1 463 keV level

[3],

a

two-quasiparticle

confi-

guration

can also be considered. In this case one should find for this level a

configuration

in which

only

one

particle

is in a différent orbital in

comparison

with

the 1 661 keV state and for which the El transition is of the OSl

= 0,1

type. This

configuration

should

also

explain

the

decay properties

of the 1 463 keV state,

taking

into account the nature of the 952.4 keV

and 1 045.0 keV levels.

4.2 THE 952.4 keV LEVEL. - The Kn = 2- characteristics of the 952.4 keV and 1 045.0 keV levels are now well established

[1, 3, 7].

For the analo-

gous level at 1 290 keV excitation energy

in 182W

the main

two-quasiparticle configuration contributing

to this

octupole

excitation was found to be

[17]

pp,

§’(514), 5/2 + (402).

Our numerical calculations for

186W

indicate that this

configuration

is at 0.98 MeV.

Also the two neutron

configuration 2/7 - (503), 11/2 + (615)

has low energy

(Ecale

= 1.1

MeV)

and may contribute to this excitation.

The

decay

characteristics of the 2-

octupole

vibra-

tional level were

investigated previously

in many nuclei in this

region.

It has been shown

[18-23]

that a

significant mixing

of E 1 + M 2 + E 3

multipolarities

exists in the 2-

> 2g+

transition. A recent

compilation

of the transition

probabilities

from this state

in 174 Yb, 176Hf, 180W and 182W

nuclei can be found in refe-

rences

[18, 19].

In the case

of 186W

the energy difference of the 2-

octupole

level and the

2+

level is much

higher

than in

the

previously

mentioned nuclei and the main

decay

of the 2- level

proceeds by

an El transition to the

2+

state.

Assuming

pure

multipolarity

the

single particle

retardation factor for this transition is

equal

to

1.0 x 104.

Although

as in other nuclei in this

region

the

2- ->

2+

830.0 keV transition is

probably

also an

El + M2 + E3

mixture,

no

experimental

data are

available to evaluate the

mixing

ratios.

Assuming by analogy

with 18 2B W

[19]

that the El component takes about

50 %

of this transition

intensity,

one

obtains the El retardation factor of 4 x

10’,

i.e.

of the same order as in

176Hf (5

x

10’), 180W (4

x

10’)

and

i82W (7

x

10’).

4. 3 THE 1463 keV ANn 1661 keV LEVELS. - Direct

experimental

evidence

concerning

the

spin-parity

of the levels discussed is not decisive.

However,

based

on the

qualitative

considerations in section

4.1,

the

nature of the 952.4 keV leBtel and our

two-quasipar-

ticle state calculations

(cf. Fig. 4)

the

following

confi-

gurations

for these levels can be

proposed :

FIG. 4. - Calculated two-quasiparticle excitations. Calculation

procedure is described in references [17, 27]. Deformation parame- ters are taken from reference [28].

The 1 463 keV level is connected with the

2-,

952.4 keV state

by

the 511 keV transition. The expe-

rimentally

determined

[1]

conversion coefficients of this transition

indicate,

within the limit of errors

(Monnand,

E. and

Moussa, A., private

communi-

cation),

El or E2

multipolarity

and therefore do not contradict the

proposed

values of

spin

and

parity

of the 1 463 keV level.

For both

previously

mentioned

configurations

of

the 186Ta ground

state the

fl-transition

to the 1 661 keV

level is classified as 1 u, in agreement with the expe-

rimentally

determined

[1] log ft equal

6.2.

With the

configuration proposed

for the 1 661 keV and 1 463 keV levels the 198.0 keV transition would

(5)

474

occur between

2 +(404)

and

2 -(514)

orbitals. In the

odd-A nuclei the retardation factor of the

analogous

E 1 transition

[24]

varies from 4 x 104 for

181Ta

to 3 x 106 for 177Lu. The

preferential decay

of the

1 463 keV level to the 2- state is

explained

as E2

transition between

2 + (411 )

and

2 + (402)

orbitals.

The 1n’ = 5 - state of nn

2 - (510), 2 + (615)

confi-

guration

was

recently

identified in

184w (cf.

ref.

[25, 26])

at the energy of 1 285 keV

(Ecale

= 1.3

MeV).

The calculated energy of this state in

186W

is

equal

to 1.1 MeV. The

feeding

of such a level from the 1 661 keV and 1 463 keV states is not observed

[1, 3, 4].

This fact can be

easily explained

within the

proposed

configurations

because transitions to this 5 - state would

require

a

change

of two

particles.

It should be mentioned that no other

configurations

for the considered levels were found which could

explain

all of the

experimental

data discussed above.

We would like to thank Mr A. Sulik for

running

the neutron generator for many

hours,

to Doctors

J. Blocki and W. Kurcewicz who

put

to our

disposal

their

two-quasiparticle

calculation code and to Mr W.

Szymczyk

for his

help

in some

experiments.

We are

greatly

indebted to Prof. J. Zakrzewski

for his kind interest in the progress of the present work.

References

[1] MONNAND, E., BLACHOT, J. and MOUSSA, A., Nucl. Phys.

A 134 (1969) 321.

[2] PATHAK, B. P., MURTY, K. S. N., MUKHERJEE, S. K. and GUJRATHI, S. C., Phys. Rev. C 1 (1970) 1477.

[3] GUJRATHI, S. C. and MARK, S. K., Can. J. Phys. 51 (1973) 241.

[4] DE BOER, J., GOLDRING, G. and WINKLER, H., Phys. Rev. 134 (1964) B 1032.

[5] MC GOWAN, F. K. and STELSON, P. H., Phys. Rev. 122 (1961)

1274.

[6] MILNER, W. T., MC GOWAN, F. K., ROBINSON, R. L., STELSON,

P. H. and SAYER, R. O., Nucl. Phys. A 177 (1971) 1.

[7] GUNTHER, C., KLEINHEINZ, P., CASTEN, R. F. and ELBEK, B., Nucl. Phys. A 172 (1971) 273.

[8] KURFESS, J. D. and SCHARENBERG, R. P., Phys. Rev. 161 (1967) 1185.

[9] GOLDRING, G. and VAGER, Z., Phys. Rev. 127 (1962) 929.

[10] BIRK, M., BLAUGRUND, A. E., GOLDRING, G., SKURNIK, E. Z.

and SOKOLOWSKI, J. S., Phys. Rev. 126 (1962) 726.

[11] OBERLEY, L. W., HERSHKOWITZ, N., WENDER, S. A. and CARPENTER, A. B., Phys. Rev. C 3 (1971) 1585.

[12] MEKSHES, M. W. and HERSHKOWITZ, N., Phys. Rev. C 2 (1970)

289.

[13] ASHERY, D., BAHCALL, N., GOLDRING, G., SPRINZAK, A. and WOLFSON, Y., Nucl. Phys. A 101 (1967) 51.

[14] KARWOWSKI, H., MAJEWSKI, S., PIETRZYK, B., WENCEL, L.

and JASTRZEBSKI, J., INR Report, to be publ.

[15] SZYMCZYK, W. and KARWOWSKI, H., INR Report 1446/IA/PL,

1973.

[16] KACZAROWSKI, R. and PIETRZYK, B., INR Report 1422/IA/PL,

1972.

[17] GALLAGHER, C. J. and SOLOVIEV, V. G., Kgl. Dan. Vid. Sels. ; Mat.-Fys. Skr. 2, 2 (1962).

[18] SCHMIDT, A. G., MICHELICH, J. W., FUNK, E. G., MADDEN,

M. S. and RIEDINGER, L. L., Proc. Int. Conf. on Nucl. Phys.

München 1973 p.301.

[19] SCHMIDT, A. G., MICHELICH, J. W. and FUNK, E. G., to be

published, in Nucl. Phys.

[20] LOBNER, K. E. G., SMITH, H. A. and BUNKER, M. E., Nucl.

Phys. A 179 (1972) 276.

[21] KONDN, J., GOUDSMIT, P. F. A., KOLDEWIJN, P. and MEYER, B. J., Proc. Int. Conf. on Nucl. Phys. Munchen 1973 p. 302.

[22] KONIJN, J., MEIJER, B. J. and VAN MIDDELKOOP, G., Phys.

Lett. 35B (1971) 567.

[23] KRANE, K. S., SITES, R. and STEYERT, W. A., Phys. Rev. C 5 (1972) 1104.

[24] LOBNER, K. E. G. and MALMSKOG, S. G., Nucl. Phys. 80 (1966)

505.

[25] YATES, S. W., DALY, P. J., JOHNSON, N. R. and ARAS, N. K., Nucl. Phys. A 204 (1973) 33.

[26] KLEINHEINZ, P., DALY, P. J. and CASTEN, R. F., Nucl. Phys.

A 208 (1973) 93.

[27] NATHAN, O. and NILSSON, S. G., in Alpha-, beta- and gamma- ray spectroscopy edited by K. Siegbahn (North Holland, Amsterdam) 1965.

[28] GABRAKOV, S., KANIOWSKA, T., ZIELINSKA-PFABÉ, M., Acta.

Phys. Pol. B 5 (1974) 295.

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