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Submitted on 1 Jan 1977

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Two-nucleon stripping process with effective interactions

M. Ismail

To cite this version:

M. Ismail. Two-nucleon stripping process with effective interactions. Journal de Physique, 1977, 38

(8), pp.897-903. �10.1051/jphys:01977003808089700�. �jpa-00208656�

(2)

TWO-NUCLEON STRIPPING PROCESS

WITH EFFECTIVE INTERACTIONS

M. ISMAIL

(*)

Faculty

of

Science,

Cairo

University, Egypt

(Reçu

le 15 décembre

1976,

révisé le 14 mars

1977, accepté

le 29 avril

1977)

Résumé. 2014 On étudie le facteur de forme du processus d’arrachement

(stripping)

de deux nucléons

4oCa(t, p)42Ca

en utilisant deux types d’interactions effectives, celles de

Skyrme

et de Brink-Boeker.

On compare les résultats avec ceux obtenus avec le

potentiel

habituel de portée nulle. On trouve que

l’emploi

des interactions effectives réduit l’importance de la région nucléaire interne. De

plus

les

facteurs de forme calculés avec ces interactions effectives diffèrent du facteur de forme obtenu pour

une portée nulle à la fois dans la

région

de surface et dans la région

asymptotique.

Abstract. 2014 The form factor of the two-nucleon

stripping

process

40Ca(t, p)42Ca

is studied

using

two types of effective interactions, namely the Skyrme and Brink-Boeker interactions. The results are compared with those of the

ordinary

zero-range

potential.

It is found that the effective interactions reduce the

importance

of the nuclear internal region. In addition the form factors calculated with effective interactions differ from the zero-range form factor in both the surface and asymptotic

regions.

Classification

Physics Abstracts

25.50

1. Introduction. -

Steady

progress has been made in recent years towards a

microscopic understanding

of nuclear

reactions,

that is to say, a

description

in

terms of detailed nuclear wave functions and an effec- tive interaction between nucleons which has some

realistic basis

[1].

The two-nucleon transfer reactions have taken on great

importance,

since

Glendenning [2]

has shown these reactions to be very sensitive to

spectroscopy.

The DWBA is a useful method for

describing

the two-nucleon transfer process. For definiteness we consider the reaction

A(t, p)B.

The DW

calculation for this reaction consists of two inde-

pendent

parts. The first part

depends

on the

overlap

of initial and final nuclear states and the effective interaction between the

outgoing proton

and the two

captured

neutrons, referred to as the form factor. The

second part of the calculation is standard and can be carried out with well known computer programs.

In references

[3]

and

[4],

the effects of

configuration mixing

and the choice of

single particle

wave functions

on the two-nucleon

stripping

form factor were studied

in zero range DWBA. The present work studies the effect of effective interactions on the two-nucleon transfer form factor. For this purpose the reaction

40ca(t., p)42Ca(g.s.)

at an incident triton energy of 12 MeV is considered. The

12 Ca

nucleus is taken to consist of two neutrons in a 1

f7/2

level

plus

the

4°Ca

closed shell. The

stripping

form factor is calculated

using

two

types

of effective nucleon-nucleon interac-

tions, namely

the Brink-Boeker

[5]

and

Skyrme [6]

interactions.

2. The two-nucleon

stripping

form factor with

Skyrme potential.

- The two-nucleon

stripping

transition

amplitude

for the reaction

A(t, p)B

may be written in DWBA as

The ’1’(-) and ’1’(+) are the usual distorted waves while the cp functions describe the internal functions of the

particles

involved. Xp is the

spin

wave function of the

outgoing

proton.

(*) Present address : Science & Mathematics Centre, P.O. Box 4577, Riyadh, Kingdom of Saudi Arabia.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01977003808089700

(3)

898

Using

the classical

decomposition

of

QJ JBMB(ÇA"

rl,

r2)

one gets

If the

interacting potentials

are

spin independent,

the differential cross-section may be

given by

where

The coordinates are defined in

figure

1. We now evaluate

integral (4) by making

three

hypotheses.

2.1 The incident triton is assumed to be in a pure S-state. This is not a crude

approximation

since it is known that the

ground

state of a triton is at least 94

%

S-wave

[7].

The internal wave function of the triton is chosen as a Gaussian

where

2.2 The interaction

potential V;p

is taken as a

density-dependent

effective interaction of the

Skyrme

type

[6],

and the sum of the two

potentials (V1p

+

V2p)

is

approximated by

where the

operators V2

and

V2

act on the left and on the

right

of the matrix element.

p(R )

is the

density

of the

residual nucleus.

2.3 The

transferred-particle

wave functions are assumed to be those of harmonic oscillators. The Talmi-

Moshimsky

transformation

gives

the result

[8]

We use the

Taylor expansion

of the wave functions

and

(4)

to get

Substituting

eq.

(5), (6), (7)

and

(8)

into eq.

(4)

and

setting Q

=

cxvf - ’ 3 Vr

we obtain

The operators

V2n

and

V>2n

now act on the functions

e1J.Q

and

e-4"õ,,2 respectively,

and their values can be

easily

obtained. The double

integration

over

r and n

can be

performed

and its value is

where

Green’s theorem

implies that, if O2

is the

Laplacian acting

on

pl+),

we can

replace

the

operator Q 2

in eq.

(10) by

Use of the

Schrodinger equation

allows each operator to be

replaced by

its

eigenvalue

where

mi*

denotes the reduced mass of the

particle

i.

Substituting

for the

eigenvalue

of

Q 2

from eq.

(11)

one gets the

following expression

for

I L

where

The factor

Fn (Rt)

is

complex

because of the existence of

optical-model potentials

in both

kf

and

kf .

The real

part

of Fn (Rt)

goes to a constant value when the real

potentials

in

equation (13)

become zero. The

imaginary

part of

Fn (Rt)

is determined

directly by

the

optical-model imaginary potentials

of the incident triton and the

outgoing

proton. For the

ordinary

zero range

potential, Vo d(n).,

the factor

Fn(Rt)

tends to a real and constant

value,

(5)

900

The two-nucleon

stripping

form factor

corresponding

to the

Skyrme potential

is

given by

where

QNL(Rt) is

the radial part of the wave function

describing

the center of mass motion of the two

captured

neutrons. For the

ordinary

zero range

potential

the two-nucleon

stripping

form factor is

given by

3. The two-nucleon

stripping

form factor with the Brink-Boeker

potential.

- The

finite-range

effective

interaction of the Brink Boeker type may be written as

where the first term is attractive while the second is

repulsive [5].

Let us consider first the attractive term

only.

In terms of the coordinate vectors

r and n) (defined

in

figure 1),

Eq. ( 17)

can be written as

Substituting

eq.

(5), (7), (8)

and

(18)

into eq.

(4),

one gets

where

If one

expands

the

plane

waves

on a

spherical

harmonic basis and assumes that A = p =

0,

the double

integral

over

r and q

can be

performed

and eq.

(19)

reduces to

where

(6)

As in the

preceding

section we

replace

the operator

Q 2 by

and the value of

can be found

by using

the LEA. This

approximation simply replaces

each

Laplacian by

its

eigenvalue

obtained

from eq.

(11).

The

repulsive

term of the Brink-Boeker

potential gives

a factor

FBR(Rr)

which is

exactly

the same as that

given by

eq.

(21 ) except

that

V 1 and P

are

replaced by Y2 and B’ respectively.

The two-nucleon

stripping

form

factor

corresponding

to the Brink-Boeker

potential

is

given by

where

4. Numerical calculations. - In order to show how the effective interactions affect the radial form factor of the two-nucleon

stripping

process, the reaction

40Ca(t, p)42Ca(g.s.)

at an incident triton energy of 12 MeV was considered. The factor

Fn(R)

was cal-

culated for this reaction

using

the Brink-Boeker and

Skyrme

effective

interactiQns

and the results are

represented

on

figures

2 and 3.

The difference in

shape

between form factors calculated

using

zero range and effective interactions

can be seen from

figure 4,

which shows the real

parts

of the form factors for both the

Skyrme

and the

Brink-Boeker

potentials together

with the zero range form factor. In each case the form factor is obtained

by multiplying

the factor

Fn.(Rt,) by

the wave func-

tion TNL as indicated

by

eq.

(14), (15)

and

(22).

The

three form factors shown on

figure

4 are calculated

for the case J = L = 0 and N = 4.

FIG. 2. - The real part of F1(Rt) calculated using Skyrme and

Brink-Boeker effective potentials. They are multiplied by the factors 1.50 x 10-3 and 3.23 x 10-3 respectively. - - - - Skyrme; 20132013

Brink-Boeker.

FIG. 3. - The imaginary part of F1(Rt) calculated using Skyrme

and Brink-Boeker potentials. - - - - Skyrme; - Brink-Boeker.

The size

parameter "0

of the triton wave function

was chosen such that the rms radius of the triton is 1.68 fm. The oscillator

parameter

v was defined so that the

single

nucleon wave functions are propor- tional to

This

parameter

is

typically

about

A - 113

fm -

2,

which

corresponds

to an oscillator

spacing

nw = 41 A -1/3 MeV.

The

density p(R )

was assumed to be

(9)

(7)

902

FIG. 4. - Plot of the real parts of the two-nucleon stripping form

factors obtained from Skyrme, Brink-Boeker and zero range inter- actions. All three curves are normalised at the point R = 4.5 fm.

zero range ; - - - - Skyrme; + + + + Brink-Boeker.

where po =

0. 172 fm - ’, a

=

0.55fmandro

= 1.12 fm.

The

optical-model

parameters were taken from refe

rence

[10].

The values

of to, t, and t2

were taken as

[6]

to

= 3 298

MeV . fm3 ,

t 1 = - 59

MeV . fm5

and

The wave function

TNL(2

v,

Rt)

was

replaced by

the

spherical

Hankel function

(- i)L hi1)(ikR)

at a radius

where the

following equality

holds

where

EB is the

separation

energy of the

pair

from the nucleus and M* is the reduced nucleon mass.

5. Discussion. - For the

ordinary

zero range

approximation

the factor

F,(,z-’-)

is real and does not

depend

on

Rt.

Thus the zero range two-nucleon

stripping

form factor is

proportional

to the wave

function

TNL(Rt).

The

Skyrme potential

results in a

complex

factor

F:(Rt)

whose

imaginary

part is due to

the presence of the

V2

term in the

potential.

This

imaginary

part is small

(about

2.3

%

of the real part

at

Rt

= 4.5

fm)

because the

V2 coefficient,

t1., is small

compared

with the values of the other two coefficients to and t2. The real part of

Fs(R,)

reduces the

impor-

tance of the nuclear interior

by

about 54

%

as shown in

figure

2. This is because the effective nucleon-nucleon interaction is small in the inner

region

and increases as

the

density p(R )

decreases. The

increasing

behaviour

of

Fn (Rt) beyond

the nuclear surface

yields

a form

factor which falls off less

rapidly

in the

asymptotic region

than the zero range form factor

does,

as is

shown in

figure

4. Iano and Pinkston

[3]

found that

slight

differences in form factors in the

region

from

4-7 fm have

important

effects on both the

shapes

and

the

magnitudes

of the differential cross sections. Thus

we expect that the small difference between the

Skyrme

and the zero range form

factors,

shown in

figure 4, yields significant

effects on the two-nucleon

stripping

differential cross-section.

The Brink-Boeker

potential gives

a form factor which differs from that of the

Skyrme

interaction in both the

asymptotic

and inner

regions.

It falls off less

rapidly beyond

the nuclear surface and

yields

less

reduction in the

importance

of the inner

region compared

with the form factor

resulting

from the

Skyrme potential. Moreover,

the

imaginary

part of

FnBB(R )

is

large (about

75

%

of the real part at R = 4.5

fm)

and

peaks

at about 5 fm. This

imaginary

part increases the contribution of the surface

region

to the cross-section.

The value of the two-nucleon

stripping

cross-section

depends

on both the value and the

shape

of the form factor in the

region

from 4-7 fm. The greater the extension of the form factor in the

asymptotic region,

the

larger

the differential cross-section

[3].

The inner

region

has a small effect on the cross-section because

nonlocality

effects and the

absorption parts

of the

optical-model potentials strongly

reduce the contri- butions to the cross-section from this

region.

In the

present work it was found that the form factors calculated with effective interactions extend farther in the

asymptotic region

than the zero range form factor.

Ibarra

[11]

found that if the nuclear

overlap

which

enters in two

particle

transfer DWBA

theory

is

calculated

using

a realistic

method,

the zero range form factor will increase in the surface

region by

about 43

%.

Thus if we use a realistic nuclear

overlap together

with

an effective

interaction,

we will get a form factor which differs from the zero range form factor in both the surface and the

asymptotic regions.

Iano and Pinkston

[3]

have used a Gaussian

potential

to calculate the form factor

assuming [12]

where

(8)

They

found that the calculated cross-section is smaller than the

experimental

data

by

a factor of 14.6.

In the present work we found that the average value of

is about 1.9 Moreover the average value

of I F,,s(R,) I2

is about 4.8 times that of the Brink-Boeker

potential.

Thus the

Skyrme

interaction

predicts

an absolute value for the two-nucleon

stripping

cross-section which is 0.63 times that found

experimentally.

This factor will increase if one introduces a realistic nuclear

overlap together

with the

Skyrme

interaction.

References

[1] LovE, W. G. and SATCHLER, G. R., Nucl. Phys. A 159 (1970) 1.

ISMAIL, M., J. Physique 34 (1973) 369.

[2] GLENDENNING, N. K., Phys. Rev. B 137 (1965) 102.

[3] IANO, P. J. and PINKSTON, W. T., Nucl. Phys. A 237 (1975) 189.

[4] DRISKO, R. M. and RIJBICKI, F., Phys. Rev. Lett. 16 (1966) 275.

[5] BRINK, D. M. and BOEKER, E.,Nucl. Phys. A 91 (1967) 1.

[6] VAUTHERIN, D. and BRINK, D. M., Phys. Rev. C 5 (1972) 626.

[7] PASCUAL, R., Phys. Lett. 19 (1965) 221.

[8] MOSHINSKY, M., Nucl. Phys. 13 (1959) 104.

[9] DE S’HALIT, A. and FESHBACH, H., Theoretical Nuclear Physics

Vol. 1 (John Wiley and Sons) 1974.

[10] BAYMAN, B. F. and HINTZ, N. M., Phys. Rev. 172 (1968) 1113.

[11] IBARRA, R. H., Nucl. Phys. A 211 (1973) 317.

[12] LIN, C. L. and YOSHIDA, S., Prog. Theor. Phys. 36 (1966) 251.

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