Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters

We present the analytic review of π⁺ and π⁰ mesons photoproduction off the proton target as the only source of information about the Δ⁺(1232) resonance parameters. The review focuses at the estimation of the influence of different contributions to the experimental database on determination of the E2...

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Автор: Omelaenko, A.S.
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Опубліковано: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2003
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Цитувати:Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters / A.S. Omelaenko // Вопросы атомной науки и техники. — 2003. — № 2. — С. 39-44. — Бібліогр.: 29 назв. — англ.

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spelling irk-123456789-1105992017-01-06T03:02:33Z Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters Omelaenko, A.S. Nuclear reactions We present the analytic review of π⁺ and π⁰ mesons photoproduction off the proton target as the only source of information about the Δ⁺(1232) resonance parameters. The review focuses at the estimation of the influence of different contributions to the experimental database on determination of the E2/M1 ratio for γp→Δ⁺ transition and the resonance parameters, with discussion of the previous Kharkov results. Представлено аналітичний огляд фотонародження π⁺ та π⁰ мезонів на протонній мішені як єдиного джерела інформації про параметри Δ⁺(1232)-разонанса. Огляд фокусується на оцінці впливу різних вкладів в экспериментальну базу даних на визначення E2/M1-відношення для γp→Δ⁺ переходу і параметрів резонанса, з обговоренням отриманих раніше в Харкові результатів. Представлен аналитический обзор фоторождения π⁺ и π⁰ мезонов на протонной мишени как единственный источник информации о параметрах Δ⁺(1232)-разонанса. Обзор фокусируется на оценке влияния различных вкладов в экспериментальную базу данных на определение E2/M1-отношения для γp→Δ⁺ перехода и параметров резонанса, с обсуждением полученных ранее в Харькове результатов. 2003 Article Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters / A.S. Omelaenko // Вопросы атомной науки и техники. — 2003. — № 2. — С. 39-44. — Бібліогр.: 29 назв. — англ. 1562-6016 PACS: 13.75Gx http://dspace.nbuv.gov.ua/handle/123456789/110599 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
topic Nuclear reactions
Nuclear reactions
spellingShingle Nuclear reactions
Nuclear reactions
Omelaenko, A.S.
Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
Вопросы атомной науки и техники
description We present the analytic review of π⁺ and π⁰ mesons photoproduction off the proton target as the only source of information about the Δ⁺(1232) resonance parameters. The review focuses at the estimation of the influence of different contributions to the experimental database on determination of the E2/M1 ratio for γp→Δ⁺ transition and the resonance parameters, with discussion of the previous Kharkov results.
format Article
author Omelaenko, A.S.
author_facet Omelaenko, A.S.
author_sort Omelaenko, A.S.
title Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
title_short Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
title_full Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
title_fullStr Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
title_full_unstemmed Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters
title_sort kharkov data on pion photoproduction and δ⁺(1232) resonance parameters
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
publishDate 2003
topic_facet Nuclear reactions
url http://dspace.nbuv.gov.ua/handle/123456789/110599
citation_txt Kharkov data on pion photoproduction and Δ⁺(1232) resonance parameters / A.S. Omelaenko // Вопросы атомной науки и техники. — 2003. — № 2. — С. 39-44. — Бібліогр.: 29 назв. — англ.
series Вопросы атомной науки и техники
work_keys_str_mv AT omelaenkoas kharkovdataonpionphotoproductionandd1232resonanceparameters
first_indexed 2025-07-08T00:50:05Z
last_indexed 2025-07-08T00:50:05Z
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fulltext KHARKOV DATA ON PION PHOTOPRODUCTION AND ∆+(1232) RESONANCE PARAMETERS A.S. Omelaenko National Science Center “Kharkov Institute of Physics and Technology”, Kharkov, Ukraine We present the analytic review of π+ and π0 mesons photoproduction off the proton target as the only source of information about the ∆+(1232) resonance parameters. The review focuses at the estimation of the influence of different contributions to the experimental database on determination of the E2/M1 ratio for γp→∆+ transition and the resonance parameters, with discussion of the previous Kharkov results. PACS: 13.75Gx 1. INTRODUCTION The successful experiment on lithium splitting on 10 October 1932 was the initiating event followed by the entire chain of long-term developments in the atomic science in Kharkov and Former Soviet Union. As one of the consequences, 33 years later the 2 GeV electron linac was built in Kharkov, under direction of K.D. Sinel’nikov and A.K. Val’ter − two participants of the “high-voltage brigade” which had split up the lithium nuclei. Unfortunately the following pulse stretcher ring project left unrealized and performing the coincidence experiments turned out to be very compli- cated. As the result the single pion photoproduction on proton happened to be practically the only one elementary process thoroughly studied in Kharkov. In particular, in the region of excitement of the first nucleon resonance there were carried out numerous measurements of asymmetry Σ in reactions with linearly polarized photons [1,2]. The first round of successful experiments using the polarized proton target in addition [3,4] (see also article [5] in this issue) was the most important result of these measurements. The new information obtained in these experiments made it possible to solve problem of the unique solution in the energy independent multipole analysis using some plausible stabilization procedure [6], and next without any additional conditions [7]. The most interesting and theoretically important result of such a multipole analyses is determination of the resonance radiative decay amplitudes, in particular the ratio EMR of the electric quadroupole E2 and magnetic dipole M1 amplitudes. The deviation of EMR from 0 is evidence in favor of the existence of color magnetism due to the gluon exchange between quarks. The EMR value plays a role of the litmus paper for hadron models that predict this ratio to be quite small with values ranging between –0.5% and –6% [8]. From the Kharkov data EMR was obtained with the range of − (1.2 ... 1.3)% [9]. However, later on and especially in the last decade the database has considerably expanded. In addition, the EMR happened to be very sensitive to some inconsis- tencies in the database [10]. The present-day EMR value is determined in many works [11], approximately with the results being at least twice-larger then those obtained in [9] (in recent work [12] EMR = =− [3.07 ± 0.26(stat + syst) ± 0.24(model)]%). The reason of this contradiction can be understood from article [10] where the model dependence and the influence of choice of database in extracting the ∆(1232) electro- magnetic transition amplitudes were investigated. In particular, the crucial correlation between the Bonn π0 cross section data [13] and the EMR was demonstrated. The strong influence of this data on the extracted EMR has also been confirmed by the LEGS group [14,12]. The mass splitting of the different ∆ charge states is another problem associated with the Kharkov data. Indeed, the πN scattering analyses has given the ∆0 and ∆++ masses, characteristic values being 1233.6±0.5 MeV and 1230.9±0.3 MeV respectively [11] (PDG)). The missing ∆+ mass can be obtained only from the single pion photoproduction reactions on proton, by the resonance fitting of the multipoles leading to the final π N state with isotopic spin T = 3/2 and total momentum J=3 /2 at condition that the Watson’s theorem is not used. The ∆+ mass value 1234.9±1.4 MeV was obtained by authors of work [15] (MIROSHNIC 79 in PDG) from the results of their preceding energy independent analysis with ‘free’ imaginary part of the magnetic dipole resonant amplitude [16]. But it has been a concern that this ∆+ mass is inconsistent with ∆++ and ∆0 masses cited above. In particular, this issue was the subject of a special publication [17], where it has also been emphasized that a similar problem arises in any analysis starting from multipoles determined in a separate analysis. The purpose of this mini-review is to shed some light on the problems with both the Kharkov EMR and ∆ + mass value, with paying a special attention to the Kharkov data. We have invoked a realistic resonance model approbated in our contribution to [18] and fulfilled a series of retrospective fits beginning from the data since 1990 and scaling down by degrees the year of the data involved. It turned out that the Bonn’s cross sections mentioned above have a strong influence not only on the EMR, but also on the ∆+ mass. PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. 2003, № 2. Series: Nuclear Physics Investigations (41), p. 39-44. 39 2. REMARKS ON THE DATABASE Several years ago the full collection of the Kharkov data on single pion photoproduction was uploaded to the public-available compilation SAID [19,20]. In connec- tion with this we have ceased replenishment of our own database using the results of the vast work undertaken by the authors of SAID. Now the Kharkov data are well accessible and up to this time they are used in the multipole analyses, for example, [12,21]. An essential feature of the SAID compilation is that it contains all accumulated data being verified by direct contacts with numerous authors, without any preliminary selection according to somebody’s preferences. As a result, the database contains some conflicting measurements, but there is a possibility to investigate the influence of these discrepancies on the results of any specific multipole analysis. 3. FORMALISM IN THE ∆(1232) REGION Our analysis was carried out in terms of the Walker’s helicity multipoles BAM I l I l I l ±±≡± , with the following isospin structure of the π0 and π+ photo- production on proton [22]: A1/2 = 1/3 A(π0) + √2/3 A(π+), (1) A3/2 = A(π0) − 1/√2 A(π+). (2) The starting point of the model used is the following expression for the resonant multipoles obtained in the K-matrix approach [23] as result of the unitary merging of the background and the ‘pure’ resonance: .sincos 3333 3333 2/3 1 eReBM iRPURE M iBORN M δ+δ= δδ+ (3) In Eq. (3) BBORN M is the background function (in [23] this is the Born contribution to the resonant multipole), RPURE M is responsible for the resonance photoexcitation. The full phase shift δ33 for the P33 wave in the πN scattering is the sum of the background δ B 33 and the ‘pure’ resonance phase shift δ R 33 : δδδ += RB 333333 . (4) To fully demonstrate the dependence on δ33, which is the main focus of our interest, Eq. (1) can be written as eReBM i M i M δδ+δδ=+ 3333 3333 2/3 1 sincos , (5) with ,sin 33δ−= BPURE M BORN MM RBB (6) .cos 33δ= BPURE MM RR (7) Eq. (5) is the base of our treatment of the resonant multipoles. The elastic background phase shift appears not only as a component part of δ33 but also has an additional influence on the redefined excitation func- tions (6,7). These corrections are expected be small and smooth, keeping in mind evaluations of the background phase shift for the mixed charge δ33. There is no possibility to determinate the elastic background phase shift by using Eqs. (6,7) because the corresponding trigonometric functions are multiplied by other unknown smooth functions. So, the whole function BM was parameterized through the Lagrange interpolation formula (Eγ being the laboratory photon energy): ,)()()()( )()( 4 )(1 )( 4 1 )( ji j ijj j i i i EEEEEBEB γγ = ≠= γγ = = γγ −−= ∏∑ (8) with four knot energies and with coefficients being the knot values of the function. In a special test it has been compared to the relevant cubic spline without the first derivatives specified at the ends, and Eq. (8) happened to be preferable for extrapolating out of the energy interval restricted by the extreme knots. The full phase shift δ33 in (5) is chosen in accordance with the standard Breit-Wigner formula: WW WWtg 22 0 0 33 )( − Γ=δ (9) with 22 2 0 23 0 0)( qX qX q qW + +     Γ=Γ , (10) where q is the c.m. momenta of the pion, q0 is the corresponding quantities at W0. Here W0 (the mass) is the value of the total c.m. energy W at which δ33 passes though 90°, and the width is Γ0 = 2/(dδ33/dW)W=M0 (‘experimental’ values). Eq. (9) corresponds to the approach without introduction the explicit background at all, and a precaution about BM seems to be excessive, as well. Accordingly, these definitions are the same as in πN phase shift analysis [24] (KH80) at determination of the ∆++ and ∆0 parameters, where “some guess for uncertainty due to the non-resonant background are simply added to the quoted errors”. The last term in Eq. (5) corresponds the to resonance contribution. It is introduced according to Walker [22]: Γ−− ΓΓ = γ + WiWW W kq qkWCWM M R 0 22 0 000 0 ,2/3 1 )()( . (11) Here )(Im 0 ,2/3 1 WM RC M +≡ is the resonance constant, 22 2 0 23 0 0)( kX kX k kW + +     Γ=Γ λ , (12) where k is the c.m. momenta of the photon, k0 is the corresponding quantities at W0. Expression (8) is used also to describe the real parts of the variable non-resonant multipoles, other background multipoles up to l=3 are taken as full Born approximation, and the corresponding imaginary parts are calculated according to the Watson’s theorem: ).(ReIm )(2,2δ= ±±± lI I l I l tgMM (13) The resonance constant in Eq. (11) refers to the ex- perimental resonance in the meaning discussed above. For parameterization with some realistic non-zero back- ground phase shift the arguments can be provided in such a way that the resonance constant would be very close to the ‘pure’ one (see [9] and discussion of this 40 work in [25]). Especially, we can expect that for the resonance ratio E2/M1 where reduction of the energy dependence is also expected. 4. RETROSPECTIVE MULTIPOLE ANALYSIS To concentrate calculations in the ∆+ region we have treated the data at the photon energy interval 260- 420 MeV. The energies 280, 320, 360, and 400 MeV were taken as knot energies in Eq. (8). The necessary for Eq. (13) πN scattering phase shifts were calculated according the recent πN analyses [26] (SM02 in SAID). The data were fitted by minimizing the standard χ2 without introducing rating factors for any type of observable. The main set of independent variables included the ∆+ mass M0 and width Γ0 (parameter X was fixed at the Walker’s value 185 MeV) and the knot values from Eq. (8) used for the following functions: (a) the background functions BA, BB in Eq. (5) for the resonant multipoles; (b) the real parts of the non- resonant multipoles A0+, A1- with isotopic I = 1/2,3/2, A1+, B1+ with I = 1/2 (s,p waves), and A2-, B2- with I = 1/2 to account the possible ‘tail’ of the second resonance. The results obtained for several series of fits with the data from different years are presented in Table 1. The first fit was obtained using the new data obtained from 1990. This data set practically corres- ponds to the BRAG low energy set [18]. As in [18] we were unlucky to describe the preliminary π0 cross section HA97MA* from Mainz (our data labels contain two letters of the first author and the laboratory name being separated by the reduced year). In addition, there is a problem with the LEGS differential cross sections (BL01LE, π0 and π+ production). The corresponding χ 2 dp ≡ χ2/N (N is the number of points) are too large, and that needs special consideration. In preliminary calcu- lations the normalization factors being introduced as additional free parameters for the both LEGS cross sections were about 0.9, but only for the π0 production it was possible to get reasonable χ2 dp ≈ 2.6. Consequently we have omitted these data in the initial data set (group I in Table 2, χ2 in this table are calculated according to our final solution discussed below). Table 1. ∆+ Parameters for different variants of the resonance model № Vari- ants Year Excluded data EMR, % M0, MeV Γ0, MeV N χ2 df 1 2 3 4 5 6 7 8 9 1 0 Main set 1990 I -2.2 ± 0.2 1232.3 ± 0.8 117.1 ± 2.9 1339 1.59 1985 I -2.2 ± 0.2 1232.7 ± 0.8 117.2 ± 2.9 1343 1.60 1980 I -2.2 ± 0.1 1231.5 ± 0.6 113.5 ± 2.1 1762 1.80 1980 I,II -2.2 ± 0.1 1232.0 ± 0.6 114.1 ± 2.2 1758 1.78 1975 I,II -2.7 ± 0.1 1232.0 ± 0.5 111.3 ± 1.9 2152 2.35 1975 I-III -2.6 ± 0.1 1231.7 ± 0.5 112.1 ± 2.0 2113 2.15 1970 I-III -1.6 ± 0.1 1234.7 ± 0.4 117.3 ± 1.7 2997 2.30 1970 I-IV -1.6 ± 0.1 1234.7 ± 0.4 117.5 ± 1.7 2992 2.28 1970 I-V -2.5 ± 0.1 1232.0 ± 0.5 111.6 ± 1.7 2660 2.05 1960 I-VI -2.5 ± 0.1 1232.1 ± 0.4 113.0 ± 1.7 3225 2.24 1 1 s,p 1960 I-VI -2.2 ± 0.1 1232.4 ± 0.5 117.7 ± 1.8 3225 2.41 1 2 s,p,d 1960 I-VI -2.6 ± 0.1 1233.0 ± 0.5 113.0 ± 2.1 3225 2.13 Table 2. Characteristics of the deleted data G. R O Label N Eγ, MeV ϑ, deg χ2 dp I π0 σ HA97MA * 51 283-402 10.0-170.0 13.5 π+ σ BL01LE 48 265-322 20.0-170.0 25.7 π0 σ BL01LE 49 265-334 70.0-130.0 12.5 II π+ G BL84KH 4 320-380 65.0-80.0 9.9 III π+ Σ GN76KH 32 280-420 25.0-140.0 10.2 π0 Σ GB77KH1 4 280-400 75.0-120.0 43.5 π0 σ JU76BO 2 373-416 89.4-90.9 7.6 IV π+ Σ ZD72ST 2 390-408 135.0 19.3 π0 σ HE73TO 3 350-420 4.4-6.1 7.8 V π0 σ GZ74BO1 332 260-420 10.0-160.0 6.9 VI π+ σ KN63UC 23 260-290 0-160 8.5 π+ Σ LU64ST 3 330 45-135 34.4 Note: R − reaction, O − observable value Table 3. χ2 per point for different values for fit 10 Reaction dσ/d Ω Σ T P γp→π+n 2.26 1.82 1.66 1.35 γp→πop 2.55 2.47 3.31 1.93 By decreasing the initial year down to 1975 we exclude some other non-numerous data (groups II-IV in Table 2) with per degree of freedom exceeding 9. There were observed rather stable values of the resonance parameters with acceptable values of χ2 df. But appearing in the current compilation of the numerous π0 cross section data resulting from some experimental setups at Bonn [13] (GZ74BO) caused the striking effect. In particular the ∆+ mass exceeding the ∆0 value known from scattering has yielded (rows 7,8 in Table 1). Because of this we have omitted this old Bonn data and a subsequent involvement of the pioneer’s photo- 41 production measurements has given our final solution, which seems to be the most realistic one (row 10). Corresponding values of χ2 dp are placed in the last column of Table 2 (rejected data), in Table 3 (π+ and π0 production separately for cross section, Σ, P, and T), and in Table 4 for the Kharkov data from the final data set. In two last fits we have restricted the background variable parameters by the s, p waves and (row 11 in Table 1) and increased to vary the full set of the background d waves (row 12). Table 4. Characteristics of the Kharkov data R O Label Eγ, MeV ϑ, deg N χ2 dp π+ Σ GE81KH 280-420 30-150 56 3.6 P GE81KH 280-420 30-150 54 1.4 T GE81KH 280-420 30-150 53 1.9 T GE80KH 340-340 30-150 7 2.2 H BL86KH 320-320 90-120 4 5.2 H BL84KH 320-380 65-80 4 1.0 π0 Σ BL83KH 280-420 60-135 38 3.6 Σ GN76KH1 300-420 60-135 35 4.7 Σ GB78KH 360-400 140 2 4.6 P BL83KH 280-420 60-135 38 1.4 P GB78KH 360-400 140 2 2.6 T BL83KH 280-420 60-135 38 3.9 T GB78KH 360-400 140 2 1.0 Note: R − reaction, O − observable value 5. DISCUSSION By going back from the last decade into the past and involving older data we observe a rather smooth and plausible variations of the ∆+ mass and ratio EMR until stumbling at the old Bonn data on π0 differential cross sections. As to the EMR the relevant jump corroborates the known effect discussed in the Introduction, but the rapid increase of M0 and Γ0 on about 2 and 4 MeV correspondingly is unexpected. For example, in our previous calculations [27] all fits were fulfilled with the data [13], but ‘small’ EMR = (−1.43±0.08)% accompanied by the mass of M0 = 1232 ± 0.71 MeV appeared only in row 8 of Table 1 for the data up to maximal year 1984, and some comment seems to be necessary. The expression for the resonant multipoles used in [27] can be obtained from present Eq. (5): eRM iS M δ= δ+ 33 33 2/3 1 sin , (14) with some function to parameterize the function RBR MM S M += δ 33cot . (15) Evident shortage of such a parameterization is that it has to describe the cot δ33 being a sufficiently strong function of independent resonance parameters. Used in [27] rigid parameterization was not relevant to reproduce this feather and that has influenced the resonance parameters. Concerning the ∆+ mass from [15] first of all one has to take into account the difference in definitions. With reference to the Olsson’s work [28] the full magnetic resonant multipole is there proportional to the following construction (electric quadroupole was not treated): ))()(exp())()((sin WWWW RR β+ϕα+ϕ , (16) where the manifest notation of [15] are conserved. This block corresponds to one from Eq. (8) in [28], namely )sin( eP ie δ−δ+δδ , (17) supposing the phase shift addition (our Eq. (4)). That is quite correct, as Eq. (8) in [28] is derived without any assumption about the low of the unitary merging of the resonance and background in scattering. (By the way, in [28] Olsson has been advocated the low with approxi- mate subtraction of the resonance and the background phase shifts). However, the important point is that by introducing the background phase shift in parameterized form the authors of [15] are dealing with ‘pure’ resonance, with parameters being different from the “experimental’ one discussed in Sect. 3. For example, the mass of the latter coincides with the energy at which the resonant photomultipole passes through zero. For involved in [15] analysis ([16], 1977, s,p waves are fitted) this is about 1240 MeV (Eγ ≈ 340 MeV). As we have previously seen to some extent that could be caused by to the Bonn data [13] already included in this analysis. It should be stressed that the main Kharkov data were absent yet and in any case could not have influence on this mass. As to the old Bonn data it is not possible yet to reject them coming from the χ2 df value. We prefer the solution obtained with more recent data and taking into account location of the ∆+ mass relatively to the masses of the ∆ ++ and ∆0 [24]. All these values can be compared using Table 5 (we only take from PDG the data with errors). Table 5. The charge splitting of the ∆(1232) State Mass, MeV Width, MeV Source ∆++ 1230.5±0.2  ABAEV 95 1230.9±0.3 111.0±1.0 KOCH 80B 1231.1±0.2 111.3±0.5 PEDRONI 78 ∆+ 1231.9±0.4 112.5±1.7 Table 1, row 10 ∆0 1233.1±0.3  ABAEV 95 1233.6±0.5 113.0±1.5 KOCH 80B 1233.8±0.2 117.9±0.9 PEDRONI 78 Some of the Kharkov data have got into groups II, III of rejected data. As it is clear now, the main reason is underestimation of the systematic errors. Nevertheless the overwhelming majority of this data has good or acceptable χ2 dp. But time is coming, and now the polarization data T, Σ and P from Kharkov are considering as having the large statistical and systematic errors, especially for the γp→π0p process [29]. In addition, the combined experiments with linearly polarized photons and polarized proton have not been repeated yet and remain to be unique. General situation with the polarization data in the both reaction at consideration is demonstrated in the figure below, where the Σ, P, T angle dependencies are presented at some energies convenient to compare with the up-to- 42 date polarization measurements at Bonn, Mainz, and Brookhaven. New points have appeared mostly for linear asymmetry, and the situation for T asymmetry and polarization P in the reaction γp→π0p continue to be rather unambiguous. It is also easy to see that our final fit is in an excellent agreement with the last GWU solution [21] (SM02 in SAID) for the observables with looking reliable measurements. Some differences are seen only for two mentioned before P and T. 0,0 0,1 0,2 0,3 0,4 0,5 π +n, 320 MeV Σ our fit BE00MA BL01LE GE81KH GN76KH SM02 -0,1 0,0 0,1 0,2 0,3 0,4 0,5 0,6 0,7 0,8 0,9 π +n, 340 MeV P our fit GE81KH SM02 0 20 40 60 80 100 120 140 160 180 -0,1 0,0 0,1 0,2 0,3 0,4 0,5 0,6 0,7 0,8 0,9 θ , deg π +n, 340 MeV T our fit AA72TO GE80KH GE81KH SM02 0,0 0,1 0,2 0,3 0,4 0,5 0,6 0,7 our fit BE97MA BJ69FR BL01LE BL83KH BP70FR DR64ST GB78KH GN76KH SM02 π 0p, 320 MeV Σ -0,3 -0,2 -0,1 0,0 0,1 0,2 0,3 π 0p 350, 360 MeV P our fit, 350 our fit, 360 AL66BO AL68BO BL83KH BM69BO GB78KH SM02 0 20 40 60 80 100 120 140 160 180 -0,2 -0,1 0,0 0,1 0,2 0,3 0,4 0,5 0,6 π 0p, 320 MeV T θ , deg our fit BL83KH BO98BO GB78KH SM02 The Σ, P, and T vs pion c.m. angle θ for γp→π+n and γp→π0p reactions at Eγ = 320,...,360 MeV, with predictions according to the final solution (row 10 in Table 1, our fit) and GWU (SAID) solution SM02 [21] 6. SUMMARY The basic points of the present analytical mini- review and its conclusions can be briefly formulated as follows: • Our parameterization of the resonant photo- multipoles is the downright corollary of the expression obtained in the framework of the K- matrix formalism with multichannel two-particle unitarity [23], with using the Walker’s model for the resonance term. The reliable presentation of the background multipoles was reached via the cubic polynomials for the real parts with using the Watson theorem for imaginary ones. • The undertaken retrospective analysis reveals the significant influence of the Bonn π0 differential cross sections [13] on the ∆+ parameters: increase by ~ 3 MeV for the ∆+ mass and about 2 MeV for the width. Such an effect for the EMR is the 43 same as in the analyses using the Watson theorem [10] (approximately dividing by 2). That fully explains the small value of the EMR obtained in [9] by using the Kharkov analysis and also can be a reason for observing very large ∆+ mass in [15]. • The withdrawal of the Bonn data [13] allows to obtain the ∆+ mass and width being in a reasonable accordance with the corresponding values for the ∆++ and the ∆0 known from the πN scattering. • Despite some criticism the overwhelming majority of the Kharkov data on pion photoproduction in the first resonance region preserve its scientific signifi cance and in some cases even the monopoly position. As to the Bonn data the question is not so simple. They systematically cover the whole resonance region including the small and the large angles, where the new measurements yet are rather seldom and spread. Besides, coming from multipole analyses one can observe some ‘suspicious’ points and “derivations” in measurements of several laboratories, first of all at the edges of the energy or the angle intervals with measurements. 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