A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes

In this paper, even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes have been studied the ground state bands using Matlab computer code (IBM-1.Mat). We apply the interacting boson model-1 (IBM-1) formula for O(6) symmetry in Ru isotopes with neutron N = 60, 62. The theoretical energy levels up to spin-parity 12⁺ have been...

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Автори: Hossain, I., Kassim, Huda H., Sharrad, Fadhil I., Al-Jubbori, Mushtaq A., Salam, A., M., Saleem
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Опубліковано: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2020
Назва видання:Вопросы атомной науки и техники
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Цитувати:A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes / I. Hossain, Huda H. Kassim, Fadhil I. Sharrad, Mushtaq A. Al-Jubbori, A. Salam, M. Saleem // Problems of atomic science and tecnology. — 2020. — № 5. — С. 13-18. — Бібліогр.: 23 назв. — англ.

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spelling irk-123456789-1945582023-11-27T16:14:10Z A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes Hossain, I. Kassim, Huda H. Sharrad, Fadhil I. Al-Jubbori, Mushtaq A. Salam, A. M., Saleem In this paper, even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes have been studied the ground state bands using Matlab computer code (IBM-1.Mat). We apply the interacting boson model-1 (IBM-1) formula for O(6) symmetry in Ru isotopes with neutron N = 60, 62. The theoretical energy levels up to spin-parity 12⁺ have been obtained for ¹⁰⁴⁻¹⁰⁶Ru isotopes. The yrast states, gamma band, beta band, and B(E2) values are calculated for these nuclei. The published experimental and calculated R4/2 values indicate that the even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes have O(6) dynamic symmetry. The present results have been compared to the published experimental data and are found good harmony with each other. The outcome of our investigation of the potential energy surfaces (PES) of both isotopes belonging to O(6) character. Використовуючи Matlab комп’ютерний код (IBM-1.Mat), досліджені полоси основних станів парно-парних ізотопів ¹⁰⁴⁻¹⁰⁶Ru. Ми застосували формулу моделі-1 взаємодіючих бозонів (IBM-1) для O(6) симетрії Ru-ізотопів для N=60, 62 нейтронів. Теоретичні значення енергетичних рівнів до значень спін-парності 12⁺ були отримані для ізотопів ¹⁰⁴⁻¹⁰⁶Ru. Для цих ядер обчислені yrast-стани, γ-смуги, β-смуги та B(E2)-величини. Опубліковані експериментальні та розрахункові величини R4/2 показують, що парно-парні ізотопи ¹⁰⁴⁻¹⁰⁶Ru мають O(6) динамічну симетрію. Ці розрахунки порівнювалися з опублікованими даними експериментальних досліджень, і знайдено добре узгодження між ними. Наші дослідження поверхні потенціальної енергії (ППЕ) вказують на O(6) характер обох ізотопів. Используя Matlab компьютерный код (IBM-1.Mat), исследовались полосы основных состояний четно-четных изотопов ¹⁰⁴⁻¹⁰⁶Ru. Мы применили формулу модели-1 взаимодействующих бозонов (IBM-1) для O(6) симметрии Ru-изотопов для N=60, 62 нейтронов. Теоретические значения энергетических уровней до значений спин-четности 12⁺ были получены для изотопов ¹⁰⁴⁻¹⁰⁶Ru. Для этих ядер вычислены yrast-состояния, γ-полосы, β-полосы и B(E2)-величины. Опубликованные экспериментальные и расчетные величины R4/2 показывают, что четно-четные изотопы ¹⁰⁴⁻¹⁰⁶Ru имеют O(6) динамическую симметрию. Эти результаты сравнивались с опубликованными данными экспериментальных исследований, и найдено хорошее согласие между ними. Наши исследования поверхности потенциальной энергии (ППЭ) указывают на O(6) характер обоих изотопов. 2020 Article A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes / I. Hossain, Huda H. Kassim, Fadhil I. Sharrad, Mushtaq A. Al-Jubbori, A. Salam, M. Saleem // Problems of atomic science and tecnology. — 2020. — № 5. — С. 13-18. — Бібліогр.: 23 назв. — англ. 1562-6016 PACS: 21.10.-k;42.40.Ht; 42.30.Kq http://dspace.nbuv.gov.ua/handle/123456789/194558 en Вопросы атомной науки и техники Національний науковий центр «Харківський фізико-технічний інститут» НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description In this paper, even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes have been studied the ground state bands using Matlab computer code (IBM-1.Mat). We apply the interacting boson model-1 (IBM-1) formula for O(6) symmetry in Ru isotopes with neutron N = 60, 62. The theoretical energy levels up to spin-parity 12⁺ have been obtained for ¹⁰⁴⁻¹⁰⁶Ru isotopes. The yrast states, gamma band, beta band, and B(E2) values are calculated for these nuclei. The published experimental and calculated R4/2 values indicate that the even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes have O(6) dynamic symmetry. The present results have been compared to the published experimental data and are found good harmony with each other. The outcome of our investigation of the potential energy surfaces (PES) of both isotopes belonging to O(6) character.
format Article
author Hossain, I.
Kassim, Huda H.
Sharrad, Fadhil I.
Al-Jubbori, Mushtaq A.
Salam, A.
M., Saleem
spellingShingle Hossain, I.
Kassim, Huda H.
Sharrad, Fadhil I.
Al-Jubbori, Mushtaq A.
Salam, A.
M., Saleem
A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
Вопросы атомной науки и техники
author_facet Hossain, I.
Kassim, Huda H.
Sharrad, Fadhil I.
Al-Jubbori, Mushtaq A.
Salam, A.
M., Saleem
author_sort Hossain, I.
title A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
title_short A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
title_full A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
title_fullStr A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
title_full_unstemmed A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes
title_sort study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶ru isotopes
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
publishDate 2020
url http://dspace.nbuv.gov.ua/handle/123456789/194558
citation_txt A study on the ground states structure of even-even ¹⁰⁴⁻¹⁰⁶Ru isotopes / I. Hossain, Huda H. Kassim, Fadhil I. Sharrad, Mushtaq A. Al-Jubbori, A. Salam, M. Saleem // Problems of atomic science and tecnology. — 2020. — № 5. — С. 13-18. — Бібліогр.: 23 назв. — англ.
series Вопросы атомной науки и техники
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fulltext A STUDY ON THE GROUND STATES STRUCTURE OF EVEN-EVEN 104−106Ru ISOTOPES I.Hossain1∗, HudaH.Kassim2, Fadhil I. Sharrad2, MushtaqA.Al-Jubbori3, A. Salam4, M. Saleem5 1Department of Physics, Rabigh college of Science and Arts, 21911 Rabigh, King Abdulaziz University, Jeddah, Saudi Arabia; 2Department of Physics, College of Science, Kerbala University, 56001 Karbala, Iraq; 3Department of Physics, College of Education for Pure Science, University of Mosul, 41001 Mosul, Iraq; 4Department of chemistry, Rabigh college of Science and Arts, 21911 Rabigh, King Abdulaziz University, Jeddah, Saudi Arabia; 5Department of Industrial Engineering, Faculty of Engineering-Rabigh, King Abdulaziz University, Saudi Arabia (Received May 6, 2019) In this paper, even-even 104−106Ru isotopes have been studied the ground state bands using Matlab computer code (IBM-1.Mat). We apply the interacting boson model-1 (IBM-1) formula for O(6) symmetry in Ru isotopes with neutron N = 60, 62. The theoretical energy levels up to spin-parity 12+ have been obtained for 104−106Ru isotopes. The yrast states, gamma band, beta band, and B(E2) values are calculated for these nuclei. The published experimental and calculatedR4/2 values indicate that the even-even 104−106Ru isotopes haveO(6) dynamic symmetry. The present results have been compared to the published experimental data and are found good harmony with each other. The outcome of our investigation of the potential energy surfaces (PES) of both isotopes belonging to O(6) character. PACS: 21.10.-k;42.40.Ht; 42.30.Kq 1. INTRODUCTION Recently Ruthenium isotope has been a focus of the nuclear structure of many theoretical and experimen- tal investigations. The low-lying even nuclei had been successfully explained nuclear collective charac- ters using IBM-1[1]. In the first beginning the collec- tive states can be describes by a system of identical bosons NB . These are S-boson (L = 0) and d-boson (L = 2). There is no discrepancy between neutron and proton in IBM-1. There are three dynamical symmetries indicated by U(5) analogous to spherical vibrator, SU(3) deformed rotor and O(6) γ-soft. The microscopic a harmonic vibrator approach (MAVA) used in investigating the lower level collective states in Ruthenium isotopes [2]. The Ruthenium isotopes have atomic number Z = 44. It belongs near to closed shell Sn (magic number Z = 50). The external forms of even 104−106Ru isotopes have πg−6 9/2 (6 proton holes) and νg10,129/2 (10 and 12 neutron particles) close to magic number 50. This configuration has been investigated the ground state structure from spherical to deformed symmetry. The edifice of yrast levels and electromag- netic strength of Ru isotopes were studied by many scientists [3-7]. Recently, the properties of the yrast level were studied in Pd isotopes with even neutron N = 54...64 [8]. The electromagnetic reduced transition strength of Cd isotopes with N = 66...74 were investigated [9]. The B(E2) value of yrast band of even 102−112Pd and 96−102Ru isotopes were investigated by IBM-1[10,11]. The lower level of 184W and 184Os nuclei were inves- tigated [12]. The present aim particularly focuses the struc- ture of the yrast band, gamma band and beta band, electromagnetic transition and the potential energy surfaces to find the dynamical symmetry of even 104−106Ru isotopes by the application of IBM. 2. METHODOLOGY The Interacting Boson Model (IBM) gives occupation to truncated model space for nuclei with N number of nucleons. It provides a quantitative description of in- distinguishable particles with forming pairs of L = 0 and 2. The Hamiltonian of IBM-1[13] is given H = ΣN i=1εi +ΣN i<jVij , (1) where εi indicates energy of boson, Vij indicates po- tential energy of boson between i and j. Hamiltonian ∗Corresponding author E-mail address: mihossain@kau.edu.sa ISSN 1562-6016. PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY, 2020, N5(129). Series: Nuclear Physics Investigations (74), p.13-18. 13 is given from multi-pole form [14] Ĥ = εn̂d + α0P̂ .P̂ + α1L̂.L̂+ α2Q̂.Q̂+ + α3T̂3.T̂3 + α4T̂4.T̂4 , (2) where n̂d = (d+, d̃), P̂ = 1 2 (d̃.d̃)− 1 2 (s̃.s̃), L̂ = √ 10[d+ × d̃](1), Q̂ = [d+ × s̃+ s+ × d̃](2) − √ 7 2 [d+ × d̃](2), T̂3 = [d+ × d̃](3), T̂4 = [d+ × d̃](4). Here P̂ ( the pairing operator), Q̂ (quadrupole oper- ator), ( number of n̂d boson), L̂ (operator of angu- lar momentum), and T̂3 (octupole operators), and T̂4 (hexadecapole operators). The Hamiltonian starting with U(6) and complete with group O(2) as given in Eq.(2) is bringing to a lower state of three limits, gamma-soft O(6), vi- bration U(5) and rotational SU(3) nuclei [15]. It is known that the limit in the O(6), SU(3) and U(5) the parameters are α0, α2, and ε respectively. The Hamiltonian and eigen-values for the three limits [16]: U(5) : ĤU(5) = εn̂d + α1L̂.L̂+ α3T̂3.T̂3 + α4T̂4.T̂4 , E(nd, σ, L) = εnd +K1nd(nd + 4) + +K4σ(σ + 3) +K5L(L+ 1), (3) with K1 = 1/12 a1 , K4 = −1/10 a1 + 1/7 a3 − 3/70 a4 , K5 = −1/14 a3 + 1/14 a4 . O(6) : ĤO(6) = α0P̂ .P̂ + α1L̂.L̂+ α3T̂3.T̂3 , E(σ, ν, L) = K3 [N(N + 4)− σ(σ + 4)] + +K4ν(ν + 3) +K5L(L+ 1), (4) with K1 = 1/4 a0 , K4 = 1/2 a3 , K5 = −1/10 a3 + a1 . SU(3) : ĤSU(3) = α1L̂.L̂+ α2Q̂.Q̂ , E(λ, µ, L) = K2 [ λ2 + µ2 + λµ+ 3(λ+ µ) ] + +K5L(L+ 1), (5) with K2 = 1/2 a2 , K5 = a1 − 3/8 a2 . K1, K2, K3, K4, and K5 are other strength parame- ters. Then applying particular limit of symmetry (O(6), SU(3), U(5)) to determine the frame of a set of nuclei is more advantageous than full Hamiltonian of IBM-1. It comprise multi-free parameters those make it simple to fit the structure of a nuclei. 3. RESULTS AND DISCUSSION The obtained results can be discussed for yrast state, γ-band, β-band, effective charge, transition probabil- ities B(E2), maxing ratio and potential energy sur- faces. The calculations were done by IBM-1. The γ-unstable limit has applied for 104,106Ru nu- clei using published data of energy ratios (E2 : E4 : E6 : E8 = 1 : 2.5 : 4.5 : 6.5). In the IBM-1, the even 104,106Ru nuclei have 3 proton boson holes and 5 and 6 neutron boson particle respectively. Therefore to- tal bosons numbers of 104Ru and 106Ru nuclei are 8 and 9, respectively. The IBM-1 models carry out with no difference between the bosons of proton and neutron. The energy ratio R = E4+1 /E2+1 gives the information of the symmetry shapes of a nucleus. The symbol E2+1 and E4+1 are at energy level 2+1 and 4+1 respectively. It is known that the R = E4+1 /E2+1 ≈ 2 is for U(5), R = E4+1 /E2+1 ≈ 2.5 is for O(6) and R = E4+1 /E2+1 ≈ 3.33 for SU(3) [17,18]. The experi- mental R4/2 of 104Ru and 106Ru isotopes is 2.48 and 2.60, respectively. In Fig.1 shows R4/2 values and found O(6) symmetry in 104Ru and 106Ru isotopes. 1.5 2 2.5 3 3.5 4 E 4 /E 2 v a lu e Neutron number U(5) SU(3) O(6) 60 62 Fig.1. The arrows indicate the U(5), O(6) and SU(3) limits. The E(4−1 )/E(2−1 ) values of ex- perimental data [22] of the 104,106Ru isotopes are presented as function of neutrons The best fit was taken up to 12+ of Ru isotopes with neutron N = 60, 62. The parameters were de- termined the experimental eigen values (E(nd, σ, L)) from the equation (4). Where nd, σ, and L are quan- tum numbers. The parameters are shown in Table 1. 14 Table 1. Adopted values of parameters used for IBM-1 calculations. All parameters are given in MeV , excepted N and CHQ A N ε a0 a1 a2 a3 a4 CHQ(χ) 104Ru 8 0.000 0.1098 0.0180 0.000 0.1770 0.000 0.000 106Ru 9 0.000 0.0990 0.0102 0.000 0.1513 0.000 0.000 The calculated energy levels as well as experimen- tal data are presented in Table 2. According to the weight of fitting the Ru − 104 and Ru − 106 nuclei are good candidates of O(6) symmetry. Table 2. g-band (in MeV ) for even 104−106Ru nuclei IBM Exp. IBM Exp. Jπ 104Ru 106Ru 0+ 0.000 0.000 0.000 0.000 2+ 0.3558 0.3580 0.2726 0.2700 4+ 0.8910 0.8884 0.6570 0.7147∗ 6+ 1.6056 1.5564 1.1532 1.2958∗ 8+ 2.4996 2.3204 1.7612 1.9734∗ 10+ 3.5730 3.1119 2.4810 2.7050 12+ 4.8258 — 3.3126 3.4500∗ The present data of γ-bands and β-bands are pre- sented in Tables 3 and 4 and they are compared with published measured data. From the tables, the IBM calculations and experimental results are in good agreements [19]. Table 3. γ-band (in MeV ) for even 104−106Ru nuclei IBM Exp. IBM Exp. Jπ 104Ru 106Ru 2+ 0.8868 0.8931 0.7256 0.7923 3+ 1.5966 1.2424 1.2610 1.0915∗ 4+ 1.5990 1.5026 1.3002 1.3068∗ 5+ 2.4870 1.8723∗ 1.9082 1.6411∗ 6+ 2.4906 2.1966∗ 1.9670 1.9078∗ 7+ 3.5568 —- 2.6672 2.2841∗ 8+ 3.4878 —- 2.7456 2.9600∗ 9+ 4.8060 — 3.6360 — Table 4. β-band (in MeV ) for even 104−106Ru nuclei IBM Exp. IBM Exp. Jπ 104Ru 106Ru 0+ 0.9882 0.9882 0.9900 0.9906 2+ 1.3440 1.5154 1.2626 1.3922 4+ 1.8792 2.0808 1.6470 —- 6+ 2.5938 — 2.1432 — 8+ 3.5616 — 2.7512 — 10+ 4.8120 — 3.5380 — The reduced electric transition probabilities give the more properties on the structure of nuclei. It is known that the E2 transition operator must be a Her- mitian tensor of rank two; consequently, the number of bosons must be conserved. TE2 = α2 [ d+s+ s+d ](2) + β2 [ d+d ](2) , (6) where (s+, d+) are creation and (s, d) are annihilation operators for bosons s and d. TE2 is the operator of reduced matrix elements of the E2. α2 is indicated the effective quadrupole charge and β2 is dimension- less coefficient, β2 = χα2. B(E2, Ji → Jf ) = 1 2Ji + 1 ∣∣⟨Jf ∥∥TE2 ∥∥ Ji⟩∣∣2 . (7) The parameters, α2 and β2 of Eq.(6), ac- commodated suitably a set to reproduce the published B(E2; 2+1 → 0+1 ). The effective charge (eB) in present calculation is shown in Table 5. The values of eB were estimated to reproduce experimentally (B(E2; 2+1 → 0+1 )). Table 5. Effective charge for even 104−106Ru nuclei A N eB(eb) 104Ru 8 0.0935 106Ru 9 0.0916 15 The values β2 = 0 for 104,106Ru isotopes because these nuclei have the O(6) property. The values of B(E2) data are presented in Table 6 for Ru iso- topes with neutron N = 60, 62 in this study [19]. The calculated data of IBM-1 is good agreements with the available published experimental results. Table 6. The B(E2) value (in e2b2) of even 104−106Ru isotopes IBM Exp. IBM Exp. Ji → Jf 104Ru 106Ru 2+1 → 0+1 0.1679 0.1682 0.1966 0.1966 4+1 → 2+1 0.2273 0.2149 0.2689 – 4+2 → 2+2 0.1282 – 0.1541 – 6+1 → 4+1 0.2448 – 0.2941 – 6+2 → 4+2 0.1626 – 0.2000 – 8+1 → 6+1 0.2384 – 0.2934 – 10+1 → 8+1 0.2152 – 0.2747 – 10+2 → 8+2 0.0941 – 0.0000 – 2+2 → 2+1 0.2273 0.1957 0.2689 – 4+2 → 4+1 0.1166 – 0.1401 – 6+2 → 6+1 0.0759 – 0.0933 – 8+2 → 8+1 0.0000 – 0.0659 – The application of potential energy surface (PES) gives the information to find microscopic and geomet- ric shapes such as spherical, prolate, oblate and γ-independent (γ-soft)). It gives us about symmetry, the shape of nuclei, the minimum deepness and the change of the shape. The PES plots using Skyrme mean field method was drawn by IBM Hamiltonian [20-23]. The state is a product of the boson creation operators b+c with |N, β, γ⟩ = 1√ N ! ( b+c )N |0⟩ , (8) b+c = (1 + β2)−12 { s+ + β [ cos γ(d+0 )+ + √ 1/2 sin γ(d+2 + d+−2) ]} . (9) The energy surface as a function of β and γ, has been given [1] E(N, β, γ) = = Nεdβ 2 (1 + β2) + N(N−1) (1+β2)2(α1β4+α2β3 cos 3γ+α3β2+α4) . (10) Here the αi’s are related to the Casimir coefficients CL, ν2, ν0, u2 and u0. β were indicated the total de- formation of a nucleus. Then, we can re-write equa- tion (10) for O(6) limit [19]. Fig.2 shows the contour plots in the γ− β plane resulting from E(N, β, γ) for 104Ru and 106Ru isotopes. The color lines show the values of the potential energy surface in MeV . The potential surfaces are approximately independent of gamma only. The mapped IBM energy surfaces of 104Ru and 106Ru are O(6) character. Fig.2. Contour map of potential energy surfaces for Ru isotopes with N = 60, 62 4. CONCLUSIONS The yrast band, gamma band and beta band, elec- tromagnetic transition and potential energy surface of 104Ru and 106Ru isotopes have been calculated in term of O(6) limit of IBM-1. The levels up to 12+ of 104,106Ru nucleus are found by the Hamilto- nian of IBM-1. The analyses of the IBM-1 results suggest a satisfactory agreement with the published experimental data. It is established that interacting boson approximations for 104Ru and 106Ru isotopes are considered as gamma soft O(6) symmetry. 16 ACKNOWLEDGMENTS This project was funded by the Deanship of Scientific Research (DSR) at King Abdulaziz University, Jed- dah, under grant No. G-223-662-37. The authors, therefore, acknowledge with thanks DSR for techni- cal and financial support. References 1. F. Iachello, and A.Aritma. The interacting boson model. Cambridge: Cambridge Univ. press, 1987. 2. J.Kotila, J. Suhonen, and D. S.Delion. Low-lying collective states in Ru98−106 isotopes studied us- ing a microscopic anharmonic vibrator approach //Phys. Rev. 2003, v.C 68, p.054322. 3. X. L.Che, et al. High spin band structure in 112Ru // Chin. Phys. Lett. 2004, v.21, p.1904. 4. X. L.Che, et al. Collective band structures in the neutron-rich 107,109Ru nuclei // Chin. Phys. Lett. 2006, v.23, p.328. 5. Y.X. Luo, et al. Odd-parity bands of 108,110,112Ru // Int. J. Mod. Phys. 2009, v.E 18, p.1697-1716. 6. A. Frank, P.V. Isacker, D.D.Warner. Super sym- metry in transitional nuclei and its application to the Ru and Rh isotopes // Phys. Lett. 1997, v.B 197(4), p.474-478. 7. D.Troltenier, J. A.Maruhm, W.Greiner, V.A.Velazquez, P.O.Hess, J. H. Z.Hamilton // Phys. 1991, v.A 338, p.261. 8. I.M.Ahmed, et al. The evolution properties of even-even 100−110Pd nuclei // Int. J. Mod. Phys. v.E 21, p.1250101. 9. H.Y.Abdullah, et al. Electromagnetic reduced transition properties of even- even 104−112Cd iso- topes // Indian J. Phys. 2013, v.87, p.571-575. 10. I. Hossain, M.A. Saeed, N.N.A.M. B.Ghani, H. Sa’adeh, M.Hussein, H.Y.Abdullah. Electro- magnetic reduced transition properties of the ground state band of even-even 102−106Pd iso- topes by means of interacting boson model-1 // Indian J. Phys. 2014, v.88, p.5-9. 11. I. Hossain, H.Y.Abdullah, I.M.Ahmed, M.A. Saeed. B(E2) value of even-even 108−112Pd isotopes by interacting boson model-1 // Chin. Phys. 2014, v.C 38, p.024104. 12. F. I. Sharrad, I. Hossain, I.M.Ahmed, H.Y.Abdullah, S. T.Ahmad, A. S.Ahmed. U(5) symmetry of even 96,98Ru isotopes under the framework of interacting boson model (IBM-1) // Braz J Phys. 2015, v.45, p.340-346. 13. L.K.Green. Nuclear structure of 112Cd through studies of decay. M.Sc. thesis. The University of Green, 2009. 14. K.A.Al-Maqtary. IBM-1 Calculations of energy levels and electric transition probabilities B(E2) in 158−160Gd isotopes // Jordan J. Phys. 2013, v.6, p.95-102. 15. F. Lachello. Nuclear Structure / Edited by K Abraham, K Allaart and A. E. L. Dieperink, New York: Plenum press, 1981. 16. P.V. Isacker. The Interacting Boson Model // Nuclear Structure and Decay Data: Theory and Evaluation workshop, Trieste - Italy, 04 - 15 April, 2005. 17. V.N. Zamfir, R. F.Casten. Proceedings of the Ro- manian Academy, Series A, 4, 1, 2003. 18. Harish Mohan MITTAL and Vidya DEVI // Turk. J. Phys., 2012, v.36, p.117. 19. B.Richard and Firestone. Table of isotopes (John willey and sons), 1999. 20. R. F.Casten and D.D.Warner. The interacting Boson approximation // Rev. Mod. Phys. 1988, v.60, p.389-469. 21. L.M.Robledo, et al. Role of triaxiality in the ground-state shape of neutron- rich Y b, Hf , W , Os and Pt isotopes // J. Phys. G: Nucl. Part. Phys. 2009, v.36, p.115104. 22. K.Nomura, et al. Derivation of IBM Hamiltonian for deformed nuclei // J. Phys.Conf. Ser. 2009, v.267, p.012050. 23. R. F.Casten, N.V. Zamfir. Empirical Realization of a Critical Point Description in Atomic Nuclei // Phys. Lett. 2001, v.87, p.052503. 17 ÈÑÑËÅÄÎÂÀÍÈÅ ÑÒÐÓÊÒÓÐÛ ÎÑÍÎÂÍÛÕ ÑÎÑÒÎßÍÈÉ ×ÅÒÍÎ-×ÅÒÍÛÕ ÈÇÎÒÎÏΠ104−106Ru I. Hossain, HudaH.Kassim, Fadhil I. Sharrad, MushtaqA.Al-Jubbori, A. Salam, M. Saleem Èñïîëüçóÿ Matlab êîìïüþòåðíûé êîä (IBM-1.Mat), èññëåäîâàëèñü ïîëîñû îñíîâíûõ ñîñòîÿíèé ÷åòíî- ÷åòíûõ èçîòîïîâ 104−106Ru. Ìû ïðèìåíèëè ôîðìóëó ìîäåëè-1 âçàèìîäåéñòâóþùèõ áîçîíîâ (IBM-1) äëÿ O(6) ñèììåòðèè Ru-èçîòîïîâ äëÿ N = 60, 62 íåéòðîíîâ. Òåîðåòè÷åñêèå çíà÷åíèÿ ýíåðãåòè÷åñêèõ óðîâíåé äî çíà÷åíèé ñïèí-÷åòíîñòè 12+ áûëè ïîëó÷åíû äëÿ èçîòîïîâ 104−106Ru. Äëÿ ýòèõ ÿäåð âû÷èñ- ëåíû yrast-ñîñòîÿíèÿ, γ-ïîëîñû, β-ïîëîñû è B(E2)-âåëè÷èíû. Îïóáëèêîâàííûå ýêñïåðèìåíòàëüíûå è ðàñ÷åòíûå âåëè÷èíû R4/2 ïîêàçûâàþò, ÷òî ÷åòíî-÷åòíûå èçîòîïû 104−106Ru èìåþò O(6) äèíàìè- ÷åñêóþ ñèììåòðèþ. Ýòè ðåçóëüòàòû ñðàâíèâàëèñü ñ îïóáëèêîâàííûìè äàííûìè ýêñïåðèìåíòàëüíûõ èññëåäîâàíèé, è íàéäåíî õîðîøåå ñîãëàñèå ìåæäó íèìè. Íàøè èññëåäîâàíèÿ ïîâåðõíîñòè ïîòåíöèàëü- íîé ýíåðãèè (ÏÏÝ) óêàçûâàþò íà O(6) õàðàêòåð îáîèõ èçîòîïîâ. ÄÎÑËIÄÆÅÍÍß ÑÒÐÓÊÒÓÐÈ ÃÎËÎÂÍÈÕ ÑÒÀÍI ÏÀÐÍÎ-ÏÀÐÍÈÕ IÇÎÒÎÏI 104−106Ru I. Hossain, HudaH.Kassim, Fadhil I. Sharrad, MushtaqA.Al-Jubbori, A. Salam, M. Saleem Âèêîðèñòîâóþ÷è Matlab êîìï'þòåðíèé êîä (IBM-1.Mat), äîñëiäæåíi ïîëîñè îñíîâíèõ ñòàíiâ ïàðíî- ïàðíèõ içîòîïiâ 104−106Ru. Ìè çàñòîñóâàëè ôîðìóëó ìîäåëi-1 âçà¹ìîäiþ÷èõ áîçîíiâ (IBM-1) äëÿ O(6) ñèìåòði¨ Ru-içîòîïiâ äëÿ N = 60, 62 íåéòðîíiâ. Òåîðåòè÷íi çíà÷åííÿ åíåðãåòè÷íèõ ðiâíiâ äî çíà÷åíü ñïií-ïàðíîñòi 12+ áóëè îòðèìàíi äëÿ içîòîïiâ 104−106Ru. Äëÿ öèõ ÿäåð îá÷èñëåíi yrast-ñòàíè, γ-ñìóãè, β-ñìóãè òà B(E2)-âåëè÷èíè. Îïóáëiêîâàíi åêñïåðèìåíòàëüíi òà ðîçðàõóíêîâi âåëè÷èíè R4/2 ïîêàçó- þòü, ùî ïàðíî-ïàðíi içîòîïè 104−106Ru ìàþòü O(6) äèíàìi÷íó ñèìåòðiþ. Öi ðîçðàõóíêè ïîðiâíþâàëèñü ç îïóáëiêîâàíèìè äàíèìè åêñïåðèìåíòàëüíèõ äîñëiäæåíü, i çíàéäåíî äîáðå óçãîäæåííÿ ìiæ íèìè. Íà- øi äîñëiäæåííÿ ïîâåðõíi ïîòåíöiàëüíî¨ åíåðãi¨ (ÏÏÅ) âêàçóþò íà O(6) õàðàêòåð îáîõ içîòîïiâ. 18