Submitted t0 <<Nuclcar Phvsics A»OCR Output
FOR DINUCLEAR SYSTEM
MASS PARAMETERS
G.G.Adamizm, N.V.Am0nenk0, R.V.J010s
PQGEIEEBEE
imtimxt» xtwm \
(i <·~-D Y? L@©3tt/7M) " "" V°` S`\ ’¤ Z3·b*>&`+
The paper is organized as follows. In sect. 2 we obtain the general form for OCR Output
the components of the mass tensor for a dinuclear system.
simpler way, we develop in this paper a simple and mainly analytical method to find
variables makes the computations very cumbersome. To obtain the results in a
evolution of the dinuclear system . However, its dependence on various dynamical
The nondiagonal component of inertia tensor plays an important role in the
production of light isotopes increases.
the stability of the dinuclear system for large mass asymmetry decreases and the
approaches to the radial potential barrier with the increase of ry. As a consequence,
of n—-mode transforms into the kinetic energy of the radial motion and system
Due to the coupling of R- and q— modes of motion the part of the kinetic energy
motion in the R — 1; plane increases significantly with increase of mass asymmetry.
it was shown that the nondiagonal component of the inertia tensor describing the
considerably influence dynamics of the dinuclear system. For instance, in refs. IL")
The values of mass parameters and their dependence on dynamical variables
given in refs. 13*5)
two-center basis. Inertia tensor obtained in terms of the adiabatic representation is
has been found in the framework of the linear response theory using quasi-adiabatic
·8) by exploiting the diabatic two-center shell model. In refs. 9*12) the inertia tensor
basis. The approach based on the dissipative diabatic dynamics has been realized in
refs. Z`4) the calculations have been done using adiabatic two-center shell model
cranking expression and perform calculations in different single particle basis. In
are different approaches to calculate its value. These approaches mainly use the
variables. The important ingredient of the Hamiltonian is an inertia tensor. There
Therefore, the Hamiltonian of dinuclear system should depend on these dynamical
of nuclei, A = A1 + A2) and a neck radius or other characteristic of a neck *6).
mass asymmetry degree of freedom ry = (A1 - A2)/A (A1 and A2 are mass numbers
interaction of two nuclei are the distance between the centers of colliding nuclei R,
OCR OutputThe most important degrees of freedom which are necessary to describe the
T = — 7) ( OCR Outputn’ ( 6 ) 1 ( 6 ) —— d V ———-—V —— . 2m/ r p(r)6p(r) n(r) p(r)6¤(r)nian in terms of the functional derivatives of p
Using eqs. (4)—(6) we can represent the kinetic energy part T of the total Hamilto
6 ( )ih 6 · = —V ——- . J(¤‘) m (Mr) Mw)and the current operator has the following functional representation
(5)_ , , lp(r),J(r )] = —:V-(6(r — r )p(r))ih
erations. Operators p andj satisfy the commutation relation 16)
The omitted term depends only on p and is not necessary for the following consid
(4). _ . H = d¤·1(r)p ‘(r)J(r) +m 5 /
operators as given below:
(3)p(r) = ¢»"`(r)·/»(r)
and density
(2), J(¤·) = —¢“'(r)V=1»(r) — V1/»"(r)¤/¤(r)zh % (
where 1/:+, xl) are nucleon field operators, can be expressed in terms of current
I I I I H = dr V1/)+(r)V1/¤(r) + I drdr ¢+(r)·¢~(r)u(r — r)1,b+(r )1/»(r ), (1)he E/
two-body forces
It can be shown 16*17) that the nuclear Hamiltonian of the general type with the
2. Inertia tensor
are presented in sect. 4.
parameters both macroscopically and microscopically. The results of calculations
is introduced. The simple analytical expressions are obtained to calculate mass
inertia tensor and discuss some useful relations. ln sect. 3 the definition of neck
n 0
(12d) OCR Output= é§(E0 — En) < n|qj|0 >< 0]qj»|n >,
= —- 2 12 ( °)n§, @,1 — Eq2 <¤|lH,<1il10 >< 0llH7<1i·lI¤>
(12b)(B`1)u· = < 0|l<1w» [H»<1illl0 >
If the nucle0n—nucleon forces are velocity independent then
(12**)(B`1))1’ Z ij < 0lZVk91(rk)Vk9j·(Fk)l0 >
we can rewrite the formula (11) in the following way:
kzi
p(r) =< Ol Z 6(r— r;,)|0 >,/$1+/$2
Using the density of the dinuclear system
(11)_ (B ‘)n = drx»(r)Vy)(r)Vyj·(r)i E/
It is evident from (10) that the components of inverse inertia tensor are:
. 2 8q],10 ( )E -——» 12-. )J]
nz 8 0 1
@(11*Z —·; ·— l` l` ‘ l' ‘» l` T 2d<>v<>v<> p g] gi/2m 1,r 3%
(*6
we obtain the kinetic energy term as:
g ( ’.L. : . UL 6»<r> ;”’( Ge
functional derivative as given below
where gj(r) are functions required to derive qj. Then, with the expression for the
(8)qi = / <1¤¤(r)y)(r)~
some number of collective variables q_, which are donned by the relations
collective motion of two—center system. We assume that the density p depends on
ln what follows, we shall use the expression (7) to derive the inertia tensor for the
Z R" (B"l·m(B")¤R · l(B`1lRnl2(17c) OCR Output
(B_1lRn
, im (B-l)vn(B—1lRR " l(B_1lRnl2(17b)(B")nR B = --———;—
: “" <B-l>m,<B-wm — 113-%,12(Bl-1)*77I
then, all the components of inertia tensor are:
centers R and mass asymmetry parameter 7; are taken as the collective variables,
(B "l)j_,I and vice versa. For example, if the relative distance between the fragment
From eq. (16) we can express matrix elements Bj,] in terms of matrix elements
which is satisfied identically because of (14).
J1J2
BM = Z BmBm·(B`1)mz
relation
ing expression (15), we insert (13) into (15) and, using (12c), obtain the following
To demonstrate the equivalence of the inertia tensor in (11,12) and the crank
using the two-center shell model basis.
MBa = 2v 2 en 0 ' ··
<n6 6`q·0><08 8q··n> 4€’ J'
Usually, the inertia tensor Bjy is calculated with the help of cranking expression
" jj'
T Z Bjwijsiy
we can obtain from (10) the well known expression for the collective kinetic energy
(14)Bm(B")j.i· = 6m
and
jr8 F Fqj ji (13)I _ 'ZBjJ’lH=qi'l = ·{2Bn·<1r8 1
corresponding energies Eg and En. Since
where |0 > and ln > are the ground and excited states of the dinuclear-system with
A= dr p(r)0(:l;z). (19a) OCR OutputU) f2
Fragment mass numbers are defined by the relation as given below:
18 ( ¢)€(z) 9(—z)= ———- — -—~—— . yn Z ( A1 A2
follows that:
is the point where the densities of nuclei are equal to each other. From (18a) it
Here z is the axis connecting fragment centers and 6 is the step function. The z = 0
(18b)gn = ·}(6'(z} ·- 9(-z))
= —- ——-—· 18dgg 6(z) G(—z)
for gg and gn defined by the equations:
ments we get the usual definitions of R and r; if we substitute in (8) the expressions
fragment centers and the mass asymmetry parameter 17. For well separated frag
Let us firstly consider as collective variables the relative distance R between the
3. Macroscopic and microscopic considerations
(B`l)iz,, < (B`l)»¤(B`1lnR
BIQU < B,,,,BRR,
lB·mBm¤¤— B}anll(B")m(B")Rn · (3**)%,,] = L
BRn(B_1)Rn 'i` BnnlB_1)vm : BR·r1(B-1)}%: + BRR(B_1)RR : lv
1} B2.: BHRBW — = BRRBM —B
n M -1 = —B -;-1 = ——-—-——— B , "" "“<B·1>Tm \/(B`llRR(B`1lnn( )“"BRRB(B-1)R
Bnn(B—l)nn = BRH(B—1)RR¤
The solution of eq. (16) as given by eqs. (17), leads to the following useful relations:
r r ,, B w ———-—-—, B x ~———, B z ——-——+———. “*‘<B-wm "" <B-¤>.. "" <B-1>..<B-wm(B`*)R
For (B“l)R,, to be small, above components (17) can be expressed as:
`1 = -———————— d —— 22 <B hm 1 rp<»>¢xp<¤>1 A A zz mmz (MM2] ( OCR OutputTaking into account (20), the approximate value of eq. (21) is
nuclei.
separated fragments we obtain a reduced mass lt : mAlA2[A for two interacting
that BE}; decreases as the overlapping of interacting nuclei increases. For the well
Since (0(;l:z) — 02(;hz)) and 0(z)0(—z) are always positive, it is obvious from (21)
_ _ — _ 0(z) — 02(z) 0(—z) — 02(—z) 0(z)0(—z)
B-] = ———- -—-—- ( )RR mA] + THA;l l
Substituting (18a,b) with 0 instead of 0 into (11) and using (19b) we obtain
A= dr p(r)0(;l;z).v) f2
norm of 0 is defined as in eq. (19a)
interval a amounts to the diffusion of nucleon density distribution in nucleus. The
(Function 0 is schematically depicted in Hg.1.). ln the limit a —> O, 0 —> 0. Physically
where a is the small interval over which the value of 0 jumps from zero to one.
(20)— 1 z 0(Z) Z - (1 + err 2 a
nuclei. This function 0 is defined in the following way
into account the mutual interpenetration of nucleons belonging to the overlapping
We generalize the definitions (18a,b) by introducing a function 0 instead of 0 to take
0.5 tion 0(z).
Fig.1. Schematic form of the func
I.O
1!(z)
we are interested in the description of the dinuclear system in the noncquilibrium OCR Output
can find A,,,ck and, therefore, the components of mass tensor microscopically. Since
the results of microscopic calculations for the nucleon occupation numbers 18) we
Substituting in (23) an expression for p in the second quantized form and using
V BRRBUU W 7V AIAZ " AAncck/4.BRUI I \/5 AAneck
· ccBA U = -——-—, ( )R TTL \/7FbA]Ag1 Ank
( A)B-] uu : —-`_`°—_» ( l m \/§b2A21 Aneck
In the same way as above we obtain
(24)v : A,,,ck/A.
in the system A:
the ratio of the number of particles in the neck Auger to the total number of particles
lt is convenient to introduce a degree of freedom ·u connected with the neck as
the mass asymmetry parameter 1; increases.
BR,, is very small for almost symmetric configurations but increases significantly if
Here A; 2 A2. As it is seen from (22c,d) the nondiagonal component of inertia tensor Y
BRRBW ,/(B—¤)RR(3—¤)W V N/27r A(AiA2 ~ A/har/4)L Ancck (A1 _ A2) (.).7d)lBRnl Z l(B_l)Rnl Z
and
(B·)Hn I -...m 2\/Fb AAIA2 (22c)1 A A — A 1i5’iLJ
22b ( )*
B·: -;; ( )YV’7 /27rb2A2
VVe obtain the other components of inverse inertia tensor as
Amr =<1rr>(r<¢x1>— (23):2 /)(§>in the neck between two fragments Amckt
The integral which appears in (22a) can be interpreted as the number of particles
where bz = vraz /4 which demonstrates that values of b and a are close.
matrix elements in (27) can be obtained analytically. For the frequency parameter OCR Output
particle wave functions of harmonic oscillator in the cylindrical representation, the
are calculated exploiting the expressions (17), (22), (25) and (27). Using the single
”Ni+5sNi—>“°Ba and “8Pd+“8Pd—>°3°U. The components of the inertia tensor
To illustrate the results of the previous sections we have considered the systems
4. Results of calculations
variables.
to elucidate the values of mass parameters and its dependences on the collective
of the elements of inertia tensor. However, the obtained results give possibility
(22), (25) and (27) in numerical calculations allows us to obtain the smoothed parts
rectly the cranking expression to determine the inertia tensor. Thus, use of (17),
definitions of Amd,. In the consistent microscopical calculation we should use di
only partly taken into account. This influence manifests through the microscopical
tensor the influence of the interacting nuclei shell structure on the value of Bjy is
Because of the approximations used to derive the components of inverse inertia
(26)Ama = E mcdr exp —|<.¤k(r)l2Z2 /(§) ke1,2where ni, are the Fermi occupation numbers. Ultimately, eq. (23) becomes:
km,2
< 0|p(r)l0 >= Z ¤»l<x¤k(r)|’»
neglecting their contribution we obtain from (26)
Assuming the chaoticity of the phases of the nondiagonal matrix elements of p and
§(<pI(r)s¤¤(r)¤¥¤¤ + M-)2,2’1,\’
n(r) = X =»¤I(r)s¤¤·(r)¤T¤¤· + Z s¤;(r)w(r)¤£`¤¤·
overlapping of the colliding nuclei, p can be written as
nuclei i.e. projectile (gal) and target (cp;). Thus, taking into account the small
stage we shall use a.s a, basis the single particle wave functions of the noninteracting
( I , , .8.0 0.2 0.4 0.6 0.8 1.0` {
$ \ "—_ i `\\ \
aol- ‘ \
~»,1g_g for the system “8Pd+u8Pd. OCR Output
Fig.3. The same as in fig. 2, but5 F Ai"
15.0 F XH
20.0 RA H8Pd+’18Pd system
0.0 0.2 · 0.4 0.6 0.8 1.00.0
N ‘· `\ .` \ " 3 dashed lines, respectively.\ __ _ \`\.1 by solid, short dashed and long
ELOF \ \ at d = -1,0,2 fm are presented
8Ni+58Ni. The calculated resultsR
R1 + R2 + d for the system10.0 t `~_ `
ues of fragment separations R =
mass asymmetry ry at various val
. l5·O E R NH, N1 System Q Fig.2. Dependence of Ama;. on55 . 5.5
of nuclei in contact.
of AMC;. are larger at smaller R i.e. Amd. is proportional to the overlapping volume
It is seen that the nucleon number in neck decreases with increasing ry. The values
1.15/I}? fm are the nuclear radii and d = -1, 0, 2 fm) are presented in figs. 2 and 3.
fm in our calculations. The dependences of AMC;. on n at R = R1 + R; + d (HL2 =
O.7)`1 fm'2 which reproduces the systematics of nuclear radii. We have used b = 0.8
of the harmonic oscillator wave functions we have taken the value *9) v = (0.9/11/ 3 +
I I OCR Output
nuclear shell structure. The values of Bm, and BW increase with increasing 1]. In the
of mass parameters which are seen in figs. 4 and 5 are the consequences of the
fragment separation R are presented in figs. 4 and 5. The oscillations of the values
The mass parameters Bjj. calculated as functions of 1] for various values of the
Fig.5. The same as in fig. 4, but for the system u8Pci+“8Pd.
°‘g.o 0.2 0.4 0.6 0.8 1.0
¤¤ 10.0
E 20.0ifA’ r
I / ,·: :0.0 3* 1
5_ 8.0 0.2 0.4 0.6 0.8 1.00.00
[D -2100.20
E »E -21.0\%E0.40 xx ___·* T. O E _/' `¤,\
"--"\*\C —I9.0
/\ YX0.60 \ é
_] * ` _' —»»` v~
0.00.0
.... .---..--,..--·"{/fi - 4 ‘’
s.¤E /·” x} / [ '2.0/_ 1 4, / ’ [
/ I, ' / I$10.0
I :4.0E 15.0
{*20.0
6.0
E 25.0
8.0OCR Output30.0
I3 OCR Output
yield of light particles in fusion-type reactions observed in the experiments 2°·21·“).
The coupling between R- and 7;- modes of motion can be the reason of the enhanced
and the nondiagonal components of the inertia tensor should be taken into account.
condition BR, < \/BRRB,,,, is not correct for strongly asymmetric dinuclear systems
7] ——» 1. This behavior of BR,, is in agreement with the results of refs. ’3·“‘). The
significantly with increasing mass asymmetry 1] and can approach to 0.4 in the limit
motion vanishes. However, the value of the ratio Bm,/\/BRRBM (figs.6,7) increases
For the symmetric configurations the coupling between R- and ry- modes of
0.0 0.2 0.4 0.6 0.8 1.00.0
0.1
0.2E "———/"“
0.:E "`··"""'N
"all
0.4
for the system “°Pd+“8Pd.
up Fig.7. The same as in fig. 6, but
xt //
{IIE [*,/4* / 4l,»· f_A- ’»’ /
0.2" ’
» Im0.3
0.4
"°Pd+`1°Pd system0.5
formation is necessary to investigate the dinuclear system transition to mononucleus.
OCR Outputfor the description of the nuclear fusion process because the consideration of the neck
14 OCR Output
2 (North—Holland, Amsterdam, 1980)
J. Maruhn, W. Scheid and W. Greiner, in Heavy ion collisions, ed. R. Bock, vol.
O. Zohni, J. Maruhn, W. Scheid and W. Greiner, Z. Phys. A275 (1975) 235
H.J. Fink, J. Maruhn, W. Scheid and W. Greiner, Z. Phys. A268 (1974) 321
Wong, Rev. Mod. Phys. 44 (1972) 320
M. Brack, J. Damgaard, A.S. Jensen, H.C. Pauli, V.M. Strutinsky and C.Y.
References
2-61—13—28
This work was supported partly by the Russia Ministry of Education under Grant
We are grateful to Dr.R.P.Malik for discussions and reading of the manuscript.
useful in the consideration of nuclear fusion process.
the condition Bm, < \/BRRBW, is justified 4). The results of this paper can be
of the strongly asymmetric systems. However, for almost symmetric configurations
account the nondiagonal matrix elements of the inertia tensor to consider dynamics
increases strongly if mass asymmetry increases. Thus, it is important to take into
R- and 1]- modes of motion is small for almost symmetric configurations but it
clusion of refs. 21*22) that the nondiagonal component of inertia tensor connecting
on the nuclear Hamiltonian of a general form. The results obtained confirm the con
in the dissipative heavy ion collisions, have been obtained. The derivation is based
and nondiagonal components of inertia tensor, describing a dinuclear system formed
On the basis of approach suggested above the general expressions for the diagonal
5. Summary
evolution of asymmetric dinuclear system.
well (figs.6,7). S0, all components of inertia tensor are necessary to describe the
The role of the coupling between R- and v—modes of motion is considerable as
I5 OCR Output
1988) p.216
Conference on Clustering Aspects in Nuclear and Subnuclcar Systems (Kyoto,
V.L.Mikheev, J.Szmiger and V.V.Volkov, Contributed Papers of International
A.N.Mezentsev, A.G.Artul»;h, G.F.Gridnev, W.Karcz, S.Kliczewski, M.Madeja,20)
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10) P..I. Johansen, P.J. Siemens, A.S. Jensen and H. Hofmann, Nucl. Phys. A288
H. Hofmann and P.J. Siemens, Nucl. Phys. A257 (1976) 165
A. Lukasiak and W. Niirenberg, Z. Phys. A326 (1987) 79
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Bromley, v01. 2 (Plenum, New York, 1984)
W.U. Schréder and J.R. Huizcnga, in Treatise on heavy-ion science, ed. D.A.
W.J. Swiatccki, Progr. Part. Nucl. Phys. 4 (1980) 383
I6 OCR Output
on August 31, 1993.Received by Publishing Department
Kaplan, M.S. Zisman and E. Duek, Phys. Rev. C22 (1980) 1080
24) D. Logan, H. Delagrange, M.F. Rivet, M. Rajagopalan, J.M. Alexander, M.
N.V. Antonenko and R.V. Jolos, Z. Phys. A341 (1992) 45923)
N.V. Antonenko and R.V. Jolos, Z. Phys. A339 (1991) 45322)
1991) p.39
1991, ed. E.Gadi0li (Ricerca Scientifica ed Educazione Permanente, Milano,
V.V.V01k0v, Proc. 6th Int. Conf. on Nuclear Reaction Mechanisms, Varenna,21)
Preprint of the Joint Institute for Nuclear Research. Dubna, 1993 OCR Output
Physics, JINR.The investigation has been performed at the Laboratory of Theoretical
asymmetry increases.
is weak for almost symmetric configuration but it enhances significantly as theproposed. It is shown that the coupling of the radial and mass asymmetry modesis analyzed. The definition of a neck parameter for the dinuclear system isdifferent modes of motion for various configurations and fragment separationscomponents of the inertia tensor for a dinuclear system. The coupling between
A microscopical method is proposed to derive the diagonal and nondiagonal
Mass Parameters for Dinuclear SystemAdamian G.G., Antonenko N.V., Jolos R.V.
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