Nuclear structure of neutron-rich nuclei from magnetic moments measurements

1998 ◽  
Author(s):  
Alex Wolf
2020 ◽  
Vol 16 (1) ◽  
pp. 34-37
Author(s):  
Meng-Hock Koh ◽  
Nurhafiza Mohamad Nor ◽  
Nor-Anita Rezle ◽  
Kai-Wen Kelvin Lee ◽  
Philippe Quentin ◽  
...  

Nuclear structure data plays an important role in nuclear physics studies and applications such as nuclear power generation. This article presents evaluations of a mean-field approach to describe two nuclear structure quantities namely the electric and magnetic moments. The Hartree-Fock-plus-pairing approach was employed with pairing correlations treated within the Bardeen-Cooper-Schrieffer (BCS) framework. The Skyrme SIII parametrization and seniority force are chosen to approximate the effective nucleon-nucleon and pairing interactions, respectively. Calculated results show that the self-consistent blocking procedure which takes into account time-reversal symmetry breaking is important to reproduce experimental magnetic moment


2019 ◽  
Vol 18 (1) ◽  
pp. 21-46 ◽  
Author(s):  
U V S Seshavatharam ◽  
S Lakshminarayana

This paper attempts to understand the role of the four gravitational constants in the nuclear structure whichhelps in understanding the nuclear elementary charge, the strong coupling constant, nuclear charge radii,nucleon magnetic moments, nuclear stability, nuclear binding energy and Neutron life time. The three assumed atomic gravitational constants help in understanding neutron-proton stability. Electromagnetic and nuclear gravitational constants play a role in understanding proton-electron mass ratio, Bohr radius and characteristic atomic radius. With reference to the weak gravitational constant, it is possible to predict the existence of a weakly interacting fermion of rest energy 585 GeV, called Higg’s fermion. Cosmological ‘dark matter’ research and observations can be carried out in this direction also.


Particles ◽  
2021 ◽  
Vol 4 (1) ◽  
pp. 75-92
Author(s):  
R. Sahu ◽  
V. K. B. Kota ◽  
T. S. Kosmas

Detection rates for the elastic and inelastic scattering of weakly interacting massive particles (WIMPs) off 23Na are calculated within the framework of Deformed Shell Model (DSM) based on Hartree-Fock states. At first, the spectroscopic properties of the detector nucleus, like energy spectra and magnetic moments, are evaluated and compared with experimental data. Following the good agreement of these results, DSM wave functions are used for obtaining elastic and inelastic spin structure functions, nuclear structure coefficients and so forth for the WIMP-23Na scattering. Then, the event rates are also computed with a given set of supersymmetric parameters. In the same manner, using DSM wavefunctions, nuclear structure coefficients and event rates for elastic scattering of WIMPs from 40Ar are also obtained. These results for event rates and also for annual modulation will be useful for the ongoing and future WIMP detection experiments involving detector materials with 23Na and 40Ar nuclei.


1987 ◽  
Author(s):  
A. Wolf ◽  
R. F. Casten ◽  
R. L. Gill ◽  
D. S. Brenner ◽  
H. Mach ◽  
...  

2002 ◽  
Vol 49 (1) ◽  
pp. 91-154 ◽  
Author(s):  
K.-H. Speidel ◽  
O. Kenn ◽  
F. Nowacki

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