i I OFT ORNL P - . F ; : como . conto o . 2434 m . • || 1.25 1.4 1.6 MICROCOPY RESOLUTION TEST CHART NATIONAL BUREAU OF STANDARDS - 1963 ORNL-P-2434 CONF-660906-19 (Submitted for presentation at the International Conference on Nuclear Physics, Gatlinburg, Tennessee -- September 12-17, 1966) MACTC CFSTI PRICES MASTER SP 2 2 1966 HC. 84.00), MN SO Differential Scattering of Neutrons from Oxygen and Intermediate States J. L. Fowler and C. H. Johnson Oak Ridge National Laboratory Oak Ridge, Tennessee Abstract The explanation of the broad structure in the total neutron cross section of dºo between 3 and 4 MeV is of importance to the understanding of intermediate states. At 3.77 MeV we find under a 17 keV flo reson- ance a 3 kev dz/2 resonance interfering with a large dzia phase shift, and thus remove a difficulty in resonance parameter assignments at the peak. RELEASED FOR ANNOUNCEMENT UU IN NUCLEAR SCIENCE ABSTRACTS LEGAL NOTICE This report was prepared as an account of Government sponsored work. Neither the United States, por the Commission, nor any person acung on behalf of the Commission: A. Makes any warianty or representation, expressed or implied, with respect to the accu- racy, v.o. npleteness, or usefulness of the information contained in this report, or that the use of any i formation, apparatus, method, or process disclosed in this report may not Infringe privately owned rights; or B. Assumes any liabilities with respect to the use of, or for damages resulung from the use of any information, apparatus, method, or process disclosed in this report, As used in the above, “person acting on behalf of the Commission" includes any en- ployee or contractor of the Commission, or employee of such contractor, to the extent that such employee or contractor of the Commission, or employee of such contractor prepares, disseminates, or provides access to, any information pursuant to die employment or contract with the Commission, or his employment with such contractor. Research sponsored by the U. S. Atomic Energy Commission under contract with the Union Carbide Corporation. Session VIII (Submitted for presentation at the International Conference on Nuclear Physics, Gatlinburg, Tennessee -- September 12-17, 1966) Differential Scattering of Neutrons from Oxygen and Intermediate States* J. L. Fowler and C. H. Johnson Oak Ridge National Laboratory Oak Ridge, Tennessee The resonance structure of neutron scattering from +0 between 3 and 4 MeV is of particular interest in connection with explanations of inter- mediate states. There are several resonances of rather large reduced widths., The narrow peak at 3.77 Mev, however, has created a problem in the phase shift analysis of scattering data in this energy region. Fossan, et al," from total cross section measurements, found the height of this peak corresponded to a J = 5/2 resonance of 25 keV width. But in 100 proton scattering, the'F level whose excitation corresponds closely to this one is a J = 7/2- resonance.+ We have remeasured the total cross section in good geometry with 5 keV resolutions as shown on the right hand side of Fig. 1. Assuming the 3.77 MeV peak is a single resonance and correcting for the experimental energy resolution of 5 keV, we find I = 19 keV, which is slightly less than, but consistent with, th: 22 keV reported by Walton, et al,' and the 25 kev found by Fossan, et al.3 With a J = 5/2- assignment, we got a reasonable fit to an angular distribution at the 3.77 Mev peak.? However, as Lister and Sayre? have pointed out, we cannot fit angular distributions -. "Research sponsored by the U. S. Atomic Energy Commission under contract with the Union Carbide Corporation. - - - - . . . - - Session VIII . - - - 2 - on either side of the resonance with a consistent set of phase shifts and a 5/2- or 5/2+ assignment. In a recent analysis we have arrived at a solution to this problem. There is a narrow, ~3 keV, J = 3/2+ resonance under a ~17 keV J = 7/2- resonance. The large dal background phase shift, Fig. 2, makes the narrow dzia resonance show up as a dip, thus reducing the peak height in the total cross section. An attempt to make a similar fit with a narrow s, 1 resonance was unsuccessful. The left hand side of Fig. 1 shows the results of angular distribu- tion of neutron scattering measured in the vicinity of the 3.77 MeV peak. We used a liquid oxygen sample contained in a 1 mil wall Dewar flask de- signed to minimize background scattering. The outer wall, which was under atmospheric pressure, was 10 mils of stainless steel. The scatterer was supported in the center of a shielded cavity about a meter square anů 0.6 m deep.' An identical enpty Dewar flask, placed in the neutron beam, allowed background measurement. We detected neutrons scattered from the sample in a stilbene crystal from which pulses due to gamma rays were depressed by pulse-shape discrimination. Since we measured the direct flux by moving the crystal into the neutron beam, we were able to obtain absolute differential cross sections. Our results have been corrected for the effects of spurious neutron backgrounds, self-attenuation and multiple scattering in the sample, finite angular resolution, and the energy dependence of the detector efficiency. The solid line through the angular distribution points is the result of a least square phase shift fit to the data, with the phase shifts - 3 - which give the fit shown in the figure. We adjusted the resonance parameters of the narrow dalo resonance and the folo resonance so as to reproduce the total cross section shown as the solid line on the right hand side of Fig. 1. While as it is evident we obtain a reasonable fit to all the experimental information with the resonance parameters listed beside the total cross section curve, it is possible that further adjustment may improve the overall fit. Figure 2 shows our phase shifts as a function of neutron energy, - and includes results at lower energy from a previous analysis.' We estimate the uncertainties in these phase shifts by a procedure described in the literature. The very narrow do lo resonance at 3.770 MeV corresponds to a similar narrow do lo resonance in the vicinity of the 7/2- resonance in 177.4 This analysis shows two relatively broad dala resonances, one at 3.40 MeV ~500 keV wide, and another at 4.191 MeV 70 keV wide. Also, there are two p resonances: a Pale 500 keV resonance at 3.75 MeV, and a 100 keV P, lo resonance at 4.00 MeV. The broad dalo resonance corresponds to ~1/2 of the single particle limit. There is, of course, already a dz/2 resonance with a very large fraction of the single particle limit at 1 MeV. The Palo resonance at 3.75 MeV is about 1/5 of the single particle limit, the pain one is 1/20 this limit, the fr/2 one at 3.77 is about 1/10 of the limit. Since near zero energy the hole states of 170 have odd parity and the single particle states even parity, intermediate states arising from two-particle one-hole excitations should have odd parity. But as we see .4. above, the state in the region 3 - 4 MeV with largest reduced width (the 3.40 MeV state) has even parity. Recently G. E. Brown and A. M. Green have described the low lying even parity spectrum of 100 and to in terms of mixing the usual states in the spherical shell model with deformed states obtained by exciting particles out of a deformed core. In their model, the rather wide 1/2+ and 3/2+ states in 17 (Fig. 2) are interpreted as three-particle two-hole and five- particle four-hole excitations mixed with shell model states. They obtain reasonable agreement. The fact that the relative values of the reduced widths of the dais, Palo, and Iris states near 3.5 MeV in Fig. 2 are in roughly the same ratio as those of the dz/2, P3/2, and fy/2 states near zero energy in the 160 plus a neutron system may be a clue to the explanation of the to spectrum in the 3 - 4 Mev energy region. -.5 - References 1. J. L. Fowler and C. H. Johnson, Bull. Am. Phys. Soc. 10, 261 (1965). 2. D. Lister and A. Sayres, Phys. Rev. 143, 745 (1966). 3. D. B. Fossan, R. L. Walker, W. E. Wilson, and H. H. Barschall, Phys. Rev. 123, 209 (1961). 4. S. P. Salisbury and H. T. Richards, Phys. Rev. 126, 2147 (1962). 5. R. B. Walton, J. D. Clement, and F. Boreli, Phys. Rev. 107, 1067 (1957). 6. J. L. Fowler, to be published in Phys. Rev., July 1966. 7. J. L. Fowler and H. o. Cohn, Phys. Rev. 109, 89 (1958). 8. G. E. Brown and A. M. Green, Nucl. Phys. 75, 401 (1966). - - - - -. - - - - - - - . - - - * - - - - - -- - - 6 - Figure Captions Fig. 1 +90 differential neutron cross sections in the vicinity of the 3.77 MeV resonance. Fig. 2 to neutron scattering phase shifts as a function of neutron energy. ORNL-OWO 16-1204 En - 3.850 :0.015 Bor -106 8pin + 32°, 89* * +124• 80 +148°,809 -6° 817 RESONANCE En = 3.780 : 0.018 8577-1350 Boy+f*, date + 82 889 RESON., doo -4• 87 - RESONANCE RESONANCES Bu 12 -0.0015 { POT. -53+ 300 (E-3.770]• LEO- 3.772 IIIIIII [Tasco 75 POT. - 0 En * 3.769 B 3.90 Ex 3.770 : 0.018 Boy -138• 8ply -11°, dan +76 81RESON., 884 -9 87= RESONANCE 3.88 3.86 3.84 En (MeV) LLLLLLLL o ($) (barns i 3.76 3.74 En = 3.767 + 0.017 854 -1390 804 -12°, dass +78° 80% RESON., 88% -13° 817 RESONANCE 3.72 3.70 17 6 5 4 3 2 1 0 og (barns) En = 3.7600.018 80m =-144. 8p4-12°, 804+ 750 8172 = RESON., 804 -17 81% = RESONANCE E, - 3.700 + 0.014 A doua-130 1 84 =-21°, 804* + 720 884-46°, 80 -10° 8p7p = RESONANCE لنلللننناه 0.8 Q4 0-04 -0.8 cos $ (C.M.) FIG. 1 ORNL-OWG 64-10113R2 1.00 1.32 2.37 3.40 3.7573.77 -4.00 -FOWLER AND COHN- —JOHNSON AND FOWLER- 883/2- PHASE SHIFT (deg) 8p% Los 12 R 1.0 1.5 3.0 3.5 4.0 2.0 2.5 En (Mev) Fig. 2 -- .. : ::: ::.. . e * . . . . - . - .- .. . 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