IEEE Ttnwactionz on NucteaA Science, VotZNS-23, No,2, Aptik 1976 IONS IN COLLISIONS OF 60-250 HELIUM BEAMS TRAVERSING CARBON FOILS* KEV A.J. Kestelman, E. Alonso and R.A. Baragiola Centro At6mico Bariloche Comisi6n Nacional de Ener4ga At6mica 8400 Bariloche, ARGENTINA FORMATION OF He Summary A grounded shield(9) surrounds the detector assembly. The whole experimental set-up is inside a chamber which was held at 2 to 5 x 106 Torr during the experiment. The detector moving system is mechanically connected to a potentiometer whose signal is sent to the X axis of an X-Y recorder, the Y axis receiving a signal proportional to the ion current as measured by an electrometer connected to the movable detector. Because of experimental reasons we have not measured the He+ and He" components (except to check that the measuring system was working properly) but to get Fj,,we have used measuinstead, the values of Fo previously prvosymau 16 red in our laboratory . A typical spectrum of components He0 and He (where component He+ is also seen) is shown in Fig. 2. The double peaks observed for each component are due to a backlash effect in the gear train mechanism of the detector moving system, and the different position of the peaks depends on whether the detector is moving CW or CCW. The measured equilibrium fractions FTO for He in carbon are shown with its statistical errors in Fig. 3 as a function of beam energy. Preliminary measurements of the charge equilibrium fraction FT,,for the negative com ponent are presented for a He + beam traversing a 2 pg/cm 2 carbon foil. This fraction decreases with energy with a value of about 2.5 x 10i4 at 60 keV and about 1 x 10 4 at 250 keV. Introduction Dukel'skii et al. first reported the formation of He ions from He beams traversing different noble gases. Since then various authors have studied the process of He formation from He traversing different gases 2-10 and metal vapors However to our knowledge, the formation of He in solids has not been studied so far. 11-13. Experimental Arrangement and Results To study the formation of He ions from a He+ beam traversing carbon foils, the equipment previously used in this laboratory to measure He formation in gases 10 was modified as sketched in Fig. 1. The magnetically separated He+ beam from a 300 keV Cockcroft-Walton type accelerator is collimated by diaphragm (2) before traversing a carbon foil(3)l4which is about 2 pg/cm2 thick, enough to charge equilibrate the beam without causing too much energy degradation (not more than - 5% at the lowest energies). The charge equilibrated beam passes through collimators (4) and (5) and the different charge components are separated by electrostatic deflector (6) and collected by a movable secondary emission detector (7) after having traversed a positively polarized diaphragm covered by a thin (rv10pg/cm2 ) carbon foil (8) thus ensuring the same detection efficiency for ions and neutral atoms 15. *Work supported in part by the Organization of American States Multinational Program in Physics. Acknowledgements We wish to thank Messrs. C. Lulich and F. Tutzauer for their fine machine work. References 1. V.M. Dukel'skii, V.V. Afrosimov, and N.V. Fedorenko, Sov. Phys., JETP 3, 764 (1956). 2. P.M. Windham, P.J. Joseph, and J.A. Weinman, Phys. Rev. 109, 1193 (1958). 3. Ya.M. Fogel', V.A. Ankudinov, and D.V. Pilipenko, Sov. Phys., JETP 11, 18 (1960). 4. T. Jorgensen, Jr., C.E. Kuyatt, W.M. Lang, D.C. Lorentz, and C.A. Sautter, Phys. Rev. 140, A 1481 (1965). S. A. Papkov and G.J. Steiger, Z. Naturforschg. 21a, 1048 (1966). 6. L.E. Collins and P.T. Stroud, Proc. Phys. Soc. 90, 641 (1967). 7. H.B. lilbody, R. Browning, K.F. Dunn, and 1143 Authorized licensed use limited to: University of Virginia Libraries. Downloaded on January 31, 2010 at 14:44 from IEEE Xplore. Restrictions apply. A.I. McIntosh, J. Phys. B (Atom. Molec. Phys.) 2, 465 (1969). 8. H.B. Gilbody, K.F. Dunn, and R. Browning, J. Phys. B (Atom. Molec. Phys.) 3, L19 (1970). 15. S.K. Allison, Rev. Mod. Phys. 30, 1143 (1958)_ 9. K.F. Dunn and H.B. Gilbody, Proc. VII Intl. Conf. on Physics of Electronic and Atomic Collisions, 1085, Amsterdam (1971). 10. A.J. Kestelman and R.A. Baragiola, Proc. VIII Intl. Conf. on Physics of Electronic and Atomic Collisions, 825, Belgrad (1973); A.J. Kestelman, R.A. Baragiola, and J. Bratina, Comunicaciones Asociacion Fisica Argentina (AFA), 1, 12 (1973); A.J. Kestelman and R. Baragiola, Comunicaciones AFA, 2, 83 (1974) and 60th Meeting AFA Paper L.3, Tucuman, May 1974 (unpublished). 11. B.L. Donnally and G. Thoeming, Phys. Rev. 159, 87 (1967). 12. R.A. Baragiola, E.R. Salvatelli, and G. Lantschner, Proc. VII Intl. Conf. on Physics of Electronic and Atomic Collisions, 788, Amsterdam (1971); R.A. Baragiola and E.R. Salvatelli, J. Phys. B (Atom. Molec. Phys.) 8, 382 (1975). 13. R.N. Il'in, V.A. Oparin, I.T. Serenkov, E.S. Solov'yov, and N.V. Fedorenko, Proc. VII Intl. Conf. on Physics of Electronic and Atomic Collisions, 793, Amsterdam (1971). 14. Supplied by Yissum Research Development Company, Hebrew University, Jerusalem, Israel. 16. A.J. Kestelman, W. Meckbach, and J.I. Cisneros, 57th Meeting AFA, Paper D.3.1, Cordoba, May 1972 and Final Scientific Report Grant AFOSR-69-1802, August 1972 (unpublished). 124 keV He'+ Carbon lOOmV-10 Qt He I Iv-lofI I Fig. 2 Typical spectrum of the He-, He0 and He+ peaks taken at 124 keV. Figures at the top of each peak indicate sensitivity settings for the electrometer. Arrows point at changes in these settings while peaks are being recorded. For explanation of double peaks see text. 3 I 2 0 0 2 1W 3 4 cm Fig. 1 1) He' beam; 2) Diaphragms; 3) 2 p/cm2 carbon foil; 4 and 5) Collimators (the configuration shown was designed for a different experiment which is now being performed); 6) Electrostatic plates; 7) Movable detector; 8) Diaphragm with charge equilibrating carbon foil; 9) Shielding. Insert shows movable detector in better detail. He +Carbon -~~~~~~~~~~~5 n 50 100 _ 200 150 BEAM ENERGY (keV) 250 Fig. 3 Charge equilibrium fraction for He- in carbon vs. He+ beam energy. 1144 Authorized licensed use limited to: University of Virginia Libraries. Downloaded on January 31, 2010 at 14:44 from IEEE Xplore. Restrictions apply.
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