Proton elastic scattering on light nuclei. II. Nuclear structure effects

1980 ◽  
Vol 21 (3) ◽  
pp. 844-860 ◽  
Author(s):  
E. Fabrici ◽  
S. Micheletti ◽  
M. Pignanelli ◽  
F. G. Resmini ◽  
R. De Leo ◽  
...  
Keyword(s):  
Elastic Scattering ◽  
Nuclear Structure ◽  
Light Nuclei ◽  
Proton Elastic Scattering

Nuclear structure ofSc43. IV. Proton elastic scattering and isobaric analog states

1974 ◽  
Vol 10 (5) ◽  
pp. 1678-1687 ◽  
Author(s):  
J. C. Manthuruthil ◽  
C. P. Poirier ◽  
S. Maripuu ◽  
W. A. Anderson
Keyword(s):  
Elastic Scattering ◽  
Nuclear Structure ◽  
Proton Elastic Scattering ◽  
Isobaric Analog

Systematics of Isospin Mixing in Proton Elastic Scattering from Light Nuclei

1976 ◽  
Vol 36 (23) ◽  
pp. 1357-1359 ◽  
Author(s):  
P. G. Ikossi ◽  
W. J. Thompson ◽  
T. B. Clegg ◽  
W. W. Jacobs ◽  
E. J. Ludwig
Keyword(s):  
Elastic Scattering ◽  
Light Nuclei ◽  
Proton Elastic Scattering

scholarly journals The Optical Model and Proton Elastic Scattering from 14N and 16O

1977 ◽  
Vol 30 (3) ◽  
pp. 287 ◽  
Author(s):  
A Gabric ◽  
K Amos
Keyword(s):  
Elastic Scattering ◽  
Optical Model ◽  
Model Potential ◽  
Light Nuclei ◽  
Projectile Energy ◽  
Strength Parameters ◽  
Proton Elastic Scattering ◽  
Doorway State ◽  
Optical Model Potential

Allowing for important doorway state effects in analyses of proton elastic scattering from the light nuclei 14N and 160 enables an average geometry optical model potential to be determined, the strength parameters of which show a smooth behaviour with projectile energy.

Proton elastic scattering on light nuclei. I. Energy dependence

1980 ◽  
Vol 21 (3) ◽  
pp. 830-843 ◽  
Author(s):  
E. Fabrici ◽  
S. Micheletti ◽  
M. Pignanelli ◽  
F. G. Resmini ◽  
R. De Leo ◽  
...  
Keyword(s):  
Elastic Scattering ◽  
Energy Dependence ◽  
Light Nuclei ◽  
Proton Elastic Scattering

scholarly journals NUCLEAR MEAN-FIELD DESCRIPTION OF PROTON ELASTIC SCATTERING BY 12,13 C AT LOW ENERGIES

2020 ◽  
Vol 31 (1) ◽  
Author(s):  
Huan Nhut Phan
Keyword(s):  
Elastic Scattering ◽  
Cross Sections ◽  
Nuclear Reactions ◽  
Mean Field ◽  
Nuclear Astrophysics ◽  
Nucleon Nucleon ◽  
Light Nuclei ◽  
Intermediate Energies ◽  
Proton Elastic Scattering ◽  
Low Energies

Nuclear reactions of proton by light nuclei at low energies play a key role in the study ofnucleosynthesis which is of interest in nuclear astrophysics. The most fundamental process whichis very necessary is the elastic scattering. In this work, we construct a microscopic proton-nucleuspotential in order to describe the differential cross-sections over scattering angles of the protonelastic scattering by 12C and 13C in the range of available energies 14 - 22 MeV. The microscopicoptical potential is based on the folding model using the effective nucleon-nucleon interactionCDM3Yn. The results show the promising use of the CDM3Yn interactions at low and very lowenergies, which were originally used for nuclear reactions at intermediate energies. This could bethe premise for the study of nuclear reactions using CDM3Yn interaction in astrophysics at lowenergies.

scholarly journals Nonlocal Structure of the Leading Order ab initio Effective Potentials for Proton Elastic Scattering from Light Nuclei

2022 ◽  
Vol 63 (1) ◽  
Author(s):  
Ch. Elster ◽  
M. Burrows ◽  
R. B. Baker ◽  
S. P. Weppner ◽  
K. D. Launey ◽  
...  
Keyword(s):  
Elastic Scattering ◽  
Ab Initio ◽  
Light Nuclei ◽  
Leading Order ◽  
Effective Potentials ◽  
Proton Elastic Scattering ◽  
Nonlocal Structure

Nuclear Electrons and Nuclear Structure

2018 ◽  
Author(s):  
Roger H. Stuewer
Keyword(s):  
Nuclear Structure ◽  
Beta Decay ◽  
Gamma Rays ◽  
Alpha Particle ◽  
Continuous Distribution ◽  
Alpha Particles ◽  
Light Nuclei ◽  
Coincidence Method ◽  
Wolfgang Pauli ◽  
Beta Particles

Serious contradictions to the existence of electrons in nuclei impinged in one way or another on the theory of beta decay and became acute when Charles Ellis and William Wooster proved, in an experimental tour de force in 1927, that beta particles are emitted from a radioactive nucleus with a continuous distribution of energies. Bohr concluded that energy is not conserved in the nucleus, an idea that Wolfgang Pauli vigorously opposed. Another puzzle arose in alpha-particle experiments. Walther Bothe and his co-workers used his coincidence method in 1928–30 and concluded that energetic gamma rays are produced when polonium alpha particles bombard beryllium and other light nuclei. That stimulated Frédéric Joliot and Irène Curie to carry out related experiments. These experimental results were thoroughly discussed at a conference that Enrico Fermi organized in Rome in October 1931, whose proceedings included the first publication of Pauli’s neutrino hypothesis.

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