Double polarized neutron-proton scattering and nucleon-nucleon tensor force: An alternative analysis

2002 ◽  
Vol 65 (4) ◽  
Author(s):  
W. Tornow ◽  
C. R. Gould ◽  
D. G. Haase ◽  
J. R. Walston ◽  
B. W. Raichle
1999 ◽  
Vol 83 (14) ◽  
pp. 2711-2714 ◽  
Author(s):  
B. W. Raichle ◽  
C. R. Gould ◽  
D. G. Haase ◽  
M. L. Seely ◽  
J. R. Walston ◽  
...  

1995 ◽  
Vol 52 (5) ◽  
pp. 2351-2361 ◽  
Author(s):  
W. S. Wilburn ◽  
C. R. Gould ◽  
D. G. Haase ◽  
P. R. Huffman ◽  
C. D. Keith ◽  
...  

1993 ◽  
Vol 71 (13) ◽  
pp. 1982-1985 ◽  
Author(s):  
W. S. Wilburn ◽  
C. R. Gould ◽  
D. G. Haase ◽  
P. R. Huffman ◽  
C. D. Keith ◽  
...  

2014 ◽  
Vol 112 (20) ◽  
Author(s):  
P. Adlarson ◽  
W. Augustyniak ◽  
W. Bardan ◽  
M. Bashkanov ◽  
F. S. Bergmann ◽  
...  

2019 ◽  
Vol 223 ◽  
pp. 01015
Author(s):  
Paolo Finelli ◽  
Matteo Vorabbi ◽  
Carlotta Giusti

In this work we study the performances of our microscopic optical potential [1, 2], derived from nucleon-nucleon chiral potentials at fifth order (N4LO), in comparison with those of a successful non-relativistic phenomenological optical potential in the description of elastic proton scattering data on tin and lead isotopes at energies around and above 200 MeV. Our results indicate that microscopic optical potentials derived from nucleon-nucleon chiral potentials at N4LO can provide reliable predictions for observables of stable and exotic nuclei, even at energies where the robustness of the chiral expansion starts to be questionable.


1990 ◽  
Vol 245 (3-4) ◽  
pp. 333-337 ◽  
Author(s):  
M. Clajus ◽  
P.M. Egun ◽  
W. Grüebler ◽  
P. Hautle ◽  
I. Slaus ◽  
...  

2021 ◽  
pp. 1-11
Author(s):  
M.K. Al-Sugheir ◽  
F.F. Mqbel

In this work, the static fluctuation approximation (SFA) is used to investigate the thermodynamic properties of spin-polarized neutron matter. The energy per particle, pressure, entropy per particle, specific heat capacity, and effective magnetic field are studied as functions of density, temperature, and polarization fraction. The Argonne v18 nucleon–nucleon potential is used here. It is found that the energy per particle, pressure, entropy per particle, and effective magnetic field increase as the density or temperature increases. Also, the energy per particle and pressure are linearly dependent on the quadratic spin polarization δ2. The system becomes more ordered as δ increases. Our calculations are found to be in good agreement with previously published results obtained with different many-body techniques, such as the lowest order constrained variational (LOCV) method, the Brueckner–Hartree–Fock (BHF) approach, and the Dirac–Brueckner–Hartree–Fock (DBHF) technique.


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