Description of the mass-asymmetric fission of the Pt isotopes, obtained in the reaction {}^{36}Ar + {}^{142}Nd within the two-stage fusion-fission model

# Description of the mass-asymmetric fission of the Pt isotopes, obtained in the reaction 36Ar + 142Nd within the two-stage fusion-fission model

V. L. Litnevsky Omsk state transport university, Omsk, Russia    F. A. Ivanyuk Institute for Nuclear Research, Kiev, Ukraine    G. I. Kosenko Omsk Tank Automotive Engineering Institute, Omsk, Russia    S. Chiba Tokyo Institute of Technology, Tokyo, Japan
today
###### Abstract

The two stages dynamical stochastic model developed earlier for description of fusion-fission reactions is applied to the calculation of mass- and energy-distributions of fission fragments of platinum isotopes in reaction . The first stage of this model is the calculation of the approaching of projectile nucleus to the target nucleus. On the second stage of the model, the evolution of the system formed after the touching of the projectile and target nuclei is considered. The evolution of the system on both stages is described by three-dimensional Langevin equations for the shape parameters of the system. The mutual orientation of the colliding ions and tunneling through the Coulomb barrier in the entrance channel are also taken into account. The potential energy of the system is calculated within the macroscopic-microscopic approach. The calculated mass-energy distributions of fission fragments are compared with the available experimental data. The impact of shell effects, rotation of the system and neutron evaporation on the calculated results is discussed.

fusion-fission
###### pacs:
25.70.Jj,24.10.-i,21.60.Cs

## I Introduction

The first theoretical description of nuclear fission discovered in 1939 Gan:39 (); meitner () was given in the framework of the liquid drop model Bohr:39 (), in which it is assumed that the properties of the atomic nucleus are similar to those of a charged viscous incompressible liquid drop. It turned out that the liquid drop model predicts splitting of fissioning nucleus into two fragments with the same masses, what was confirmed by experiments of highly excited nuclei. However, in the case of low excitation energies, such as the fission of U by thermal neutrons, the masses of the fission fragments were not equal. The explanation of mass-asymmetric fission was given later by the influence of shell effects. The presence of mass-asymmetric fission valley for transuranium elements was demonstrated by Pashkevich in Pashkevich:71 (). In this work the dependence of the potential energy of nuclei on their deformation was constructed using the shell correction method of Strutinsky Strutinsky:67 (); Brack:72 () and it was shown that the fission process is strongly affected by the deformation dependence of the potential energy of the system. Further progress in the description of the process of nuclear fission is associated with the use of statistical Fong:69 (); mebel:92 () and dynamical Adeev:89 (); usang2019 () models, as well as their combinations Mavlitov:92 (). These models describe the fission of a nucleus initially located in a potential well near the ground state (compound nucleus). Such an excited compound nucleus can be formed by irradiating of atomic nuclei by light particles.

The description of the fission process becomes much more complicated if the excited nucleus was formed in the result of fusion reaction of two massive ions. In this case, one can’t talk merely about the fission of compound nucleus. From the moment of touching of the initial nuclei to the moment of formation of the compound nucleus passes quite a long time, during which the system may undergo fission or may reduce its excitation energy by emitting a light particle or gamma quanta and form the compound nucleus in the ground state. As the result, for the description the mass distribution of fission fragments it is necessary to consider the whole evolution of fusion-fission process starting from the approaching of the initial nuclei to each other and ending with the formation of compound nucleus or fission.

For this purpose in GI:02 (); Litnevsky:14_1 (); Litnevsky:14_2 () the so called two-stage dynamic stochastic model for description of fusion-fission reaction with heavy ions was developed. In this model on the first stage of calculations the approaching of projectile nucleus to the target nucleus up to their touching point is considered. On the second stage we study the evolution of compact system, formed after merging of colliding nuclei.

In present work we apply the two-stage model GI:02 (); Litnevsky:14_1 (); Litnevsky:14_2 () for the description of the kinetic energy and mass distributions of the fission fragments obtained in recent publication Andreev:18 () for the reaction at beam energy and MeV. This publication contains experimental data on the energy- and mass-distributions of fission fragments, average energy taken away by the pre-fission neutrons, average induced angular momentum and the rotational energy. Comparison of such data with calculated results would be a good test for the theoretical models.

## Ii The two-stage approach

For the calculation of fusion-fission reaction with heavy ions we use the two-stage dynamic stochastic model GI:02 (); Litnevsky:14_1 (); Litnevsky:14_2 (). As it was mentioned above, on first stage of calculations we consider the approaching of projectile nucleus to the target nucleus up to their touching point. On the second stage we study the evolution of compact system, formed after merging of colliding nuclei. The schematic comparison of the potential energy in fusion and fission channels is shown in Fig. 1. The final point of the second stage calculations could be the splitting of the system back into two fragments or formation the evaporation residue , where is a number of neutrons, evaporated by the compound system in order to reduce its excitation energy. Of course, the outcome depends on the reaction energy.

The evolution of both separated ions and compact system is described by Langevin equations for the collective parameters that fix the shape of the system. For the approaching process the collective parameters are the parameters and of quadrupole deformation for both ions and the distance between their centers of mass. On the approaching stage we also take into account the orientation of target nucleus – the angle between the symmetry axis of the deformed in the ground state target nucleus and the line connecting centres of mass of colliding nuclei. The shape of the compact system is described by the parameters , and of Cassini parameterization Pashkevich:71 () that specify the total elongation, the mass asymmetry and neck radius of the system.

At the end of the first stage calculations (at the touching point) we fix the center-of-mass distance, the potential and internal (dissipated) energy of the system. At the initial point of the second stage calculations we use this data to define the shape of the system, formed after collision of the initial nuclei. To do it we use three conditions. First we fix and define and from the requirement that the center of mass distance and the mass asymmetry of separated ions and the compact system are the same. Then, we vary and among all possible shapes, which satisfies that requirement, we chose the one, that corresponds to the lowest potential energy of compact shape. An example of relation between the shapes of separated ions and the compact system is shown in Fig. 2.

At both stages of calculation the time evolution of the collective degrees of freedom and corresponding momenta is described in terms of the Langevin equations Abe:96 (); Marten:92 (), namely,

 ˙qβ = μβνpν, ˙pβ = −12pνpη∂μνη∂qβ+Kβ−γβνμνηpη+θβνξν. (1)

Here are the deformation parameters and a convention of summation over repeated indices , is used. The quantity is the tensor of friction coefficients and is the tensor inverse to the mass tensor , is a component of the conservative force , where is the free energy of the system, – its potential (deformation) energy, is the level density parameter mebel:92 () and the temperature of system is related to the internal (dissipated) energy by the Fermi-gas formula .

Friction provides the dissipation of collective motion energy into internal energy. The fluctuations in the system are described by the random force . Here is a random number with the following properties

 <ξν> = 0, <ξβ(t1)ξν(t2)> = 2δβνδ(t1−t2). (2)

The magnitude of the random force is expressed in terms of diffusion tensor , which is related to the friction tensor via the modified Einstein relation , where is the effective temperature hofkid ().

The internal energy of the system could be calculated from the energy conservation condition:

 Ecm=Vpot+Ekin+Edis, (3)

here is the reaction energy, calculated in the center-of-mass system, and is the kinetic energy of the collective motion.

Some terms of the equation (1) should be determined twice, ones for the first, and ones for the second stage of calculations. Such terms we will denote by the upper indexes () and (), respectively.

The deformation energy and of colliding ions and of the combined system are calculated within the macroscopic-microscopic shell-correction approach proposed by Strutinsky Strutinsky:67 (); Brack:72 (); Pashkevich:71 (). The interaction potential between the colliding ions consists of Coulomb part kurmanov () and nuclear – Gross-Kalinowski potential Gross:78 () , which was modified Marten:92 () in order to describe the interaction of deformed ions. The rotation of the system is also taken into account on the both stages of calculations:

 EIrot=ℏ2L(L+1)2(Mr2+Jt+Jp),EIIrot=ℏ2L(L+1)2J, (4)

where is the reduced mass of target and projectile, , and are the rigid body moments of inertia of the target, projectile nucleus and of the combined system, respectively, and is an angular momentum of the whole system.

Finally, the potential energy of the system is:

 VIpot = VCoul+VGK+E(t)def+E(p)def+EIrot, (5) VIIpot = Edef+EIIrot. (6)

Besides the deformation energy, the dynamic properties of each nucleus are characterized by the friction and inertia tensors, that were calculated within the linear response approach and local harmonic approximation Hofmann:97 (); Hofmann:08 (). In this approach many quantum effects such as shell and pairing effects, and the dependence of the collisional width of single particle states on the excitation energy, are taken into account. The precise expressions for the components of the friction and inertia tensors can be found in Ivanyuk:1999 (). Tensors and Ivanyuk:1999 () characterize completely the inertia and friction properties of the combined system and were used in our previous calculations within three-dimensional Langevin approach with Cassini shape parameterization and the two-center shell model shape parameterization usang2016 ().

For the first stage of calculation, besides the internal processes in ions, one should account also for their relative motion. The inertial tensor in this case has only diagonal components: (reduced mass), , and . The friction tensor for the first stage of the process was defined as the sum of friction tensor for the relative motion , obtained in the surface-friction model Frobrich:84 (), like it was done in Litnevsky:75:2012 (), and the diagonal friction tensor for colliding ions, which has only two non zero components (; ).

## Iii The results of first stage calculations

In the present paper, the first stage calculations were ended as soon as the system overcomes the potential barrier. The position of the barrier depends on deformations and orientation of the colliding ions. It also slightly depends on angular momentum of the system (see fig. 3).

As one can see, some experimental data in Andreev:18 () are obtained for the sub-barrier energies. In order to describe such reactions we took into account the quantum tunneling through the potential barrier. The penetrability of the barrier was defined in the WKB approximation Nevzorova:08 () as

 TL(E)=[1+exp(2ℏ∫r1r2√2m(Vfus−E)dr)]−1, (7)

where the integration is carried out between the turning points and in the subbarrier region and is the incident energy, equal to the potential energy of the system at the turning points. As one can see from Fig. 4 (bottom), the account of quantum tunneling increases substantially the probability of penetration throw the barrier in the subbarrier region.

The angular momentum is a free parameter of our model. So, the first stage calculations are carried out for various values of . One can see from Fig. 3, that the height of potential barrier increases with the angular momentum of the system. The probability to overcome the barrier will decrease in this case, see Fig. 4. Knowing the probability of event, we can calculate its partial, Fig. 4 ( middle) and total, Fig. 4 (bottom) cross sections, respectively:

 σLbarrier(L,Ecm) = πto0.0pt$¯a$λ2(2L+1)Pbarrier(L,Ecm), (8) σbarrier(Ecm) = ∑LσLbarrier(L,Ecm). (9)

The main goal of the first stage calculations is to get the potential energy of the system, and its internal (dissipated) energy at the touching point.

Having at our disposal the distributions given in Fig. 4 (middle) and Fig. 5b,c,d we can specify (by hit and miss method) the initial values of angular momentum, internal and potential energy of the system for the beginning of the second stage of calculations. The way to choose the initial shape parameters of the combined system was discussed in the previous section, see Fig. 2 and the text around it. So, the initial values for the second stage calculations are defined by the final data from the first stage

 EIIkin,in(L) = EIkin(L), EIIdis,in(L) = EIdis(L)+VIpot−VIIpot. (10)

In order to bring and to the same scale, the so called -value of reaction should be added to

 VIIpot,in⟶VIIpot,in+Q (11)

where is defined in terms of ground state energies . One can also define the excitation energy of reaction

 E∗=Ecm+Q. (12)

The distribution in Fig. 5d is the distribution of rotational energy at the touching point. The width of this distribution is very small. The contribution to this width comes from the uncertainly of center-of-mass distance (which is also small, see Fig. 5a) that appears in the moment of inertia in Eq. (4).

Each point in Fig. 5d is the contribution of trajectory that reached the touching point. By summing over all trajectories one can define the average angular momentum and the average rotational energy of the system at the touching point,

 ⟨L⟩=∑iLi/∑i1,⟨Erot⟩=∑iEirot/∑i1. (13)

The summation over trajectories based on distribution of Fig. 5d leads to the value and 1.89 MeV. In the same way we can calculate the average value of dissipated energy 4.40 MeV. As we can see, the sum of rotational and dissipated energy at the touching point is not so large compared with the excitation energy =50.5 MeV.

## Iv The evolution of compact system

The potential energy surface of Pt in coordinates - mass asymmetry, , is shown in Fig. 6. The star in this figure marks the position of initial point corresponding to the shape shown in Fig.2.

Starting from the touching point under the action of random force the system would move in the direction of ground state, form the compound nucleus and then undergo fission. The evolution of the compound nucleus could last long enough to evaporate gammas or light particles, so we should take into account this de-excitation process. The evaporation of particles and -quanta by the excited compact system is described in our approach within the statistical model mebel:92 (). On each integration step the partial width of the corresponding decay channel mebel:92 () is calculated, then by the hit-and-miss method we decide whether some particle was emitted and which kind of particle was emitted. If some particle was emitted, the binding energy of this particle was subtracted from the excitation energy of the system. Also the particle can carry away some energy (its kinetic energy).

The main evaporation channel is the evaporation of neutrons. Probability of the neutron evaporation and its kinetic energy depends on the dissipated energy of the system (see Fig. 7). One can see, that system with dissipated energy MeV, for example, should live on average zs before first neutron is evaporated.

After evaporation it loses about MeV as a neutron kinetic and binding energy, so, to evaporate the second neutron it needs about zs, and so on. Of course, during this evolution time there is a competition between neutron evaporation and fission. The fission of nucleus can occur before it evaporates any neutron (dashed line), or it could evaporate one (short dashed line), two (dotted line) or more neutrons before fission (see Fig. 8). The maximal number of the evaporated neutrons depends on the initial excitation energy of the system , see Eq. (12).

After evaporation of several neutrons the systems internal energy decreases and the role of the nuclear shell structure become more and more significant. In Fig. 9 one can see the evolution of fragment mass distribution due to the de-excitation process (for the initial excitation energies MeV and MeV). The mass distribution is symmetric if the system undergoes fission before it evaporates any neutron. Then, after the first neutron evaporation, the system slightly cools down and the influence of the shell effects will be noticeable. And, finally, after second neutron evaporation the distribution becomes strongly asymmetric.

The total mass distribution obtained by superimposing of distributions shown in Fig. 9 is compared in Fig. 10 with the experimental data Andreev:18 (). One can see that the calculated mass distributions for all three values of excitation energy are very close to the experimental data.

## V The total kinetic energy

The mass-energy distribution of fission events is shown in the left part of Fig. 11. In these calculations for each trajectory that reached the scission point we define as the sum of the Coulomb interaction of spherical fragments at the scission point and prescission kinetic energy ,

 TKEi=E(int)Coul(qi)+KE(pre)i. (14)

Here

 E(int)Coul(qi)≡ZLZHe2/r(qi), (15)

where and are the charges of light and heavy fragments. The prescission kinetic energy is the kinetic energy in fission direction obtained from the solutions of Langevin equations at the scission point. It turned out in these calculations that the average value of is very small, of the order of MeV and the main contribution to TKE comes from the Coulomb repulsion energy.

The TKE-distribution of fission fragments is shown in the right part of Fig. 11. The shape of distribution is very close to a single Gaussian.

The average value of TKE is equal to 130.4 Mev what is rather close to the position of main peak, TKE=133.4 MeV, in experimental results Andreev:18 (). The width of TKE-distribution = 11 MeV is, however, much smaller than experimental value, see Fig. 2a of Andreev:18 (). The difference might be attributed to the uncertainty of scission point configuration formed in the reaction, the finite (in)accuracy of TKE measurements and some limitations of theoretical approach.

## Vi Acknowledgments

This study includes the results of Research and development of an innovative transmutation system of LLFP by fast reactors, entrusted to the Tokyo Institute of Technology by the Ministry of Education, Culture, Sports, Science and Technology of Japan (MEXT). The authors would like to thank to Prof. A.N. Andreyev and Prof. I. Tsekhanovich for useful discussions.

## Vii Conclusions

Within the developed earlier two-stage approach for the fusion-fission reactions we have studied the reaction . The obtained results are compared with the available experimental data. The calculated mass distributions of fission fragments for three energies =122.78, 134.68 and 142.58 MeV are in good agreement with the experimental data Andreev:18 (). The most probable mass division for asymmetric component of fission fragments mass distribution (Fig. 10) is found to be about , what is rather close to the experimental data Andreev:18 (). From our calculations it follows that the competition between symmetric and asymmetric fission channels is caused by the enhancement of shell effects in the compound nucleus due to the process of its de-excitation by neutron emission.

The average value of TKE is equal to 130.4 Mev what is rather close to the position of main peak, TKE=133.4 MeV, in experimental results. The calculated shape of distribution is very close to a single Gaussian. We did not find the contributions to TKE-distribution from two fission modes as it was argued in Andreev:18 ().

From the results of calculations it follows that the dynamical trajectories do not follow the bottom of fission valley and the mass- and energy-distributions of fission fragments of Pt are formed mainly at the saddle.

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