T- UNITED STATES AT O M I C E N E R G Y CO M M I SS I ON AECU - 1638 ENERGY RESPONSE OF NaI(Tl) CRYSTALS TO ALPHA PARTICLES OF LESS THAN 10 MEW By - - Ralph H. Lovberg ENGR 188Ary **** JUN l tº ić ºf UNIV. OF WAs. tº #: September 24, 1951 |Date Declassified] Los Alamos Scientific Laboratory |- Technic a l l n form a tion Service, O a k Ridge, Te n n e s see UNIVERSITY OF MICH III.iii. 390.1508647 *. *-** tº ‘’ ‘. . . ,” *...* INSTRUMENTATION Reproduced direct from copy as submitted to this office. This report is based on LADC-loló. AEC, Oak Ridge, Tenn., 10-24-51--555-W7552 # *f: t gº & §*::: º !-- §§ &zº. ENERGY RESPONSE OF NaI (Tl) CRYSTALS TO ALPHA PARTICLES OF LESS THAN 10 MEW Ralph H. Lovberg Recent investigation") of the response of NaI crystals as scintil- lation counters of charged particles has shown that while the light output is essentially linear with energy of incident electrons, protons, and deuterons, there is nonlinearity in the response to alpha particles of less than 10 Mev. The investigation described here was undertaken to determaine in detail the shape of this nonline arity. In this experiment, energy control was accomplished by air attenuation and the particles were allowed to strike a freshly cleaved crystal face. To avoid the usual rapid moisture contamination of the crystal surface in the open atmosphere, the entire operation was performed in a dry-box, with signal and high-voltage cables brought in to the 5819 photomultiplier by means of airtight feed-through connectors. P20 g was used as a drying agent, and no detectable deterioration of crystals cleaved in the box took place in a three-week periode Two sources of alpha particles were used, both thin to their own radi- ations. The first was a "thorium active" deposit yielding alpha groups at 8.78 Mev and 6.0l. Mew from Thº' and The disintegrations, respectively. The 239 second was Pu‘’’, giving 5.16 Mev alphas. Both sources were deposited on the ends of probe rods which passed through a light-tight, sliding seal in the end of the phototube housing. The l x 1 x 0.1 cm crystal was held to the tube face by a wire clip, with a drop of mineral oil providing addi- tional optical coupling. The thorium probe was used in seven positions from l.00 to 6.00 cm from the crystal, and the Pu source in five positions from 2.00 to 3.62 cm, * Work done under the auspices of the AEC. – l - the near position in each case being the limit at which the source backing reflected a significant amount of light back into the photocathode, pro- ducing spurious heightening of output pulses. Appropriate range corrections for the local atmospheric pressure of 60.2 cm Hg were made, and the mean particle energies were computed from Bethe's range-energy curves"?). “s Output of the 5819 was fed into a low gain preamplifier for polarity inversion, through a Los Alamos model 503 pulse amplifier, and into a con- tinuously variable single-channel pulse height discriminator. Line arity of the electronic system was checked by applying standard pulses to the phototube anode resistor and observing the corresponding discriminator dial readings. No corrections were found necessary. ! --- In the accompanying figure, mean output pulse height for each probe position is plotted against computed mean energy. In every position, the peak of the pulse height distribution could be determined to within one volt. I wish to thank Mr. Hugh Stoddart of the Los Alamos Cyclotron group for preparation of the sources used in this experiment. *Taylor, Remley, Jentschke, and Kruger, Phys. Rev. 83, 169 (1951) (*)Bethe, The Properties of Atomic Nuclei II., Brookhaven National Laboratory (1919)