4 NUMERICAL METHODSThe code GOSIA is designed to perform various functions defined by user-specified sequence of options. Inthe simplest mode, GOSIA can be used to calculate the <strong>excitation</strong> probabilities, population of the levels <strong>and</strong>γ-decay statistical tensors, equation 2.30, thus providing an equivalent of the code COULEX. Activatingthe γ-decay module of the code extends this type of calculation to obtain the γ yields for a single valueof bombarding energy <strong>and</strong> scattering angle, as well as performing integration over specified ranges of thebombarding energy (due to the projectile energy loss in a target ) <strong>and</strong> projectile scattering angle to reproducereal experimental conditions. These calculations require an input set of matrix elements treated as fixed <strong>data</strong>.The main purpose of GOSIA is, however, to fit the electromagnetic matrix elements to reproduce availableexperimental <strong>data</strong>. GOSIA can h<strong>and</strong>le simultaneously experimental γ yields (up to 48000) observedin50independent experiments. Additional <strong>data</strong>, i.e. branching ratios (max. 50), lifetimes of the nuclear levels(max. 10), E2/M 1 mixing ratios (max. 20) <strong>and</strong> previously measured Eλ matrix elements (max. 30) alsomay be included. All these <strong>data</strong>, <strong>and</strong> their experimental uncertainties, are used to construct a least-squaresstatistic, usually called χ 2 or penalty function. The minimum of this statistic, treated as a function of matrixelements, defines the solution, while its distribution in the vicinity of the minimum determines the errors offitted matrix elements. In the present version of the code, the investigated nucleus is described by maximumof 75 energy levels, with the number of magnetic substates not exceeding 600. The levels may be coupledwith up to 500 matrix elements (E1 through E6 <strong>and</strong> M1, M2), any number of them allowed to be declaredas the variables to be fitted.As mentioned before, direct use of the full Coulomb <strong>excitation</strong> formalism to perform the minimizationis out of the question due to the computer time necessary for repeated calculations. The mimimization canbe accelerated using the approximation presented in Chapter 3. A significant amount of time also can besaved if the recoil-velocity correction ( 2.2.2) is neglected. The effect of both replacing the full <strong>excitation</strong>formalism by the matrix approximation <strong>and</strong> neglecting the relativistic correction is only weakly dependenton the matrix elements, therefore it is feasible to introduce the “correction factors“, that account for thedifferences between full <strong>and</strong> approximate calculations which are assumed to be independent of the fittedmatrix elements. The minimization can be performed using only the fast, approximate formalism, withcorrection factors refreshed by running the full calculation periodically. In addition, the Coulomb <strong>excitation</strong>approximation is applied only to ∆m =0<strong>and</strong> ∆m =±1 couplings, thus an effect of truncation of the numberof magnetic substates being taken into account is also included in the correction factors, since this is notstrongly dependent on the actual set of matrix elements.Further acceleration of the fitting procedure is made possible by replacing the integration over experimentdependentscattering angle <strong>and</strong> bombarding energy ranges with a single calculation of the Coulomb <strong>excitation</strong>induced γ yields assuming the mean values of the scattering angle <strong>and</strong> bombarding energy. This approximationalso is not explicitly dependent on the fitted matrix elements, thus the difference between the integrationprocedure <strong>and</strong> the result of using the mean values of bombarding energy <strong>and</strong> scattering angle can be accountedfor by introducing another set of correction factors, treated as constants. Actually, it is convenientto apply this correction to the experimental yields, i.e. to rescale the experimental <strong>data</strong> according to thecomparison of integrated <strong>and</strong> “mean“ yields. This is done initially using a starting set of matrix elements<strong>and</strong> the resulting “corrected experimental yields“ are subsequently used as the experimental values for fitting(this procedure is presented in detail in Section 4.4). Thus, the fitting of matrix elements is performed usingtwo levels of iteration - first, external, is to replace the experimental ranges of bombarding energy <strong>and</strong> scatteringangle with the average values of these parameters, while second, internal, is the actual minimizationof the least-squares statistic. After the convergence at the internal level is achieved, one should recalculatethe correction to the experimental yields with the current set of matrix elements <strong>and</strong> repeat the minimization.Usually, for thin targets <strong>and</strong> a not excessively wide range of scattering angles, the second repetition ofexternal iteration already yields negligible changes in the matrix elements found by the minimization. It hasbeen checked, that even if no particle coincidences were required, only 2-3 recalculactions on the externallevel were necessary despite the integration over the full solid angle.Estimation of the errors of fitted matrix elements is a final step for the Coulomb <strong>excitation</strong> <strong>data</strong> <strong>analysis</strong>.This rather complicated procedure is discussed in Section 4.6. A separate program, SELECT, has beenwritten to reduce the considerable computational effort required for this task using the information obtainedduring minimization. This information, preprocessed by SELECT, is fed back to GOSIA. Optionally, the34
esults of minimization <strong>and</strong> error runs can be used to evaluate quadrupole sum rules by a separate codeSIGMA ( Chapter 6 ).The extraction of the matrix elements from experimental <strong>data</strong> requires many runs of GOSIA. Duringthese runs, GOSIA creates <strong>and</strong> updates a number of disk files, containing the <strong>data</strong> needed to resume the<strong>analysis</strong> or to execute SELECT or SIGMA <strong>codes</strong>. The details of permanent file manipulation are presentedin Chapter 7.Relatively modest central memory requirements of GOSIA (about 1.5MB) are due to the sharing ofthe same memory locations by different variables when various options are executed <strong>and</strong> to replacing thestraightforward multidimensional arrays (such as e.g. matrix elements) with catalogued vectors <strong>and</strong> associatedlogical modules. The description of the code given in this chapter therefore will not attempt to accountfor its internal organization, which is heavily dependent on the sequence of options executed <strong>and</strong>, in general,of no interest to the user. Instead, it will concentrate on the algorithms used <strong>and</strong> the logic employed inGOSIA. The basic knowledge of the algorithms is essential since the best methods of using the code arestrongly case-dependent, so much freedom is left to the user to choose the most efficient configurationsaccording to the current needs.All three <strong>codes</strong>- GOSIA, SIGMA <strong>and</strong> SELECT- are written in the st<strong>and</strong>ard FORTRAN77 to make theirimplementation on various machines as easy as possible. The necessary modifications should only involvethe output FORMAT statements, which are subject to some restrictions on different systems. Full 64 bitaccuracy is strongly recommended since the results can be untrustworthy when run using 32 bit accuracy.4.1 Coulomb Excitation Amplitudes <strong>and</strong> Statistical TensorsThe state of a Coulomb excited nucleus is fully described by the set of <strong>excitation</strong> amplitudes, a IM (M 0 ),defined by the solution of Eq. 2.17a at ω = ∞, or, approximately, by the matrix expansion 3.5., used forminimization <strong>and</strong> error estimation. To set up the system of coupled-channel differential equations 2.17ait is necessary first to define the level scheme of an excited nucleus. Certainly, from a practical point ofview, the level scheme should be truncated according to the experimental conditions in such a way thatreasonable accuracy of the <strong>excitation</strong> amplitudes of the observed states is obtained with a minimum of thelevels included in the calculation. As a rule of thumb, two levels above the highest observed state in eachcollective b<strong>and</strong> should be taken into account to reproduce a given experiment reliably. Truncation of thelevel scheme at the last observed level leads to an overestimation of the <strong>excitation</strong> probability of this leveldue to the structure of the coupled-channels system 2.17a, while including additional levels above, even iftheir position is only approximately known, eliminates this effect.The solution to the coupled-channels system 2.17a should, in principle, involve all magnetic substates ofagivenstate|I >, treated as independent states within a framework of the Coulomb <strong>excitation</strong> formalism.However, due to the approximate conservation of the magnetic quantum number in the coordinate systemused to evaluate the Coulomb <strong>excitation</strong> amplitudes (as discussed in Chapter 2) it is practical to limit thenumber of the magnetic substates taken into account for each polarization of the ground state, M 0 . Inany case, the <strong>excitation</strong> process follows the “main <strong>excitation</strong> path“, defined as a set of magnetic substateshaving the magnetic quantum number equal to M 0 , the remaining magnetic substates being of less <strong>and</strong>less importance as the difference between their magnetic quantum number <strong>and</strong> M 0 increases. The relativeinfluence of the <strong>excitation</strong> of magnetic substates outside the main <strong>excitation</strong> path is experiment-dependent,therefore GOSIA allows the user to define the number of magnetic substates to be taken into accountseparately for each experiment. This choice should be based on the requested accuracy related to the qualityof the experimental <strong>data</strong>, keeping in mind that reasonable truncation of the number of the magnetic substatesinvolved in Coulomb <strong>excitation</strong> calculations directly reduces the size of the coupled channels problem to besolved.The integration of the coupled differential equations 2.17a should be in theory carried over the infiniterange of ω, which, practically, must be replaced with a finite range wide enough to assure the desired accuracyof the numerical solution. To relate the effect of truncating the ω-range to the maximum relative error ofthe absolute values of the <strong>excitation</strong> amplitudes, a c , the following criterion is used:R ∞1 −∞ Q λ0( =1,ω)dω − R ω maxQ−ω max λ0 ( =1,ω)dωR4∞−∞ Q ≤ a c (4.1)λ0( =1,ω)dω35
- Page 1: COULOMB EXCITATION DATA ANALYSIS CO
- Page 4 and 5: 10 MINIMIZATION BY SIMULATED ANNEAL
- Page 6 and 7: 1 INTRODUCTION1.1 Gosia suite of Co
- Page 8 and 9: 104 Ru, 110 Pd, 165 Ho, 166 Er, 186
- Page 13 and 14: Figure 1: Coordinate system used to
- Page 15 and 16: Cλ E =1.116547 · (13.889122) λ (
- Page 17 and 18: Figure 2: The orbital integrals R 2
- Page 19 and 20: 2.2 Gamma Decay Following Electroma
- Page 21 and 22: where :d 2 σ= σ R (θ p ) X R kχ
- Page 23 and 24: Formula 2.49 is valid only for t mu
- Page 25 and 26: Ã XK(α) =exp−iτ i (E γ )x i (
- Page 27 and 28: important to have an accurate knowl
- Page 29 and 30: 3 APPROXIMATE EVALUATION OF EXCITAT
- Page 31 and 32: with the reduced matrix element M c
- Page 33: q (20)s (0 + → 2 + ) · M 1 ζ (2
- Page 37 and 38: adjustment of the stepsize accordin
- Page 39 and 40: approximation reliability improves
- Page 41 and 42: Zd 2 σ(I → I f )Y (I → I f )=s
- Page 43 and 44: 4.5 MinimizationThe minimization, i
- Page 45 and 46: X(CC k Yk c − Yk e ) 2 /σ 2 k =m
- Page 47 and 48: However, estimation of the stepsize
- Page 49 and 50: It can be shown that as long as the
- Page 51 and 52: een exceeded; third, the user-given
- Page 53 and 54: where f k stands for the functional
- Page 55 and 56: x i + δx i Rx iexp ¡ − 1 2 χ2
- Page 57 and 58: method used for the minimization, i
- Page 59 and 60: OP,ERRO (ERRORS) (5.6):Activates th
- Page 61 and 62: -----OP,SIXJ (SIX-j SYMBOL) (5.25):
- Page 63 and 64: 5.3 CONT (CONTROL)This suboption of
- Page 65 and 66: I,I1 Ranges of matrix elements to b
- Page 67 and 68: CODE DEFAULT OTHER CONSEQUENCES OF
- Page 69 and 70: 5.4 OP,CORR (CORRECT )This executio
- Page 71 and 72: 5.6 OP,ERRO (ERRORS)ThemoduleofGOSI
- Page 73 and 74: 5.7 OP,EXIT (EXIT)This option cause
- Page 75 and 76: M AControls the number of magnetic
- Page 77 and 78: 5.10 OP,GDET (GE DETECTORS)This opt
- Page 79 and 80: 5.12 OP,INTG (INTEGRATE)This comman
- Page 81 and 82: ¡ dE¢dx1 ..¡ dEdx¢Stopping powe
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5.13 LEVE (LEVELS)Mandatory subopti
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5.15 ME (OP,COUL)Mandatory suboptio
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Figure 10: Model system having 4 st
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ME =< INDEX2||E(M)λ||INDEX1 > The
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When entering matrix elements in th
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There are no restrictions concernin
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5.18 OP,POIN (POINT CALCULATION)Thi
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5.20 OP,RAW (RAW UNCORRECTED γ YIE
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5.21 OP,RE,A (RELEASE,A)This option
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5.25 OP,SIXJ (SIXJ SYMBOL)This stan
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5.27 OP,THEO (COLLECTIVE MODEL ME)C
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2,5,1,-2,23,5,1,-2,23,6,1,-2,2Matri
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5.29 OP,TROU (TROUBLE)This troubles
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to that of the previous experiment,
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To reduce the unnecessary input, on
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OP,STAR or OP,POIN under OP,GOSI. N
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5.31 INPUT OF EXPERIMENTAL γ-RAY Y
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6 QUADRUPOLE ROTATION INVARIANTS -
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*½P 5 (J) = s(E2 × E2) J ׯh¾
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The expectation value of cos3δ can
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where ē is an arbitratry vector. D
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achieved using “mixed“ calculat
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TAPE9 Contains the parameters neede
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TAPE18 Input file, containing the i
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7.4.4 CALCULATION OF THE INTEGRATED
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OP,EXITInput: TAPE4,TAPE7,TAPE9Outp
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OP,ERRO0,MS,MEND,1,0,RMAXand the fi
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8 SIMULTANEOUS COULOMB EXCITATION:
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4, 3, 1kr88.corKr corrected yields
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0 Correction for in-flight decay ch
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OP, ERRO Estimation of errors of fi
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9 COULOMB EXCITATION OF ISOMERIC ST
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configurations with a probability e
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The average range covered by each m
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SFX,NTOTI1(1),I2(1),RSIGN(1)I1(2),I
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11.2 LearningtoWriteGosiaInputsThe
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(1.6 MeV)1.1 MeV0.75 MeV0.4 MeV0.08
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Define the germaniumdetector geomet
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Figure 15: Flow diagram for Gosia m
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gosia < 2-make-correction-factors.i
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Issue the commandgosia < 9-diag-err
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At this point, it is suggested to c
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calculation.) In this case, a copy
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4,-4, -3.705, 3,44,5, 4.626, 3.,7.5
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90145901459014590145901459014590145
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.10.028921.10.026031.10.023431.10.0
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5,5,634,650,82.000,84.000634,638,64
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*** CHISQ= 0.134003E+01 ***MATRIX E
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CALCULATED AND EXPERIMENTAL YIELDS
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11.7 Annotated excerpt from a Coulo
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11.8 Accuracy and speed of calculat
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18,10.056,0.068,0.082,0.1,0.12,0.15
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line 152 Eu 182 Tanumber (keV) (keV
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1.6 Normalization between data sets
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13 GOSIA 2007 RELEASE NOTESThese no
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Matrix elements 500(April 1990, T.
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14 GOSIA Manual UpdatesDATE UPDATE2
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[KIB08]T.Kibédi,T.W.Burrows,M.B.Tr