Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV

The simultaneous least-square fit of expressions for differential cross-sections and asymmetry to the experimental data on dσ/dΩ and Σ(θ), obtained at NSC KIPT, was realized. A set of three bilinear equations with three unknown amplitude modules | ³P₁ | E1, | ³S₁ | M1 and | ³D₁ | M1 was derived; pre...

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Published in:Вопросы атомной науки и техники
Date:2002
Main Authors: Lyakhno, Yu.P., Gorbenko, E.S., Dogyust, I.V.
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Language:English
Published: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2002
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/80106
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Cite this:Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV / Yu.P. Lyakhno, E.S. Gorbenko, I.V. Dogyust // Вопросы атомной науки и техники. — 2002. — № 2. — С. 22-24. — Бібліогр.: 8 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Lyakhno, Yu.P.
Gorbenko, E.S.
Dogyust, I.V.
author_facet Lyakhno, Yu.P.
Gorbenko, E.S.
Dogyust, I.V.
citation_txt Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV / Yu.P. Lyakhno, E.S. Gorbenko, I.V. Dogyust // Вопросы атомной науки и техники. — 2002. — № 2. — С. 22-24. — Бібліогр.: 8 назв. — англ.
collection DSpace DC
container_title Вопросы атомной науки и техники
description The simultaneous least-square fit of expressions for differential cross-sections and asymmetry to the experimental data on dσ/dΩ and Σ(θ), obtained at NSC KIPT, was realized. A set of three bilinear equations with three unknown amplitude modules | ³P₁ | E1, | ³S₁ | M1 and | ³D₁ | M1 was derived; preliminary data about the magnitudes of these amplitude modules were obtained. It is shown that the ³D₁ М1 am­p­li­tu­de is the highest in magnitude.
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fulltext SPIN-TRIPLET TRANSITIONS IN (γ,p) AND (γ,n) REACTIONS OF TWO-BODY 4He DISINTEGRATION BY PHOTONS OF ENERGIES BELOW 80 MeV Yu.P. Lyakhno, E.S. Gorbenko, I.V. Dogyust National Science Center “Kharkov Institute of Physics and Technology”, Kharkov, Ukraine The simultaneous least-square fit of expressions for differential cross-sections and asymmetry to the experimental data on dσ/dΩ and Σ(θ), obtained at NSC KIPT, was realized. A set of three bilinear equations with three unknown amplitude modules 3P1 E1, 3S1 M1 and 3D1 M1 was derived; preliminary data about the magnitudes of these amplitude modules were obtained. It is shown that the 3D1 М1 amplitude is the highest in magnitude. PACS: 25.20.Dc; 29.27.Hj; 29.40. Cx INTRODUCTION The interest in the studies of two-body (γ,р) and (γ ,n) reactions of 4Не disintegration by low energy pho- tons is determined by their relatively simple spin struc- ture and a small number of particles participating in the reaction. On the one hand, this makes possible a more detailed theoretical calculation with a minimum of mo- del assumptions introduced. On the other hand, the laws of conservation of the total momentum and parity sig- nificantly restrict the number of multipole transitions participating in the reaction. Neglecting the contribu- tions of higher multipoles which correspond to high to- tal- momentum values of the photon, one can determine to sufficient accuracy the amplitudes of the basic multi- pole transitions. This makes possible the comparison be- tween the theoretical calculations and the experime- ntally measured multipole amplitudes. This comparison is of great importance because each of the multipole transitions can be governed by different reaction mecha- nisms. It should be also noted that for the low particle energy range there exist the phase-analysis data on elastic (N,T) scattering. These data can be used for theoretical calculations of photodisintegration reactions on 4He. The laws of conservation of the total momentum and parity at two-body (γ,р) and (γ,n) disintegration of 4Не in Е1, Е2 and М1 approximations permit six multipole amplitudes: 1P1 Е1, 1D2 Е2, 3P1 Е1, 3D2 Е2, 3S1 М1 and 3D1 М1 (in spectroscopic notation). At present, only the values of the first two amplitudes with ∆S=0 are deter- mined. The analysis of experimental data has revealed that in the low photon energy region it is the electric di- pole E1 transition that is dominant, and the next in prominence is the Е2 transition with ∆S=0. These transitions occur without any change in the final-state spin ∆S=0, the remaining four transitions take place with changing the spin ∆S=1. Unfortunately, no evi- dence for the amplitudes of the processes with ∆S=1, obtained from the direct reactions, can be found in the literature, and the data gained from the inverse reactions are available only for low photon energies (Е γ < 30 MeV). Moreover, most of the data are contradictory. Wagenaar etal. [1] have investigated the radiative capture of polarized protons of energies Tp between 0.8 and 9 MeV by tritium nuclei. Those authors have come to the conclusion that the cross-section for the reaction with ∆S=1 is mainly contributed by the magnetic dipole M1 transition. The investigation [2] of the same reaction with a polarized proton beam at Tр=2 MeV has led the investigators to the conclusion that the dominant amplitude in the ∆S=1 transitions is 3P1 Е1. It has been reported in ref. [3] that the cross- section for the M1 transition in 3Не(n,γ)4Не is extremely low at thermal neutron energies, and also on extrapola- tion of the data to the nucleon energy range of a few MeV [2]. In view of this, an additional experime- ntal information on the nature of ∆S=1 is needed. The NSC KIPT team has obtained the most comprehensive experimental data on both the differential cross-sections [4] and the azimuthal cross-sectional asymmetry Σ(θ) of (γ,р) and (γ,n) reactions [5,6], that enables one to derive new information on the transitions with ∆S=1. In this paper we report our preliminary results from the multipole analysis of these data. MULTIPOLE ANALYSIS The differential cross-section can be expressed in terms of multipole transition amplitudes as follows: d d A σ θ β θ γ θ ε θ ν Ω = ⋅ + + + + 2 2 2 32 1[sin ( cos cos ) cos ], (1) where 22 PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. 2002, № 2. Series: Nuclear Physics Investigations (40), p. 22-24. A P E P E D M D E D M S M D E S M D E D M = − + − − + +∗ ∗ ∗ 18 1 9 1 9 1 25 2 18 2 1 1 30 6 2 1 30 3 2 1 1 1 2 3 1 2 3 1 2 3 2 2 3 1 3 1 3 2 3 1 3 2 3 1 Re( ) Re( ) Re( ) (2) β = −∗ ∗[ Re( ) Re( )]60 3 2 1 60 2 11 2 1 1 3 2 3 1D E P E D E P E A (3) γ = −[ ]150 2 100 21 2 2 3 2 2 D E D E A (4) ε = − − +∗ ∗ ∗ [ Re( ) Re( ) Re( )] 12 6 1 1 12 3 1 1 60 2 1 3 1 3 1 3 1 3 1 3 2 3 1 S M P E D M P E D E P E A (5) ν = + + + + − −∗ ∗ ∗ [ Re ( ) Re( ) Re( )] 18 1 12 1 6 1 50 2 12 2 1 1 20 6 2 1 20 3 2 1 3 1 2 3 1 2 3 1 2 3 2 2 3 1 3 1 3 2 3 1 3 2 3 1 P E S M D M D E D M S M D E S M D E D M A (6) In the approximation used here, Eqs. (2) to (6) allow the determination of only five relationships between the multipole transition amplitudes from the differential cross-section. It can be demonstrated that the azimuthal cross- sectional asymmetry Σ(θ) is given by the expression Σ ( ) sin ( cos cos ) sin ( cos cos ) cos θ θ α β θ γ θ θ β θ γ θ ε θ ν = + + + + + + + 2 2 2 2 1 1 , (7) where: α = − + + − − ∗ ∗ ∗ [ Re( ) Re( ) Re( )] 18 1 50 2 36 2 1 1 20 6 2 1 20 3 2 1 3 1 2 3 2 2 3 1 3 1 3 2 3 1 3 2 3 1 D M D E D M S M D E S M D E D M A (8) Thus, the data on Σ(θ) permit the determination of an additional relationship between the amplitudes of multipole transitions; it is specified by expression (8). The coefficients А, α, β, γ, ε and ν were calculated by the least-squares method (LSM) from the fit of expressions (1) and (7) to the experimental data histog- rammed with a bin value of 10°. It should be noted that for determination of cross-sections for low multipole amplitudes some experimental errors must be taken into account. In particular, the calculated cross-section in the collinear geometry, entering into the coefficient ν, can depend on the bin value of the differential cross-section, and also on the resolution of measuring device in the polar angle of nucleon emission. Besides, the calculated multipole amplitude values can appear to be biased as a result of using the LSM. Strictly speaking, this method is applicable only with a great body of statistics in each bin, this being not fulfilled in the case of reactions under study in the vicinity of the angles θn∼0°, 180°. The corresponding corrections were calculated through the Monte-Carlo simulation of the differential cross-section. The values of the parameters calculated by expression (1) were used as initial. More exact values of the para- meters were calculated by averaging over 1000 simula- tions using the relation L L Li i im= −2 0 , (9) where i is the parameter number, Li0 is the parameter value computed by the LSM, Lim is the average para- meter value computed by the LSM. The computed values are listed in Table 1 and Table 2 for the 4He(γ,p)T and 4He(γ,n)3He reactions, res- pectively. The existing experimental data are not sufficient to determine the cross-sections of all the mentioned tran- sitions, and also the interference terms. In the first variant of the analysis it was supposed that the lowest of the ∆S=1 amplitudes under discussion is 3D2 Е2, and the terms involving this amplitude were neglected. It is known [7] that Е1 and М1 transitions are isovectoral. This enables us to determine the phase differences between 3P1 Е1, 3S1 М1 and 3D1 М1 amplitudes from the phase analysis data for the elastic scattering of protons by 3Не nuclei, available [8] in the energy range from 35 to 59 MeV. Table 1. Fitting coefficients for (γ,p) reactions on 4He for three intervals of photons energy Coef- fic. Eγ=34-46 MeV Eγ=46-65 MeV Eγ=65-90 MeV А β γ ε ν α χ2 d.o.f. 87.98±1.55 0.76± 0.03 0.43±0.06 0.014±0.005 0.030±0.005 -0.16±0.09 1.2 29.91±0.75 1.15±0.05 0.85±0.10 0.008±0.006 0.018±0.006 -0.15±0.1 1.4 13.4±0.4 1.06±0.06 0.88±0.12 0.003±0.008 0.019±0.008 -0.10±0.14 1.16 Table 2. Fitting coefficients for (γ,n) reactions on 4He for three intervals of photons energy Coef- fic. Eγ=34-46 MeV Eγ=46-65 MeV Eγ=65-90 MeV А β γ ε ν α χ2 d.o.f 85.6±1.31 -0.08±0.03 0.62±0.06 0.002±0.004 0.027±0.004 -0.10±0.11 1.18 33.63±0.84 0.152±0.044 0.76±0.10 0.013±0.006 0.018±0.007 -0.28±0.11 1.26 14.9±0.46 0.35±0.06 0.83±0.13 0.008±0.008 0.027±0.009 -0.08±0.14 1.06 Thus, the coefficients А, β and γ are also used to calculate the amplitude modules 1P1 E1 and 1D2 E2, and also the phase differences δ(1Р1)-δ(1D2). The remaining relationships for α, ε и ν represent a set of three bilinear equations with three unknown amplitude modules 3P1 E1,3S1 M1 and3D1 M1: α δ δ= − + −[ cos( ( ) ( ))]18 1 36 2 1 13 1 2 3 1 3 1 3 1 3 1D M D M S M S D A ε δ δ δ δ = − − − − [ cos( ( ) ( )) cos( ( ) ( ))] 12 6 1 1 12 3 1 13 1 3 1 3 1 3 1 3 1 3 1 3 1 3 1 S M P E S P D M P E P D A 23 ν δ δ = + + − [ cos( ( ) ( ))] 18 1 12 1 12 2 1 13 1 2 3 1 2 3 1 3 1 3 1 3 1 P E S M D M S M S D A (10) The experimental data on the coefficients α0, ε0 and ν0 have appeared such that the set (8) had no solutions. Therefore, the set was solved for the following values of the coefficients: α α α ε ε ε ν ν ν = + = + = + 0 0 0 k k k ∆ ∆ ∆ (11) where ∆α, ∆ε and ∆ν are the statistical errors of the corresponding coefficients, and к takes on the lowest possible value. In this case, the set has two positive so- lutions. However, at кmin≠0 these solutions coincide. The solution of the set was determined in the range of one standard deviation (k≤1). The computational results are presented in Table 3 and Table 4 for 4Не(γ,n)3He and 4Не(γ,p)T reactions, respectively. It is evident from the tables that it is the 3D1 М1 amplitude that has the highest value. In the subsequent analysis it was assumed that 3D2 E2>>3D1M1. From expression (8) it is obvious that in this case there should be α≥0, and this does not agree with the experimental data. Table 3. The computed amplitude module ratios for 4Не(γ,p)T reactions for two photon energy ranges Ratios of amplitude modules Eγ=34 -46 MeV Eγ=46 – 65 MeV  3 D 1 2 M1 1 P12E1 0.054±0.03 0.046±0.03  3 S 1 2 M1 1 P12E1 0.022±0.02 0.005±0.02  3 P 1 2 E1 1P12E1 0.010±0.02 0.008±0.02 Table 4. The computed amplitude module ratios for 4Не(γ,n)3He reactions for two photon energy ranges Ratios of amplitude modules Eγ= 34 – 46 MeV Eγ=46 – 65 MeV  3 D 1 2 M1 1P12E1 0.051±0.03 0.092±0.04  3 S 1 2 M1 1P12E1 0.011±0.02 0.024±0.03  3 P 1 2 E1 1P12E1 0.003±0.02 0.005±0.02 CONCLUSIONS The data on the cross-section asymmetry Σ(θ) make it possible to derive an additional relationship between the amplitudes of multipole transitions. A simultaneous least-square fit of expressions for differential cross- sections and asymmetry to the experimental data on dσ /dΩ and Σ(θ), obtained at NSC KIPT, was realized. To extract the information about the cross-sections of ∆S=1 transitions, a set of three bilinear equations with three unknown amplitude modules 3P1 E1, 3S1 M1 and 3D1 M1 has been set up, and the preliminary data on the values of these amplitude modules have been obtained. It is shown that the 3D1 М1 amplitude is the highest in value, and accordingly, σ(М1)>> σ(3P1 Е1). The experimental data on the azimuthal cross-sectional asymmetry of (γ,p) and (γ,n) reactions show that the main contribution to the cross-section of transitions with spin variation comes from the M1 transition. A consi- derable cross-section of the М1 transition may be due to the contribution of wave function components of the 4Не nucleus with nonzero orbital moments of nucleons. ACKNOWLEDGMENT The authors are grateful to P.V. Sorokin, L.G. Levchuk, V.N. Gur'ev, A.F. Khodyachikh for the discussion of present results. REFERENCES 1. D.J. Wagenaar, N.R. Robertson, H.R. Weller and D.R. Tilley. Evidence for M1 strength in the 3He(p,γ)4He reactions // Phys. Rev. C. 1989, v. 39, №2, p. 352-358. 2. W. Pitts. Spin-triplet strength in the 3He(p,γ) 4He reactions at Ep=2 MeV // Phys. Rev. C. 1992, v. 46, №1, p. 15-19. 3. R. Werwelman, K. Abrahams. Nucleon captures by 4He and the production of solar hep -neutrons. Cross-section measurement and shell- model calculation // Nucl. Phys. A. 1991, v. 526, p. 265-291. 4. Yu.M. Arkatov et al. Photodisintegration of 4He nuclei below meson production threshold // UFZh. 1978, v. 23, №11, p. 1818-1023 (in Russian). 5. V.B. Ganenko et al. Two-body photodisinteg- ration of 4He by linearly polarized γ-quanta // Problems of Atomic Science and Technology: ser. Nuclear-physical studies (theory and experiment). 1989, iss. 8(8), p. 64 (in Russian). 6. Yu.P. Lyakhno et al. Measurement of angular dependence of the asymmetry of cross-sections for 4He(γ,p)T and 4He(γ,n)3He reactions induced by 40, 60 and 80 MeV linearly polarized photons // Yad. Fiz. 1996, v 49, №5, p. 18-22 (in Russian). 7. B.T. Murdoch, D.K. Hasell, A.M. Sourkes et al. 3He(p,p) scattering in the energy range 19- 48 MeV // Phys. Rev. C. 1984, v. 29, p. 2001-2008. 8. J.M. Eisenberg and W. Greiner. Nuclear Theory, Mechanisms of the nucleus v.2. Amsterdam, 1970, 345 p. 24 PACS: 25.20.Dc; 29.27.Hj; 29.40. Cx
id nasplib_isofts_kiev_ua-123456789-80106
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1562-6016
language English
last_indexed 2025-12-02T09:00:33Z
publishDate 2002
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
record_format dspace
spelling Lyakhno, Yu.P.
Gorbenko, E.S.
Dogyust, I.V.
2015-04-11T19:26:29Z
2015-04-11T19:26:29Z
2002
Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV / Yu.P. Lyakhno, E.S. Gorbenko, I.V. Dogyust // Вопросы атомной науки и техники. — 2002. — № 2. — С. 22-24. — Бібліогр.: 8 назв. — англ.
1562-6016
PACS: 25.20.Dc; 29.27.Hj; 29.40. Cx
https://nasplib.isofts.kiev.ua/handle/123456789/80106
The simultaneous least-square fit of expressions for differential cross-sections and asymmetry to the experimental data on dσ/dΩ and Σ(θ), obtained at NSC KIPT, was realized. A set of three bilinear equations with three unknown amplitude modules | ³P₁ | E1, | ³S₁ | M1 and | ³D₁ | M1 was derived; preliminary data about the magnitudes of these amplitude modules were obtained. It is shown that the ³D₁ М1 am­p­li­tu­de is the highest in magnitude.
The authors are grateful to P.V. Sorokin, L.G. Levchuk, V.N. Gur'ev, A.F. Khodyachikh for the discussion of present results.
en
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
Вопросы атомной науки и техники
Nuclear reactions
Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
Спин-триплетные переходы в реакциях (γ,p) и (γ,p) двухчастичного расщепления ядра ⁴Не при энергиях ниже 80 МэВ
Article
published earlier
spellingShingle Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
Lyakhno, Yu.P.
Gorbenko, E.S.
Dogyust, I.V.
Nuclear reactions
title Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
title_alt Спин-триплетные переходы в реакциях (γ,p) и (γ,p) двухчастичного расщепления ядра ⁴Не при энергиях ниже 80 МэВ
title_full Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
title_fullStr Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
title_full_unstemmed Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
title_short Spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴He disintegration by photons of energies below 80 MeV
title_sort spin-triplet transitions in (γ,p) and (γ,n) reactions of two-body ⁴he disintegration by photons of energies below 80 mev
topic Nuclear reactions
topic_facet Nuclear reactions
url https://nasplib.isofts.kiev.ua/handle/123456789/80106
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