Downloaded By: [University of Virginia] At: 14:24 12 June 2007 @ Gordon and Breach Science Publishers Ltd. Radiation Effects 1976, VOI.27, pp. 179-181 Printed in Great Britain STOPPING CROSS-SECTIONS AND ATOMIC POTENTIALS J. C. ECKARDT, W. MECKBACH and R. A. BARAGIOLA Centro Atbrnico Bariloche, Cornisibn Nacional d e Enerpa Atornica, Instituto de Fisica “Dr. Jose A. Balseiro ”, Universidad Nacional de Cuyo, Bariloche, Argentina (Received May 16, I 9 7 3 A strong correlation is shown to exist throughout the periodic table between the 22 dependence of the electronic stopping cross-sections for 4He ions o f a given velocity and the Z dependence of the atomic potentials at a certain radius. An empirical formula is presented which allows the extrapolation o f stopping cross-section data for any ion at a given velocity in some elements, to elements for which experimental data are not available. This study covers the energy interval 100 < E/m < 1000 keV/amu. In the last few years, several authors have presented measurements and theories about the oscillating behaviour of the stopping cross-section S either as a function of target atomic number Zz for a given projectile or as a function of projectile atomic number Z , for a fixed target.’-’’ Ziegler and Chu’ have presented semiempirical values of S(Zz)for 400-4000 keV ‘He ions on 92 target materials. These values were derived from experimental data and from the Lindhard-Winther theory for electronic stopping. Chu and Powers4 have proposed that a Hartree-FockSlater (HFS) potential could be used to account for the structure of S ( Z z ) they observed for He ions in the region 22 G Zz Q 29. We have found that it is possible to fit the semiempirical values of Ziegler and Chug at each energy by the expression S = CVr, where V is the HFS potential of the target at a certain radius r from the nucleus and Cis a constant scale factor. For a given 4He+energy, a fit is obtained using constant values for r a n d C, the oscillatory dependence with Z2 being accounted for only by the variation of V with Z z . For each data set corresponding to a given He’ energy C-and r were computed to obtain a best fit of the semiempirical S ( Z z ) of Ziegler and Chu and the HFS potentials as calculated by Lu et aLz’ This was done using values for Z 2 20. The data for elements with Z2 < 20 were not included since the accuracy of the fits is less at these low Z z values. After establishing Cand r, S(Zz)was also calculated for these elements. Table I shows the values of C and r for different projectile energies. Figure 1 shows S = CVr curves at three different energies together with the semiempirical values of Ziegler and Chu.’ Also shown for 400 keV/ 179 amu are the theoretical results of the same authors. It is seen that our curve has the same shape as the theoretical curve but it agrees better with the semiempirical data. Since the Z2 dependence of S is similar for ions other than 4He3i’i6722there is a possibility to obtain values of S ( Z z ) for other projectiles for which S is known for some elements. We propose that w,,zz , u) = W l , u ) T(u) w ,zz 1 where r is given by Table I as a function of the velocity of the projectile u and C(Z,, u ) is a quantity which depends only on Z1 and on u . TABLE I Radial distances r, and scale factors C for 4He ions, at different . . ion velocities . . Elm U r keV/amu au a, C 6.9445. 10-9 cm/at 100 150 200 250 300 350 400 450 500 600 700 800 900 1000 2.00 2.45 2.83 3.16 3.46 3.74 4.00 4.24 4.47 4.90 5.29 5.66 6.00 6.32 1.549 1.367 1.284 1.133 1.133 1.064 1.ooo 0.939 0.882 0.829 0.779 0.732 0.687 0.687 35.9 32.8 30.7 25.6 24.9 22.1 19.5 17.3 15.4 13.2 11.5 10.1 8.9 8.5 Downloaded By: [University of Virginia] At: 14:24 12 June 2007 180 J. C. ECKARDT, W. MECKBACH AND R. A. BARAGIOLA TABLE I1 Scale factor C for 35CI ions at different energies Elm keV/amu C 6.9445.10* cm/at r a. ~~ ~~ 343 457 571 714 857 1.064 0.939 0.8 29 0.779 0.687 266 256 235 232 208 - other elements. Figure 2 shows the values so derived for 3 5 C ions ~ in Uranium as a function of Elm, together with values tabulated by Northcliffe and Schilling.24 It is interesting to note that the discrepancy between both curves is of the same magnitude as the discrepancy of the semiempirical values of Ziegler and Chu’ and the tabulations of Northcliffe and Schilling24 for 4He on U. r SOOl m FIGURE 1 Stopping cross-sections for 4He ions as a function of Z 2 . Full drawn line: semiempirical data of Ziegler and Chug; dotted line: C-r . Y; and dashed line: theoretical values from Ref. 9. a) Elm= 100 keV/amu r = 1.549 a, C = 35.9.6.9445.10-9 cm/at. b) Elm = 400 keV/amu r = 1.000 a, C = 19.5.6.9445. lo-’ cm/at. c) E/m = 1000 keV/amu r = 0.687 a, C = 8.5 .6.9445 . 10-9 cm/at. 1 I I I I Elm I . . . m I YXMO [keVlamu) FIGURE 2 Stopping cross-sections for 3 s C l ions in U as a function of energy per atomic mass unit. Full drawn line: extrapolated from experimental data of Ward ef aLZ3;dashed line: from Northcliffe and Schilling.24 The same calculations were made for I6O ions as projectiles, using experimental data of Porat and Ramavataram2’ and Ward ef U I ! , , ~ for fixed values of the ion velocities. It was again found that C did not depend on Z,. ACKNOWLEDGEMENTS This formula was tested by calculating C ( Z , , u ) for 35 C1 projectiles of different velocities in the targets Ni, Ge, Y,Ag and Au, using experimental S values of Ward et 0L2’ and the values of r(u) given in Table I. At each velocity, we obtain the same factor C for all the measured elements within 5%, the quoted errors in the experimental data being 4%. This, together with the fact that the elements used cover a wide Z2 range, some of them lying at maxima and minima of the oscillatory S(Z2)curve, gives a good proof that C i s independent of Z 2 . The calculated C values, listed in Table 11, were then used to extrapolate the data of Ward ef aL23 to We wish to thank Lic. V. H. Ponce and Lic. N. Arista for stimulating discussions. Mrs. Bibiana de Espincl is gratefully acknowledged for making the computer program. This work has been supported partially by the Organization of American States, Multinational Program in Physics. REFERENCES M. Bader, R. E. Pixley, F. S. Mozer and W. Whaling, Phyr Rev. 103,32 (1956). 2. F. Bernhard, U. Muller-Jahreis, G. Rockstroh and S. Schwabe, Phys. Srur. SOL 35, 285 (1969). 3. P. Apel, U. MulIer-Jahreis, G. Rockstroh and S. Schwabe, Phys. Star. Sol. 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