Proceedings of the International School of Physics "Enrico Fermi.", Volume 69N. Zanichelli, 1977 - Nuclear physics |
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Page 5
They can be extended to deformations that are invariant with respect to any
subgroup of the full rotation group . One may also consider a combination of
rotation with other symmetry operations , such as space and time reflection . For
example ...
They can be extended to deformations that are invariant with respect to any
subgroup of the full rotation group . One may also consider a combination of
rotation with other symmetry operations , such as space and time reflection . For
example ...
Page 16
The highly excited states on the yrast line are unstable with respect to particle
emission ( nucleons and a - particles in particular ) . If the particle carries away 1
units of angular momentum , the reduction in rotational energy gives an effective
...
The highly excited states on the yrast line are unstable with respect to particle
emission ( nucleons and a - particles in particular ) . If the particle carries away 1
units of angular momentum , the reduction in rotational energy gives an effective
...
Page 19
The Coriolis term proportional to ji violates the assumed axial symmetry and time
reversal in variance of H . , but the Hamiltonian ( 32 ) remains invariant with
respect to space reflection P and with respect to a rotation R = R ( 1 ) of 180°
about ...
The Coriolis term proportional to ji violates the assumed axial symmetry and time
reversal in variance of H . , but the Hamiltonian ( 32 ) remains invariant with
respect to space reflection P and with respect to a rotation R = R ( 1 ) of 180°
about ...
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Contents
A BOHR Some aspects of rotational motion | 3 |
B R MOTTELSON Elementary excitations in the nucleus | 42 |
R BÉs and R A BROGLIA Nuclear superfluidity | 55 |
Copyright | |
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addition angular momentum appears approximation associated backbending band calculated closed collective compared comparison components configurations considered contributions corresponding coupling cross-sections deformation density dependence describe determined discussed distribution effects electron equations estimate evidence example excitation energy expected experiment experimental expression fact factor field given gives ground Hamiltonian hole included increase indicate inertia interaction Lett levels limit mass matrix elements measured modes moments motion neutron Nucl nuclear nuclei nucleons observed obtained operator orbits oscillator pairing parameters particle particular peak Phys physical possible potential predictions present processes protons quadrupole reaction region relation relative resonance respect rotational rule scattering seen shape shell model shown in fig shows simple single single-particle space spectra spectrum strength structure surface symmetry theory tion transfer transition values vibrational wave functions