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HAL Id: jpa-00207314

https://hal.archives-ouvertes.fr/jpa-00207314

Submitted on 1 Jan 1972

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L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.

Lifetime measurement of the first excited state in 22Ne

H. Sztark, J.L. Quebert, P. Gil, L. Marquez

To cite this version:

H. Sztark, J.L. Quebert, P. Gil, L. Marquez. Lifetime measurement of the first excited state in 22Ne.

Journal de Physique, 1972, 33 (10), pp.841-845. �10.1051/jphys:019720033010084100�. �jpa-00207314�

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LIFETIME MEASUREMENT OF THE FIRST EXCITED STATE IN 22Ne

H.

SZTARK,

J. L.

QUEBERT,

P. GIL and L.

MARQUEZ

Centre d’Etudes Nucléaires de

Bordeaux-Gradignan, IN2P3,

Le

Haut-Vigneau, 33-Gradignan (Reçu

le 20 mars

1972,

révisé le 2

juin 1972)

Résumé. 2014 La vie moyenne du

premier

état excité de 22Ne

(2+,

1,277

MeV)

a été mesurée par la méthode du parcours de

recul,

à l’aide de la réaction

19F(03B1, p03B3)22Ne

à basse

énergie :

les rayonne- ments 03B3 ont été détectés en coïncidence avec les protons émis à 170° du faisceau incident. La vie moyenne trouvée est : 03C4 =

(5,9 ± 0,6)

ps.

Abstract. 2014 The mean lifetime of the first excited state of 22Ne

(2+,

1,277

MeV)

has been mea-

sured

by

the recoil distance

Döppler-shift method, using

the reaction

19F(03B1,

p03B3)22Ne at low energy.

The 03B3-rays were recorded in coincidence with the protons emitted at 170° to the incident beam.

The mean lifetime was determined to be : 03C4 =

(5.9 ±

0.6) ps.

Classification : Physics Abstracts 12.00, 12.13, 12.20

1. Introduction. -

Among

the nuclear informations that can be deduced from

experiment,

the lifetimes

of the excited states are

directly

connected with nuclear models

by

means of the reduced transition

probabilities.

In the

region

between

10-10

and

10-12

s, the «recoil-shift méthode

[1], [2], [3]

is

the

only

one which has

proved

to be

sufhciently

accurate.

Indeed, by

this method the average recoil

velocity

can be

accurately

known

by measuring

the

energy difference between the y-rays emitted

by

recoil-

ing

and

stopped

nuclei.

We

adjusted

this

technique

to very low

energies

with 2.9 and 4 MeV

a-particles

as

projectiles,

and we

applied

it to the 1.27 MeV state of

22Ne :

the mean

lifetime enables us to calculate the

B(E2, 0+ - 2+)

of the 1.27 MeV

level,

that we have

compared

with

previous

results on

quadrupole

moments,

using

the

rotational model.

II.

Expérimental

method. - The

experiments

have

been

performed

at the 4 MeV Van de Graaff from the CEN de

Bordeaux-Gradignan.

Because of the

low incident energy, we had to choose an

exoergic

reaction to

get

a recoil

speed

sufhcient for the studied

nucleus. We used the reaction

19F(a, p) 22 Ne,

whose

Q-value

is 1.698

MeV,

at two incident

energies :

2.9 and 4

MeV,

with a beam of about 50 nA

intensity.

The thin

targets

of

F2Ba (30 Jlg/cm2)

were

evaporated

onto a copper foil 1 gm thick : this was then stretched

to

get

a surface as flat as

possible.

The

recoiling

nuclei were

stopped by

a brass

plun-

ger, movable with

regard

to the

target,

the surface of which was

thoroughly parallel

to the stretched

target :

the distance d between

target

and

plunger

is

determined by measuring

the

capacitance

between

these two

surfaces,

and was known with an accuracy of ± 1.5 gm.

The y-rays emitted

by

the

recoiling

nuclei were

recorded

by

a 60

cm’ Ge(Li)

coaxial detector at

to the beam : this detector has a resolution of 2.5 keV for the 1.27 MeV

22Na

line.

To

get

a

good separation

of the two

y-lines

and a

good

definition for the recoil

velocity,

the y-rays were

recorded in coincidence with the backscattered

protons

associated with the

recoiling

nuclei. These

protons

are detected with a surface barrier

ring-counter,

at

180° to the incident beam : to

stop

the

a-particles

diffused

elastically

at 1800

by

the brass

plunger,

we

put

a 20 gm aluminium foil in front of the

ring-

counter, the thickness of which was calculated to

stop

the diffused beam and let go

through

the back-

scattered

protons.

The size of the detector defines the directions of the recorded

particles,

and then

those of the

recoiling

nuclei taken into account :

so, the recoil

velocity

is very well established. More-

over the coincidence

circuit,

of the multidimensional

kind,

allows us to choose a well defined energy group of

protons,

and

then,

the y-rays

coming

from the

decay

of a well defined level

(the

first of

22 Ne

in our

case) :

so, we can avoid

possible feeding

of the studied

level

by

a

decay

of

higher

states.

On

figure 1,

one can see the difference between direct

spectra

for distances d = 6 and 30 gm, and the same

spectra

in coincidence with

protons :

we can see the

advantage

of this last method in the definition of the two

y-lines.

From the energy difference AE between the two lines of the coincidence

spectra,

we can determine

accuratly

the

recoiling

nuclei

velocity

v,

after correction for the effective solid

angle

at the.

Ge(Li)

detector

[3].

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019720033010084100

(3)

842

FIG. 1. - Comparison between direct and coincidence y spectra.

Coincidences are obtained with protons emitted at 170° to the incident beam, at 2.9 MeV incident energy.

In our

experiment,

the direction of the

recoiling

nucleus is very well known and no other corrections

are needed. On the

contrary,

if we want to evaluate this

velocity

from the direct

spectra

we have to consi- der other

corrections,

as described in reference

[1].

We obtained the effective

values, for fi

=

v/c :

III. Results and

interprétation.

-1. EXPERIMENTAL

DATA. -

Figure

2 shows some of the

spectra

obtain- ed in coincidence with

protons,

as a function of the

stopping distance,

for 4 MeV incident energy. The variations in the relative intensities of the shifted and unshifted

peaks

can be

clearly

seen : all

spectra

were normalised to

keep

a same total surface.

The same

experiment

was made with a 2.9 MeV

incident energy.

For each

distance d,

we calculated the surfaces u

and s of the two

y-lines

after

subtracting

the back-

ground,

evaluated on the most distant

spectrum (d

= 79.4 pm at 4

MeV).

In this kind of measurement, it is necessary to make

a number of corrections as described in reference

[3].

Many

of these corrections are

negligible

in our case ;

for

instance,

all corrections due to the variations of solid

angles

are very

small,

because of the very short distances involved. In the same way, the variation in the counter

einciency

for the shifted

peak

leads

to an increase of

0.7 %

in the shifted

peak intensity.

The most

important

correction is due to the varia- tion of the

angular

distribution of the y-rays emitted

FIG. 2. - y spectra in coincidence with protons emitted at 170° to the incident beam, for distances d between 9.4 and 79.4 pm. These spectra come from a 4 MeV incident energy.

All the spectra were normalised on the spectrum corresponding

to the higher statistic (d = 23.2 pm) to keep the same total surface (Iu + Is).

by

the

recoiling

nuclei. We measured the

angular

distribution of the y-rays emitted

by

the

stopped nuclei, by using

a thick

F2Ba target to stop

the recoil-

ing

nuclei.

Figure

3 shows the

experimental

results

fitted with an

expression

of the form :

where

Q2

and

Q4

are the finite

geometry

correction factors.

The

angular

distribution of y-rays emitted

by

the

recoiling

nuclei is modified and can be

written,

at 0° :

with

This leads to a decrease in the shifted

peak

inten-

sity

of 1.5

%.

(4)

FIG. 3. - Angular distribution of y-rays in coincidence with protons emitted at 170° to the incident beam.

e experimental points normalised by the particle spectrum.

- theoretical curve : W(O) = 1 + a2 P2 (cos 0) + a4 P4(cos 0).

2)

INTERPRETATION. - We assume that the

2’

level can

only

be fed

by

direct excitation. This is the

case for the reaction studied because the

feeding by higher

states is

rejected by

the coincidence method.

The

decay

law is :

We then have :

where T is the time of

flight corresponding

to the

distance d : T =

d/v.

If we assume no

dependance

in time for the

angular

distribution of the y-rays, we have :

which

gives :

In

fact,

a nucleus

recoiling

in vacuum is

subject

to the field of its electrons which modifies the

angular

distribution of the emitted y-rays. To take this effect into

account,

we used the

expressions given by

Ben

Zvi et al.

[4],

and the values measured

by

Nakaï

et al.

[5]

for the

integral

attenuation coefficients

G2

and

G4 :

The intensities

I.

and

7g

can then be

written,

at 0° :

These

expressions

lead to a value of F as a function

of the distance d. A

least-square

fit program

gives

the

best value of the mean

life r,

from the corrected values

F(d)

as a function of the distance.

Figure

4 shows

the

experimental

data

points

for

F(d)

versus the

stop- ping distance,

for the two studied

energies :

the

straight

line is the best fit curve.

FIG. 4. - Plot of Log

[ (I. iu + is)-l

versus the separation dis- L(iu u -E- 7s)

tance between target and plunger. The lower curve displays experimental results at 4 MeV, and the upper one the results at 2.9 MeV. The distance origin is arbitrary, because it is an

adjustable parameter.

|

.

2022 experimental points.

- best fit curve.

3. EVALUATION OF THE ERROR IN THE MEAN LIFE i. - The mean life is

dependant

on three expe- rimental

parameters fi

=

v/c,

F and d.

The error

on f3

is

easily

calculated from the esti- mate of the center of

gravity

of the two rays. For the

two other sources of error, we simulated a series of

experiments by replacing

in the

expression

of F

against d,

the

experimental

results F and d

by pseudo-

random

weighted

values. The series of best fits so

obtained enable us to extract errors

coming

from the

experimental

values of F and d.

(5)

844

Results. - After corrections as mentioned above and error calculations

including AT(d, F, B),

we

finally

obtained :

which

gives

the average :

IV. Discussion. - After correction due to the internal conversion coefficient as calculated

by

Rose

[6],

the mean lifetime

gives

the reduced transition

probability :

FIG. 5. - Comparison between our results and previous

results. In the lower figure, we show B(E 2) values, in e2 b2 units, for the 0+ -> 2+ transition. In the upper figure are the intrinsic

quadrupole

values in barn. References are as follow : a) Reference [1].

b) Reference [7].

c) Reference [13].

d) Our measurement.

e) We calculated Qo with the expressions (3) and (4) using Morand’s [12] results.

f ) Same calculations using Raynal’s [11] results.

g) Reference [8].

h) Our result, using the rotational model and the adopted sign

of Qo.

Figure

5 shows the

comparison

between the value of

B(E 2)

found

by

our measurement with the results found

by

Jones et al.

[1] ]

and Eswaran et al.

[7].

By using

the rotational

model, the

transition pro-

bability

is

directly

connected with the intrinsic

quadru- pole Qo

of the rotational band :

the static

quadrupole

moment of the studied level

being :

The static

quadrupole

moment

Q(2+)

was measured

by

Nakaï et al.

[5], [8]

and Schwalm et al.

[9] using

the reorientation effect

[10].

We have

compared

these

results with the value deduced from eq.

(1)

and

(2).

On

figure 5,

we show the

comparison

between the result of Nakaï et al.

[8]

and our result.

The intrinsic

quadrupole

moment can also be deduc- ed from the deformation parameters

32

and

{34.

Using

an axial

symetry

deformation as :

the

ground

state

quadrupole

moment can be written

as it follows :

with :

We used the

parameters P2

and

B4

obtained

by Raynal et

al.

[11] and by

Morand

[12]

to calculate

Qo.

On

figure 5,

are shown our results for radii ro = 1.2 and 1.4 fm.

Nakaï’s result is near the value

corresponding

to

ro = 1.4

fm,

and our result seems close to the value

corresponding

to ro = 1.2 fm.

In

conclusion,

our

experimental

results seems to

be a

tangible

link in

testing

a model between direct measurement on

quadrupole

moments and on mean

lifetimes. In

spite

of their small

difference,

the results in both methods with

regard

to their

precision

agree well

enough

in the framework of the rotational model.

(6)

References

[1] JONES

(K.

W.), SCHWARZSCHILD

(A. Z.),

WARBURTON

(E.

K.) and FossAN

(D. B.), Phys.

Rev.,

1969, 178,

1773.

[2]

DIAMOND

(R. M.),

STEPHENS

(F. S.),

KELLY

(W. H.)

and WARD

(D.), Phys.

Rev. Letters, 1969, 22, 546.

[3]

QUÉBERT

(J. L.), NAKAÏ

(K.),

DIAMOND

(R. M.)

and

STEPHENS (F.

S.),

Nucl.

Phys.,

1970, A 150, 68.

[4]

BEN ZVI

(I.),

GILAD

(P.),

GOLDBERG

(M.),

GOL-

DRING

(G.),

SCHWARZSCHILD

(A.),

SPRINZAK

(A.)

and VAGER

(Z.),

Nucl.

Phys., 1968,

A

121,

592.

[5] NAKAÏ

(K.),

STEPHENS

(F. S.)

and DIAMOND

(R. M.),

Nucl.

Phys., 1970,

A

150,

114.

[6]

ROSE

(M. E.),

GOERTZEL

(G. H.),

SPINRAD

(B. I.),

HARR

(J.),

STRONG

(P.), Phys.

Rev., 1951, 83, 79.

[7]

ESWARAN

(M. A.)

and BROUDE

(C.),

Can. J.

Phys., 1964, 42,

1311.

[8]

NAKAÏ

(K.),

WINTHER

(A.),

STEPHENS

(F. S.),

DIA-

MOND

(R. M.),

To be

published

and

private

com-

munication.

[9]

SCHWALM

(D.),

PovH

(B.), Phys.

Letters,

1969, 29B,

103.

[10]

DE BOER

(J.)

and EICHLER

(J.),

Advances in Nuclear

Physics,

Plenum Press, New

York, 1968,

1.

[11]

RAYNAL

(J.)

and DE SWINIARSKI

(R.), Colloque

sur

« Certains aspects

microscopiques

des réactions nucléaires » La

Toussuire,

1971.

[12]

MORAND

(B.), Thèse,

Université de

Bordeaux,

1971.

[13]

SKORKA

(J.),

HERTEL

(J.),

RETZ-SCHMIDT

(T. W.),

Nuclear

Data, 1966,

2, 347.

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