scholarly journals Effect of the Pauli Principle and Channel Coupling on the Nuclear Reactions. II: Six-Nucleon System

1976 ◽  
Vol 55 (2) ◽  
pp. 471-481 ◽  
Author(s):  
H. Kanada ◽  
T. Kaneko ◽  
M. Nomoto
Keyword(s):  
Nuclear Reactions ◽  
Pauli Principle ◽  
Channel Coupling ◽  
Nucleon System

Test of the Pauli principle in nuclear reactions

1990 ◽  
Vol 252 (3) ◽  
pp. 487-490 ◽  
Author(s):  
Đ. Miljanić ◽  
G. Calvi ◽  
M. Lattuada ◽  
A. Ljubičić ◽  
C. Spitaleri ◽  
...  
Keyword(s):  
Nuclear Reactions ◽  
Pauli Principle

The Pauli Principle for Two Particles in a Dequantization Scheme Based on Coherent States

1983 ◽  
Vol 38 (10) ◽  
pp. 1049-1053
Author(s):  
B. Boll
Keyword(s):  
State Space ◽  
Weyl Group ◽  
Coherent States ◽  
Pauli Principle ◽  
Expectation Values ◽  
Permutational Symmetry ◽  
Nucleon System ◽  
Classical Trajectories

Abstract The expectation values of operators in state space between symmetrized or antisymmetrized coherent states associated with the Weyl group are introduced as classical functions. The dequantization scheme provided by these functions yields an interpretation of permutational symmetry for classical trajectories. The two-nucleon system is treated as an example.

Pauli principle and rearrangement collisions in unified theory of nuclear reactions

1968 ◽  
Vol 47 (2) ◽  
pp. 275-284 ◽  
Author(s):  
T.G Efimenko ◽  
B.N Zakhariev ◽  
V.P Zhigunov
Keyword(s):  
Nuclear Reactions ◽  
Pauli Principle ◽  
Unified Theory

Nuclear Processes Related to the Ap Stars and the Heaviest Chemical Elements

1976 ◽  
Vol 32 ◽  
pp. 169-182
Author(s):  
B. Kuchowicz
Keyword(s):  
Nuclear Physics ◽  
Nuclear Reactions ◽  
Chemical Elements ◽  
Fission Products ◽  
Abundance Pattern ◽  
Isotopic Shifts ◽  
Processed Material ◽  
R Process ◽  
Ap Stars ◽  
Nuclear Processes

SummaryIsotopic shifts in the lines of the heavy elements in Ap stars, and the characteristic abundance pattern of these elements point to the fact that we are observing mainly the products of rapid neutron capture. The peculiar A stars may be treated as the show windows for the products of a recent r-process in their neighbourhood. This process can be located either in Supernovae exploding in a binary system in which the present Ap stars were secondaries, or in Supernovae exploding in young clusters. Secondary processes, e.g. spontaneous fission or nuclear reactions with highly abundant fission products, may occur further with the r-processed material in the surface of the Ap stars. The role of these stars to the theory of nucleosynthesis and to nuclear physics is emphasized.

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