scholarly journals Field modified spin–orbit potential curves of IBr. Preliminary dynamical results

2019 ◽  
Vol 21 (26) ◽  
pp. 14429-14439 ◽  
Author(s):  
Cristina Sanz-Sanz ◽  
Graham A. Worth
Keyword(s):  
Spin Orbit ◽  
Preliminary Results ◽  
Seminal Work ◽  
Orbit Potential ◽  
Dissociation Dynamics ◽  
Potential Curves

We revisit the seminal work on the control of IBr photodissociation using a strong non-resonant IR pulse, calculating the full 36-state manifold of spin–orbit coupled states. Preliminary results on the eld-driven IBr dissociation dynamics are presented.

scholarly journals Contribution of the ρ meson and quark substructure to the nuclear spin-orbit potential

2020 ◽  
Vol 102 (2) ◽  
Author(s):  
Guy Chanfray ◽  
Jérôme Margueron
Keyword(s):  
Nuclear Spin ◽  
Spin Orbit ◽  
Orbit Potential ◽  
Quark Substructure

The Spin-Orbit Potential in Proton-Proton Scattering

1960 ◽  
Vol 76 (6) ◽  
pp. 1002-1002
Author(s):  
D W L Sprung ◽  
J B Willis
Keyword(s):  
Proton Scattering ◽  
Spin Orbit ◽  
Proton Proton ◽  
Orbit Potential

Microscopic spin-orbit potential for p +6He elastic scattering

2019 ◽  
Vol 28 (09) ◽  
pp. 1950074
Author(s):  
Zakaria M. M. Mahmoud ◽  
Awad A. Ibraheem ◽  
M. A. Hassanain
Keyword(s):  
Experimental Data ◽  
Elastic Scattering ◽  
Cross Sections ◽  
Optical Model ◽  
Spin Orbit ◽  
Current Form ◽  
Density Distributions ◽  
Orbit Potential ◽  
Scattering Cross Sections ◽  
Good Agreement

In this work, we simultaneously reanalyzed the differential elastic scattering cross-sections ([Formula: see text]) and the vector analyzing power ([Formula: see text]) of [Formula: see text]He elastic scattering. This analysis was performed using the folded optical model for both real central and spin-orbit (SO) potentials, respectively. For the imaginary central, we used the usual Woods-Saxon (WS) form. Three different model density distributions are used to calculate the potential. We aimed to examine the applicability of the microscopically derived SO potential and the structure effect of 6He nucleus. The presence of the [Formula: see text] experimental data of [Formula: see text]He makes it interesting for this study. Our calculations showed that the three densities gave similar predictions for the cross-sections data. The three microscopic SO potentials calculations of [Formula: see text] are not in a good agreement with the experimental data. We concluded that the SO formalism in its current form needs more investigations for exotic halo nuclei.

scholarly journals Attractive Spin-Orbit Potential from the Skyrme Model

2020 ◽  
Vol 125 (4) ◽  
Author(s):  
Chris Halcrow ◽  
Derek Harland
Keyword(s):  
Skyrme Model ◽  
Spin Orbit ◽  
Orbit Potential

Mixing of parity of a nucleon pair at the nuclear surface due to the spin-orbit potential inF18

2014 ◽  
Vol 90 (5) ◽  
Author(s):  
Yoshiko Kanada-En'yo ◽  
Fumiharu Kobayashi
Keyword(s):  
Nucleon Pair ◽  
Nuclear Surface ◽  
Spin Orbit ◽  
Orbit Potential

scholarly journals A Survey of Stellar Families: Multiplicity Among Solar-type Stars

2006 ◽  
Vol 2 (S240) ◽  
pp. 254-257
Author(s):  
Deepak Raghavan ◽  
H. A. McAlister ◽  
T. J. Henry ◽  
B. D. Mason
Keyword(s):  
Survey Methods ◽  
Sample Survey ◽  
Accurate Mass ◽  
Mass Determination ◽  
Multiple Star ◽  
Preliminary Results ◽  
Seminal Work ◽  
Comprehensive Survey ◽  
Solar Type ◽  
Targeted Observations

AbstractStellar multiplicity is a fundamental astrophysical property. In addition to being the only physical basis for accurate mass determination, this parameter is believed to influence important aspects such as planet formation and stability. Contrary to earlier expectations, recent studies have shown that even against selection biases, as many as 23% of the planetary systems reside in multiple star systems (Raghavan et al. 2006)). Leveraging recent efforts in identifying stellar and substellar companions to solar-type stars, and augmenting them with targeted observations, we are conducting a comprehensive survey, aimed at providing a modern update to the seminal work of Duquennoy & Mayor (1991). The details of our sample, survey methods, and some preliminary results are presented here.

The shape of the nuclear spin-orbit potential

1995 ◽  
Vol 350 (4) ◽  
pp. 285-286 ◽  
Author(s):  
G. Mairle
Keyword(s):  
Nuclear Spin ◽  
Spin Orbit ◽  
Orbit Potential

Effect of the spin-orbit potential on the single particle levels in the superheavy region

1979 ◽  
Vol 83 (3-4) ◽  
pp. 279-283 ◽  
Author(s):  
Y. Tanaka ◽  
Y. Oda ◽  
F. Petrovich ◽  
R.K. Sheline
Keyword(s):  
Single Particle ◽  
Spin Orbit ◽  
Orbit Potential

scholarly journals The spin-orbit potential and Poincaré invariance in finite temperature pNRQCD

2011 ◽  
Vol 2011 (7) ◽  
Author(s):  
Nora Brambilla ◽  
Miguel Ángel Escobedo ◽  
Jacopo Ghiglieri ◽  
Antonio Vairo
Keyword(s):  
Finite Temperature ◽  
Spin Orbit ◽  
Orbit Potential
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