W. Dodge
National Institute of Standards and Technology
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Archive | 1994
G. A. Retzlaff; H.S. Caplan; Emil Hallin; D. M. Skopik; D. Beck; K.I. Blomqvist; G. Dodson; K. Dow; M. Farkhondeh; J. Flanz; S. B. Kowalski; W. Sapp; C.P. Sargent; D. Tieger; W. Turchinetz; Claude F. Williamson; W. Dodge; X. K. Maruyama; J. W. Lightbody; R. Goloskie; J. McCarthy; T. S. Ueng; R. R. Whitney; B. P. Quinn; S. A. Dytman; K.F. von Reden; R. Schiavilla; John Tjon
Inclusive inelastic electron scattering cross sections for 3H and 3He were measured for excitation energies below 18 MeV. For six values of the three-momentum transfer q in the range 0.88 < q < 2.87 fm−1, longitudinal and transverse response functions were determined. The experimental data are in good agreement with two recent calculations. One uses variational ground-state wave functions and the orthogonal correlated states method to describe the two- and three-body breakup channels. The other uses bound and continuum Faddeev wave functions for a simple central potential. The inclusion of final-state interactions (FSI) in the Faddeev continuum is found to be very important; inclusion of FSI changes the response functions in the threshold kinematics by a large amount, yielding excellent agreement with the data.
Capture gamma‐ray spectroscopy | 1991
G. Feldman; L. H. Kramer; H. R. Weller; Evans Hayward; W. Dodge
The 30Si(p↘,γ)31P reaction has been studied in the energy range Ep=20–36 MeV. A transition matrix element analysis of σ(θ) and σ(θ)Ay(θ ) at Ep=25.5 MeV reveals substantial E2 strength (σE2/σtot∼26%) in the (p,γ1) channel, in excess of a direct E2 capture estimate (∼7%). The energy dependence of Ay(90°) for γ1 shows a resonance structure which can be reproduced by a direct‐semidirect calculation including an E2 resonance (EIVGQR=38.6 MeV, ΓIVGQR=5.0 MeV, SIVGQR=50%) at the expected peak of the isovector giant quadrupole resonance built on the first excited state of 31P. Angular distributions of σ(θ) and σ(θ)Ay(θ) have also been obtained from the 89Y(p↘,γ)90Zr reaction at Ep=22.5 MeV. A preliminary analysis reveals large E2 contributions (∼28%) for the γ0 transition, as well as possible E3 strength.
Physical Review Letters | 1988
K. Dow; S. A. Dytman; D. Beck; Aron M. Bernstein; I. Blomqvist; H.S. Caplan; D. Day; M. Deady; P. Demos; W. Dodge; G. Dodson; Manouchehr Farkhondeh; J. Flanz; K. Giovanetti; R. Goloskie; Emil Hallin; Emanuel Knill; S. B. Kowalski; J. Lightbody; R. Lindgren; X.K. Maruyama; J. McCarthy; B. P. Quinn; G. A. Retzlaff; W. Sapp; C. P. Sargent; D. M. Skopik; D. Tieger; W. Turchinetz; T. S. Ueng
Physical Review C | 1987
O'Connell Js; W. Dodge; J. W. Lightbody; X. K. Maruyama; J.-O. Adler; K. Hansen; Bernd Schröder; Aron M. Bernstein; K.I. Blomqvist; Cottman Bh; J. Comuzzi; R. A. Miskimen; B. Quinn; Koch Jh; Ohtsuka N
Physical Review Letters | 1987
D. Beck; Aron M. Bernstein; I. Blomqvist; H.S. Caplan; D. Day; P. Demos; W. Dodge; G. Dodson; K. Dow; S. A. Dytman; Manouchehr Farkhondeh; J. Flanz; K. Giovanetti; R. Goloskie; Emil Hallin; Emanuel Knill; S. B. Kowalski; J. Lightbody; R. Lindgren; X.K. Maruyama; J. McCarthy; B. P. Quinn; G. A. Retzlaff; W. Sapp; C. P. Sargent; D. M. Skopik; D. Tieger; W. Turchinetz; T. S. Ueng; N. Videla
Physical Review C | 1994
G. A. Retzlaff; H.S. Caplan; Emil Hallin; D. M. Skopik; D. Beck; K.I. Blomqvist; G. Dobson; K. Dow; M. Farkhondeh; J. Flanz; S. B. Kowalski; W. Sapp; C. P. Sargent; Daniel Raymond Tieger; W. Turchinetz; Claude F. Williamson; W. Dodge; X. K. Maruyama; J. Lightbody; R. Goloskie; J. S. McCarthy; T. S. Ueng; R. R. Whitney; B. P. Quinn; S. A. Dytman; K.F. von Reden; R. Schiavilla; John Tjon
Physical Review C | 1993
Sarty Aj; Doss Kg; G. Feldman; Emil Hallin; R. E. Pywell; G. A. Retzlaff; D. M. Skopik; Weller Hr; W. Dodge; J. W. Lightbody; O'Connell Js; C.C. Chang
Physical Review C | 1993
R.M. Whitton; H. R. Weller; Evans Hayward; W. Dodge; S. Kuhn
Physical Review C | 1991
G. Feldman; L. H. Kramer; H. R. Weller; Evans Hayward; W. Dodge
Physical Review C | 1991
M. A. Godwin; Evans Hayward; G. Feldman; L. H. Kramer; H. R. Weller; W. Dodge