Mixed symmetry states in samarium isotopes with a=146-154 by using (ibm-2)



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[Al – Sadi * et al., 6(10): October, 2017] Impact Factor: 4.116

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International Journal of Engineering Sciences & Research Technology

MIXED SYMMETRY STATES IN SAMARIUM ISOTOPES WITH A=146-154 BY USING (IBM-2)

Mohammed Abdul Kadhim Al – Sadi*

*Environmental Pollution Department , Collage of Environment Science, Al- Qasim Green University


DOI: 10.5281/zenodo.1036266
ABSTRACT

In this work, we used tthe (IBM-2) to study the mixed symmetry state property (MSS) foreven-even146-152Sm isotopes, this model gave a good agreementfor the excited energy levels for the g- band and acceptable for quasi (β and γ) bands, Also identified and emphase some states un certain experimentally, Furthermore it have been studied the mixed symmetry state (MSS) for the states (,,,,) Which received a quick response when changing the Majorana parameters for these isotopes.Well, it was calculated the electromagnetic transition B(E2), B(M1) and mixing ratios


KEYWORDS: IBM-2,Smisotopes, Mixed Symmetry State(MSS),Electomagnetic transition, Mixing ratios.


  1. INTRODUCTION

In the interacting boson model (IBM), the nuclear shape for even – even nuclei is characterized as far as interaction among s(L=zero) and d(L=2 ) bosons. through modifying a little amount of parameter, it creates the overall population of the low-ling condition of such cores [1,2]. The early model of the communicating boson display known as IBM-1, in which no distinction is made among protons (sπ, dπ), neutron bosons (sν,dν), and the quantity of bosons taken to be the assortment of nucleons open air the shut shell partitioned by . the second one variant of the Interacting Boson demonstrate ( IBM-2 ) , recognizes among protons (sπ,dπ) and neutron bosons(sν,dν) . while the principal show has a symmetry issue, similar to; dipole attractive change, blended symmetry states and electric monopole advances, the second one variant has no impediment [3-4].


  1. THE (IBM-2) MODEL

The IBM-2 Hamiltonian in this model is given as bellow [5,6];


where is the energy difference between s and d boson, is the number of d bosons , where ρ corresponds to π ( proton ) or ν ( neutron ) bosons , the second term denotes the quadrupole – quadrupole interaction between proton and neutron with strength κ , where the quadruple operator is define as [7] .


Where VππandVνν are represented the interaction of identical bosons which is given as bellow [8] .


The Majorana term Includes three parameters and can be written as;


The (MSS) happen when the protons and neutrons are not in stage in the quantum state [9]. These states were made by blend of two wave function, one for proton and other for neutron [13]. The blended symmetry states dictated by the F-spinshape, where the F-turn formalism is similar to the isospin quantum number of the nucleons. Proton bosons and neutron bosons have F = 1/2 and z-projection, where Fz = +1/2 , - 1/2 for protons and neutrons separately. For a framework comprise of Nπ proton boson and Nν neutron boson , the most extreme F-turn is F = Fmax = ( Nπ + Nν )/2 , while the blended symmetry states described by diminishing F-turn esteem ( F = Fmax , F = Fmax – 1, F = Fmax - 2 , . . . , Fmin= |Nπ - Nν |/2 ). In the F-turn space, one can likewise characterize the creation and obliteration administrators F+ and F− by [10-11];

, . ..........(5)
The projection operator Fz is given by .

.........(6)
A state formed by Nπ proton bosons and Nν neutron bosons with F-spin quantum number F = Fmax can be changed by the progressive activity of the F-spinraising administrator F+ into an express that comprises of proton bosons as it were. This state has still an aggregate F-turn quantum number F=Fmax since the raising administrator does not change the aggregate F-turn quantum number. This new state has just proton bosons and clearly remains unaltered under a pairwise trade of proton and neutron names. Accordingly, IBM-2 states with F=Fmax are called Full Symmetry States (FSS). These states compare really to the IBM-1 states which are largely symmetric. All others states with F-turn quantum numbers F< Fmax contain sets (no less than one) of proton and neutron bosons that are against symmetric under a pairwise trade of protons and neutrons names. They are called Mixed-Symmetry States(MSS) [12] . The general F-turn choice run is ΔF = 0 , ± 1. Other than , the M1 progress gather between two absolutely symmetric states (F = Fmax ) are prohibited, therefor M1 change happen between low-lying aggregate states , these states must be contain segments with blended symmetry state, when ( F < Fmax ), this permits to utilize the quality of M1 progress between low-lying aggregate state and F-turn blending [13-14].
IBM-2 Parameters and Energy Spectrum

The 146-154Sm isotopes have Z=62 , the boson proton number Nπ = 6 and neutron boson Nv shift from 5 to 1 boson molecule. The parameters in table 1. regarded as a free parameters and their esteems were assessed by fitting to experimental energy level.We used the χπ = -1.2 and ζ2= +0.10 fixed for all studied isotopes,as well as to see the systematic of (ε, κ, χπ, χν, ζ2, ζ 1=3 ) parameters, ploted these parameters as a function of the neutrons number as shown in figure :1.


Table:1.The even-even 146-154Sm isotopes parameters in IBM-2

Isotope

Nv

ε

κ

χν

CLv(0,2,4)

CLπ(0,2,4)

ζ2

146Sm

1

0.999

-0.14

-0.14

-0.05, -0.05, -0.05

-0.10, -0.20, -0.28

+0.13

148Sm

2

0.959

-0.13

-0.12

-0.05, -0.05, -0.05

-0.10, -0.20, -0.09

+0.12

150Sm

3

0.910

-0.12

-0.11

-0.05, -0.05, -0.05

-0.35, -0.26, -0.15

+0.11

152Sm

4

0.763

-0.11

-0.10

-0.05, -0.05, -0.05

-0.35, -0.30, -0.19

+0.10

154Sm

5

0.620

-0.10

-0.08

-0.05, -0.05, -0.05

-0.35, -0.30, -0.19

+0.09



Figure :1.Systematic of (ε, κ, χπ, χν, ζ2, ζ 1=3 ) parameterswith neutron numbers
By and large, we watched that the (ε) parameters diminishing with neutron numbers up to mid shell and specifically relative to vitality levels, the (κ) parameter increments relatively with the expansion the neutrons number, the (χν) esteem continually expanding straightly with expanding neutron numbers. The estimations of Majorana parameters terms (ζ1,3 , ζ2) were chosen for a specific esteems and flexible with the investigation of blended symmetry states (MSS) of the vitality levels. The vitality spectra of146-154Smre delivered by utilizing the parameters in Table 1. The best fit to energized vitality levels have been watched uniquely for the ground state groups, while the semi β groups and semi γ groups it was found to have satisfactory understanding, Figure:2. demonstrates a correlation amongst hypothetical and accessible exploratory vitality levels[15-16-17-18-19] for all examined Samarium isotopes.



Figure 1. Comparison between calculated energy level and the available experimental for all considered Samarium isotopes.( 146Sm=A,148Sm=B,150Sm=C,152Sm=D, 154Sm=E)
The experimental energy ratio between (,) and (,) states which have limiting values of ( 2 , 3) for vibrator rotor, (2.5 , 4.5) for gamma-soft and 3.33, 7 for rotational symmetry respectively, we deduced that these nuclei has many dynamic symmetries, which begin close to U(5) vibrator limit for 146Sm nuclues, transition region U(5)-O(6) for 147-150Sm neuclei, but 148Sm nearly close to vibrator roter and 150Sm nearly close to gamma soft, as well as a transition limit between O(6)-SU(3) for 152Sm nucleus and finally 152Sm close to rotational limit U(3). Similar outcomes are additionally anticipated by the IBM-2 comes about, likewise to demonstrate the decent variety of the dynamic symmetries for these cores and all the more obviously, has been drawing vitality proportions (E/and E/)as a function of the number neutrons, as shown in Figure:3.


Figure 1. Thecomparison experimental ratio E/and E/ with IBM-2 result.


  1. THE MIXED SYMMETRY STATE (MSS)

At the point when think about the impact of Majorana parameter (ζ1,3 , ζ2 ) on the ascertained excitation vitality level, we settled the estimation of ζ2= +0.10for all isotopes and fluctuate theζ1,3. t is discovered that the vitality estimations of the state; , , , ,are reacted quickly to the progressions of the theζ1,3 parameters, hence these states are checked the primary property of the Mixed symmetry state (MSS). Figure:4. clarify the vitality variety of these state as an element of the Majorana parameterζ1,3.






Figure 2.variety of (MSS) as a function of the Majorana parameter ζ1,3 .( 146Sm=A,148Sm=B,150Sm=C,152Sm=D, 154Sm=E)


  1. ELECTROMAGNETIC TRANSITION


Electric quadrupole

The electromagnetic transition operator (In IBM-2,is given by [10,11].




where eπ and eνare boson effective charges, dep finishing on the boson number , those parameters are free and can take any an incentive to suit the test information. In this work, the successful charge of proton eπ = 0.0026 (eb) and neutron eν = 0.329 (eb) (got from test information of. The computed decreased electric quadrupole probabilities B(E2) of 146-154Sm isotopes are demonstrated inside the table:2. The ascertained esteems are proper in contrast with the accessible trial esteems [15-16-17-18-19] and they appearance to have a decent systematism

Table:2. The B(E2) transition of 146-154Sm isotopes , units (eb)2

Transition

146Sm

148Sm

150Sm

Exp.

IBM-2

Exp.

IBM-2

Exp.

IBM-2

21+→01+

0.0338

0.0338

0.1477

0.1451

0.2131

0.2704

02+→21+

0.0140

-----

0.0540

----

0.1166

0.2535

22+→01+

0.0013

-----

0.0140

0.0155

0.0284

0.0038

22+→21+

0.0293




0.0933




0.0770

-----

23+→21+

0.0011




0.0034

0.0008

0.0315

-----

24+→21+

0.0004




0.0046




0.0029

-----

25+→21+

0.0017

-----

0.0057




0.0013




31+→22+

0.0251




0.0999




0.1003

-----

41+→21+

0.0343

0.0091

0.2626

0.2399

0.3136

0.5216

41+→22+

0.0011




0.0021




0.0101

-----

61+→41+

0.0353

0.0438

0.1575




0.5048

0.7125

Transition

152Sm

154Sm




Exp.

IBM-2

Exp.

IBM-2







21+→01+

0.4045

0.6700

0.6437

0.9220







02+→21+

0.0316

0.1760

0.0046

0.2350







22+→01+

0.0075

0.0046

0.0181

0.0600







22+→21+

0.0102

0.0258

0.0339

0.0120







23+→21+

0.0328

0.0417

0.0125

0.0200







24+→21+

0.0021

-----

0.0096

------







25+→21+

0.0705

-----

0.0409

-----







31+→22+

0.0114

-----

0.4706

-----







41+→21+

1.0406

1.0170

0.9147

1.1860







41+→22+

0.0057

-----

0.00008

-----







61+→41+

0.6330

1.179

0.9952

1.3740








Magnetic dipole

To calculate M1 transition probability, one have to assess the successful g_ factors for proton and neutron. It is found that amid this circumstance Sambataro connection [12-13] is helpful and composed as;




where are -factors of nuclear proton and neutron separately. The aggregate�� – factor related with attractive energy, is µ=2��, and in this work we utilize the test estimation of attractive force for the 2+1state to gauge the g factor, whereµ(2+1)=2(2+1) = 0.775 (µN).it is watched that the foreseen esteems are=0.73(µN) and = 0.27(µN), and ( -) = 0.46(µN). However, the M1 operator can be written as bellow[20];




The calculated values for B(M1)is appropriate to some degree contrasting and the accessible trials esteems which may be generally not very many in atomic data sheet. The B(M1) progress of 146-154Sm isotopes is computed and exhibited in Table (3).
Table (3) The magnetic transition B(M1) of 146-154Sm isotopes, units N)2

Transition

146Sm

148Sm

150Sm

Exp.

IBM-2

Exp.

IBM-2

Exp.

IBM-2

11+→01+

----

0.00842

0.02103

----

----

0.0437

11+→02+

----

0.01449

0.02486

----

----

0.0420

31+→22+

----

0.00009

0.00005

----

----

0.00003

22+→21+

----

0.00027

0.00064

0.0082

----

0.00146

23+→21+

----

0.00099

0.00498

----

----

0.00059

24+→21+

----

0.03280

0.04233

0.0320

----

0.00036

25+→21+

----

0.00167

0.00897

0.0690

----

0.0020

Transition

152Sm

154Sm




Exp.

IBM-2

Exp.

IBM-2




11+→01+

0.09985

----

0.15349

0.0338

11+→02+

0.03869

----

0.02811

----

31+→22+

0.00006

----

0.00025

----

22+→21+

0.00063

----

0.00009

0.00004

23+→21+

0.00001

0.00134

0.00057

----

24+→21+

0.00022

----

0.01211

----

25+→21+

0.01765

----

0.22694

----


Mixing ratio δ (E2/M1)

The multipole mixing ratio between E2 and M1 transition is given as bellow [20-21];




is the transition energy between the two states units (MeV) and Δ(E2/M1) is the proportion between lessened framework component for E2 and M1 change which is communicated in the shape [21];


In Table:4. we show the estimations of the mixing ratio for for the chose Samarium isotopes in examination with the accessible exploratory esteems. It is seen that both the size and indication of δ are effectively gotten for the greater part of the chose isotopes. The assention between trial esteems and those of IBM-2 looks satisfactory in correlation with the accessible trial information.
Table:4.Mixing ratios( eb/µN )for 146-154Sm

Nucleus

Transition


Eγ (MeV)



δ(E2/M1) ( eb/µN )

Exp.

IBM-2



146Sm

22+→21+

0.9008

-----

-5.091

23+→21+

1.4087

----

+0.540

24+→21+

1.6538

----

-0.129

25+→21+

1.7970

----

+0.647

31+→22+

0.6219

---

32.36



148Sm

22+→21+

0.9039

+2.32

+4.023

23+→21+

0.9108

-----

+0.4469

24+→21+

1.1140

-0.565

-0.3488

25+→21+

1.4222

-0.556

-2.199

31+→22+

1.3535

+8.21

+3.608



150Sm

22+→21+

0.7134

-----

-4.322

23+→21+

0.8598

----

+5.250

24+→21+

1.0840

----

-2.571

25+→21+

1.4603

----

+1.003

31+→22+

1.1705

---

-5.911



152Sm

22+→21+

0.6889



+5.321

23+→21+

0.9641



-10.354

24+→21+

1.1042

----

-2.897

25+→21+

1.1709

----

-1.955

31+→22+

0.4232

---

+5.103



154Sm

22+→21+

1.0958



+17.688

23+→21+

1.2043



+22.734

24+→21+

1.3580

----

-3.1993

25+→21+

1.5919

----

+0.5643

31+→22+

0.3612

----

+13.096

  1. CONCLUSION

In the current work, we've calculated the some properties of the nuclear strucure for146-154Sm, right off the bat, recognized and accentuation some energized vitality states un certain tentatively, which get a decent understanding between the IBM-2 result and test esteems, secodary distinguished the (MSS) states(, , , ,)which got a brisk reaction while changing the Majorana parameters for these isotopes, thirdly the E2 and M1 decreased progress probabilities are ascertained and contrasted and the accessible exploratory information. At last, the estimations are reached out to δ(E2/M1) demonstrated worthy concurrence with the accessible trial information, exceptionally the indication of the blending proportion.¶

  1. REFERENCES

  1. Werner V., Pietralla N., Smith M.,"Centrifugal stretching of 170Hf in the interacting boson model", EPJ.C, 66 (2109), 2014.

  2. Baylan M., Atlihan M.,"The IBM-2 study for some even - even platinum isotopes",Turk .J. Phys., 26 , 305- 309, 2002. .

  3. Subber A. R.H.,"Nuclear structure of even-even Ge isotopes by means of interacting boson models",Turk. J. Phys., 35, 43-52, 2011.

  4. Abood S., SaadA., Kader A., L. Najim, Nuclear structure of the germanium nuclei in the interacting boson model (IBM)",J.Pure & Applied Science, 4(3):63-73, 2013.

  5. Abood S., Najim L., "Interacting boson model (IBM-2) calculations of selected even-even Te nuclei",J. Advances in Applied Science, 4(1), 444-451, 2013.

  6. Yazar H., Uluer I, ,"Some electromagnetic transition properties and mixing ratios of tellurium isotopes",International J. Physical Sciences,2(2),50-55, 2007.

  7. Jin Z., Al-Khudair F., Gui, Z., Jiang L, Dong R., " Mixed symmetry state in even-even 96-108Mo nuclei ",J.Theoretical Phys., 37(3) , 335-340, 2002.

  8. Khalat J., " Nuclear structure of even-even 104-110Mo isotopes ",J. International of scientific & engineering research, 3(12), 1-7, 2012.

  9. Mahdi A., Al-Khudair F., Subber A., "Identification of mixed symmetry state in 180-186 W isotopes in framework of IBM-2",International. J. Phys., 4(5),2250-2230, 2014.

  10. Al-Khudair F.,Subber A., Ashwaq F, "Bands structure and electromagnetic transitions of O(6) nucleus 128Xe" J, Basrah Researches Sciences ,40(1), 49-60, 2014.

  11. Yazar H., Uluer I., "A correspondence between IBA-1 and IBA-2models and electromagnetic transitions in the decayof some erbium isotopes", J. Pramana Phys., 65(3), 393 – 402, 2005.

  12. Al-KhudairF., Jin Z.,HongB., Chinese Phys., 2009, 33(1), 46.

  13. Al-KhudairF., Subber A., JaaferA.,J. Basra Science, 2014, 40 (1), 46.

  14. JinZ.,Al-KhudairF., Gui L., Jiang Z., Dong R., Theo. Phys.,2002, 37(3),335.

  15. L. K. Pekerand J. K. Tuli, Nuclear Data Sheets for A = 146*, USA, 1997, 82, 178.

  16. N. Nica, Nuclear Data Sheets for A = 148, sciencedirect., 2014 , 117,1–229.

  17. S. K. Basu, Nuclear Data Sheets for A = 150, sciencedirect., 2013, 114,345–660.

  18. M. J. Martin,Nuclear Data Sheets for A = 152*, sciencedirect., 2013, 114,1197–1487.

  19. C. W. Reich, Nuclear Data Sheets for A = 154*, sciencedirect., 2009, 110,2257–2532.

  20. Ashij A., "The δ (E2/M1) mixing ratio and X (E0/ E2) ratio of transitions in some of samarium isotopes", J. Al-Anbar for pure science, 1(3), 1991-8941, 2007.[21] Subber A., Al-Khudair F.,"δ(E2/M1) and X(E0/E2) mixing ratios in 134Ba by means of IBM-2",Turk. J. Phys., 36 , 368-376, 2012


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