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Dive into the research topics where W.N. Catford is active.

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Featured researches published by W.N. Catford.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1988

The identification and rejection of energy-degraded events in gas ionization counters

T.R. Ophel; L.K. Fifield; W.N. Catford; N.A. Orr; C.L. Woods; A.B. Harding; G.P. Clarkson

Abstract A common feature of the measurement of charged particles with gas detectors is the presence of a small fraction of events (∼ 0.1–0.2%) for which significantly less than the total ionization is recorded. These events cause an energy tailing that can seriously impair the identification functions of gas detectors used either to instrument the focal plane of magnetic spectrometers or for accelerator mass spectrometry. The anomalous, energy-degraded events are shown to arise both from reactions between the incident ions and the detector gas and, more importantly, from the scattering of ions by the gas. It is demonstrated that an appropriate detector configuration provides the means to reject most of the anomalous events, allowing the measurement of very low cross section reactions without significant background interference from such events.


Nuclear Physics | 1989

Study of 19N and 21O by multinucleon transfer

W.N. Catford; L.K. Fifield; N.A. Orr; C.L. Woods

Abstract The multinucleon transfer reactions 18 O( 18 O, 17 F) 19 N and 18 O( 18 O, 15 O) 21 O have been studied at a beam energy of 117 MeV and a mean reaction angle of 10°. The same reactions, but detecting the neutron-rich ejectiles, have also been studied at a mean angle of 4.5°. Excitation energies for low-lying levels in the two T z = 5 2 nuclei 19 N and 21 O have been derived. The correspondence between the observed levels and those predicted by 0kh ω shell-model calculations is discussed. The proposed level assignments are deduced by analogy with results from the 16 O( 18 O, 17 F) 17 N and 16 O( 18 O, 15 O) 19 O reactions, which were also studied in the present work, and are supported by calculations employing a semi-classical reaction model.


Nuclear Physics | 1989

Reaction studies of the neutron-rich nuclei 22, 23F

N.A. Orr; L.K. Fifield; W.N. Catford; C.L. Woods

Abstract The masses and excited states of the neutron-rich nuclei 22 F and 23 F have been measured using the heavy-ion transfer reactions 22 Ne( 7 Li, 7 Be) 22 F and 22 Ne( 18 O, 17 F) 23 F. Mass excesses of 2.80 ± 0.02 MeV and 3.32 ± 0.09 MeV, respectively, were deduced from the reaction Q -values. The value for 22 F differs from that previously accepted due to the existence of a low-lying doublet. A number of excited states have been identified in both nuclei, and the results are compared with shell-model calculations.


Nuclear Physics | 1986

The mass of 35Si

L.K. Fifield; C.L. Woods; W.N. Catford; R.A. Bark; P.V. Drumm; K.T. Keoghan

Abstract The mass excess of 35 Si has been determined as −14.427 ± 0.060 MeV from a measurement employing the 36 S( 13 C, 14 O) 35 Si reaction. No excited states of 35 Si were observed. The 34 S( 13 C, 14 O) 33 Si reaction was studied simultaneously, and previously unreported excited states in 33 Si were observed at 1.47, 2.00, 3.19, 4.13 and 5.48 MeV.


Nuclear Physics | 1992

The missing 12+ mirror state in 9B

W.N. Catford; L.K. Fifield; E.L. Reber; K. W. Kemper; J.D. Brown

Abstract The status of the mirror state in 9 B of the first excited 1 2 + 1.68 MeV state in 9 Be is reviewed. The experimental evidence is inconclusive except for an apparent peak recently reported in a spectrum from the 9 Be( 6 Li, 6 He) 9 B reaction. This reaction has been reinvestigated at the same energy and angle but with substantially improved resolution and statistics, and the present results provide no evidence for the previously reported peak. Spectra obtained at other energies and angles have very low background and yet similarly fail to exhibit a peak. In addition, no evidence for population of the mirror state is found in spectra taken for the reaction 10 B( 9 Be, 10 Be) 9 B at two bombarding energies. The energy and width of the expected 1 2 + state in 9 B remain open questions for which several different theoretical descriptions offer quite different predictions.


Nuclear Physics | 1991

Measurements of E3 transition strength in the stable even-mass Hg isotopes

C.S. Lim; W.N. Catford; R.H. Spear

Abstract Values of B( E 3; 0 + 1 →3 − 1 ) have been determined for the nuclei 198, 200, 202, 204Hg by Coulomb excitation using 12C projectiles. The results obtained are 0.44 (14), 0.41 (4), 0.42 (4) and 0.37 (5) e2 · b3, respectively, corresponding to enhancements of 27 (9), 25 (2), 25 (3) and 22 (3) W.u. The data indicate a clear discontinuity of E3 transition strength between Pt (Z = 78) and Hg (Z = 80), and also between Hg and Pb (Z = 82).


Nuclear Physics | 1988

A measurement of the mass of 39Sc

C.L. Woods; W.N. Catford; L.K. Fifield; N.A. Orr

Abstract The mass of the proton-rich nucleus 39 Sc has been derived from a measurement of the Q -value of the 40 Ca( 14 N, 15 O) 39 Sc reaction at a beam energy of 102.5 MeV and mean reaction angle of 6°. A value of −27.67 ±0.03 MeV was obtained for the Q -value, implying a mass excess of −14.19 ± 0.03 MeV for the ground state of 39 Sc, which is therefore unbound to proton emission by an energy of 580 ±30 keV. There is some evidence for an excited state in 39 Sc at an energy of 950 ±keV. This state is tentatively identified as the analog of the 1.27 MeV 3 2 − state in 39 Ar. The cross sections to the 1 2 + and 5 2 + states in 15 C confirm an earlier suggestion that this reaction is well suited to the observation of proton-rich nuclei via direct transfer reactions having very negative Q -values.


Nuclear Physics | 1988

Heavy-ion reaction studies of 35,36P

N.A. Orr; W.N. Catford; L.K. Fifiekd; T.R. Ophel; D.C. Weisser; C.L. Woods

Abstract The spectroscopy of the T z ⩾ 3 2 nuclei 35 P and 36 P has been studied using a variety of multi-nucleon heavy-ion transfer reactions. This has led to the observation of a number of new levels in both nuclei. The probable structure of these and previously reported levels are deduced through comparison with DWBA and shell-model calculations.


Nuclear Physics | 1988

Studies of the Tz = 52 nuclei 31Al and 29Mg

C.L. Woods; W.N. Catford; L.K. Fifield; N.A. Orr; R.J. Sadleir

Abstract The multi-nucleon transfer reactions 30Si(18O,17F)31Al and 30Si(13C, 14O)29Mg have been investigated at incident energies of 100 and 93 MeV respectively and a mean reaction angle of 8°. Excited states of the T z = 5 2 nuclei 31Al and 29Mg have been studied and a mass excess of −14.967 ± 0.025 MeV obtained for the ground state of 31Al. The 28Si(18O,17F)29Al and 28Si(13C, 14O)27Mg reactions have also been studied, enabling conclusions to be drawn concerning the probable structure of many of the states observed in 31Al and 29Mg. Several 0ħω levels predicted in recent complete sd-shell calculations have been assigned experimental counterparts for the first time. The results also support a previous suggestion that negative-parity states occur in 29Mg at 1.10 and 1.46 MeV.


Nuclear Physics | 1988

Study of 51Ca via three-neutron transfer

W.N. Catford; L.K. Fifield; T.R. Ophel; N.A. Orr; D.C. Weisser; C.L. Woods

Abstract Low-lying levels in 51 Ca have been studied via the reaction 48 Ca( 18 O, 15 O) 51 Ca at a beam energy of 108 MeV. Recoiling 51 Ca nuclei were detected in coincidence with 15 O ejectiles, largely removing the substantial background from target contaminants that was encountered in previous work. The lowest 51 Ca level identified is 1.01 ±0.11 MeV less bound than the ground state, according to a recent measurement of the ground state mass using the 48 Ca( 14 C, 11 C) 51 Ca reaction. Consider- ations of the difficulty in identifying the ground state peak suggest that published values of the mass excess should be viewed with caution, and that a definitive mass measurement is still required in order to resolve questions on the structure of the neutron-rich calcium isotopes. A total of six energy levels in 51 Ca have been identified, and their mass excesses measured. Only two of these levels have been observed previously, via the ( 14 C, 11 C) reaction. Striking differences in selectivity between the ( 18 O, 15 O) and ( 14 C, 11 C) transfer reactions are discussed.

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L.K. Fifield

Australian National University

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C.L. Woods

Australian National University

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N.A. Orr

Australian National University

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T.R. Ophel

Australian National University

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D.C. Weisser

Australian National University

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R.J. Sadleir

Australian National University

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A.B. Harding

Australian National University

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C.S. Lim

Australian National University

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F. C. Barker

Australian National University

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G.P. Clarkson

Australian National University

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