J.C. Peng
University of Pittsburgh
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Physics Letters B | 1979
W.J. Jordan; J.V. Maher; J.C. Peng
Abstract Complete fusion cross sections have been measured for the systems 12 C and 16 O + 28,29,30 Si in the energy ranges 20 MeV ⩽ E 12 C 49 MeV and 21 MeV ⩽ E 16 O ⩽ 61 MeV . Weak structure is observed in the 12 C + 28 Si excitation function while the remaining five systems exhibit an energy dependence which is consistent with smooth behavior. Maximum fusion cross sections for 12 C + 28 Si and 16 O + 28 Si are measured to be ≈ 1000 mb while those for 29,30 Si peak at ≈ 1200 mb. Data have been analyzed in terms of the Bass model and the model of Glas and Mosel.
Physics Letters B | 1978
J.C. Peng; J.V. Maher; M.S. Chiou; W.J. Jordan; F.C. Wang; M.W. Wu
Abstract Oscillatory structure appears in 28 Si( 16 O, 12 C) excitation functions populating the ground state and first excited state of 32 S over a range of center-of-mass bombarding energy from 22.3 MeV to 32.5 MeV. This structure is weaker in magnitude and less regular than that previously reported for 24 Mg( 16 O, 12 C) excitation functions. The structure in the 28 Si → 32 S ground state excitation function does not correlate with entrance or exit channel elastic scattering excitation functions, but it does correlate with some of the structure observed in excitation functions for 28 Si( 16 O, 16 O) 28 Si ∗ (2 + ). At most bombarding energies the 28 Si → 32 S ground state transition shows angular distributions which are dominated by one grazing partial wave (which can be calculated with the sample semiclassical Frahn-Venter model), but in two narrow energy ranges the angular distributions shift abruptly to oscillatory shapes which are not dominated by the grazing partial wave.
Nuclear Physics | 1980
J.C. Peng; H. Song; F.C. Wang; J. V. Maher
Abstract A CCBA (coupled-channels Born approximation) analysis has been performed on a very large set of rare-earth (d, t) transitions. Calculations were performed for states in 159 Gd, 161, 163 Dy and 165, 167 Er which have been identified as members of rotational bands built on the Nilsson single- hole states 11 2 − [505], 1 2 − [521], 3 2 − [521], 5 2 − [523], 5 2 + [642], 5 2 + [633] and 7 2 + [404]. In the cases where the DWBA works well, the CCBA gives results similar to those of DWBA. For the anomalous transitions the CCBA calculations tend to fit better than do the DWBA calculations — but the overall agreement is still rather poor.
Physical Review C | 1979
C.M. Cheng; J.V. Maher; M. S. Chiou; W.J. Jordan; J.C. Peng; W. Oelert; G.D. Gunn; F. D. Snyder
/sup 12/C + /sup 28/Si elastic scattering angular distributions have been measured at twenty-three bombarding energies over a range 19 MeV < or = E/sub lab/ < or = 48 MeV. At energies below 30 MeV the angular distributions are smooth and can be reproduced with a wide variety of optical potentials; similarly, above 40 MeV the angular distributions exhibit diffraction oscillations which optical potentials can rather easily reproduce. Irregular structure is observed in the cross sections for angles larger than 50/sup 0/ in the bombarding energy range 30--40 MeV. No optical potential has been found to give a good account of all the data; the best potential is a surface transparent Woods-Saxon potential which has energy dependences for both real and imaginary well depths. Examination of potentials which give reasonably good fits to the 36 MeV data shows that, although these potentials agree on a real well depth at a reasonable strong absorption radius, they can have quite different Argand diagrams: even in the range of the most sensitive partial waves. A Regge analysis finds several equally good families of Regge parameters for the same choice of background potential, but larger angle data might allow this ambiguity to bemorexa0» lifted. A Breit-Wigner analysis gives results which are at least partially consistent with the resonance parameters reported by Ost et al. Coupled-channel calculations with a 20% reduction of real and imaginary optical model well depths give a good account of inelastic scattering to the /sup 28/Si 2/sup +/ state while leaving the elastic scattering essentially unchanged from the predictions of the unmodified one-channel optical model. In the energy range of this study the grazing partial wave is found to be the same as the most important exit channel partial wave of the /sup 24/Mg(/sup 16/O,/sup 12/C)/sup 28/Si ground state transition.«xa0less
Physical Review C | 1979
C.M. Cheng; J.V. Maher; Chiou; W.J. Jordan; J.C. Peng; W. Oelert; G.D. Gunn; Franklin D. Snyder
/sup 12/C + /sup 28/Si elastic scattering angular distributions have been measured at twenty-three bombarding energies over a range 19 MeV < or = E/sub lab/ < or = 48 MeV. At energies below 30 MeV the angular distributions are smooth and can be reproduced with a wide variety of optical potentials; similarly, above 40 MeV the angular distributions exhibit diffraction oscillations which optical potentials can rather easily reproduce. Irregular structure is observed in the cross sections for angles larger than 50/sup 0/ in the bombarding energy range 30--40 MeV. No optical potential has been found to give a good account of all the data; the best potential is a surface transparent Woods-Saxon potential which has energy dependences for both real and imaginary well depths. Examination of potentials which give reasonably good fits to the 36 MeV data shows that, although these potentials agree on a real well depth at a reasonable strong absorption radius, they can have quite different Argand diagrams: even in the range of the most sensitive partial waves. A Regge analysis finds several equally good families of Regge parameters for the same choice of background potential, but larger angle data might allow this ambiguity to bemorexa0» lifted. A Breit-Wigner analysis gives results which are at least partially consistent with the resonance parameters reported by Ost et al. Coupled-channel calculations with a 20% reduction of real and imaginary optical model well depths give a good account of inelastic scattering to the /sup 28/Si 2/sup +/ state while leaving the elastic scattering essentially unchanged from the predictions of the unmodified one-channel optical model. In the energy range of this study the grazing partial wave is found to be the same as the most important exit channel partial wave of the /sup 24/Mg(/sup 16/O,/sup 12/C)/sup 28/Si ground state transition.«xa0less
Physical Review C | 1979
C.M. Cheng; J.V. Maher; W.J. Jordan; F.D. Snyder; W. Oelert; J.C. Peng; Chiou; G.D. Gunn
/sup 12/C + /sup 28/Si elastic scattering angular distributions have been measured at twenty-three bombarding energies over a range 19 MeV < or = E/sub lab/ < or = 48 MeV. At energies below 30 MeV the angular distributions are smooth and can be reproduced with a wide variety of optical potentials; similarly, above 40 MeV the angular distributions exhibit diffraction oscillations which optical potentials can rather easily reproduce. Irregular structure is observed in the cross sections for angles larger than 50/sup 0/ in the bombarding energy range 30--40 MeV. No optical potential has been found to give a good account of all the data; the best potential is a surface transparent Woods-Saxon potential which has energy dependences for both real and imaginary well depths. Examination of potentials which give reasonably good fits to the 36 MeV data shows that, although these potentials agree on a real well depth at a reasonable strong absorption radius, they can have quite different Argand diagrams: even in the range of the most sensitive partial waves. A Regge analysis finds several equally good families of Regge parameters for the same choice of background potential, but larger angle data might allow this ambiguity to bemorexa0» lifted. A Breit-Wigner analysis gives results which are at least partially consistent with the resonance parameters reported by Ost et al. Coupled-channel calculations with a 20% reduction of real and imaginary optical model well depths give a good account of inelastic scattering to the /sup 28/Si 2/sup +/ state while leaving the elastic scattering essentially unchanged from the predictions of the unmodified one-channel optical model. In the energy range of this study the grazing partial wave is found to be the same as the most important exit channel partial wave of the /sup 24/Mg(/sup 16/O,/sup 12/C)/sup 28/Si ground state transition.«xa0less
Physical Review C | 1979
G. P. A. Berg; M. A. G. Fernandes; K. Nagatani; J.C. Peng; B. Berthier; J. P. Fouan; J. Gastebois; J. P. Le Fèvre; M. C. Lemaire
Physical Review C | 1976
J.C. Peng; J.V. Maher; G. H. Wedberg; C.M. Cheng
Physical Review C | 1979
Cheng Chu; J. V. Maher; M. S. Chiou; W. J. Jordan; J.C. Peng; W. Oelert; G. D. Gunn; Franklin D. Snyder
Physical Review C | 1979
Cheng Chu; J. V. Maher; M. S. Chiou; W. J. Jordan; J.C. Peng; W. Oelert; G. D. Gunn; Franklin D. Snyder