scholarly journals Light nuclei in the hadron resonance gas

2020 ◽  
Vol 29 (05) ◽  
pp. 2040001 ◽  
Author(s):  
Benjamin Dönigus
Keyword(s):  
Thermal Model ◽  
Binding Energies ◽  
Light Nuclei ◽  
Recent Developments ◽  
Model Approach

The description of the production of light (anti-)(hyper-)nuclei in a hadron resonance gas, or statistical-thermal model approach, has proven to be rather successful, despite the fact that the binding energies of these compound objects are small compared to the emitting fireball temperature. We summarize some recent developments and findings in this approach.

scholarly journals Quantum Monte Carlo Methods in Nuclear Physics: Recent Advances

2019 ◽  
Vol 69 (1) ◽  
pp. 279-305 ◽  
Author(s):  
J.E. Lynn ◽  
I. Tews ◽  
S. Gandolfi ◽  
A. Lovato
Keyword(s):  
Monte Carlo ◽  
Quantum Monte Carlo ◽  
Nuclear Physics ◽  
Degrees Of Freedom ◽  
Effective Field ◽  
Binding Energies ◽  
Neutron Matter ◽  
Light Nuclei ◽  
Medium Mass ◽  
Recent Developments

In recent years, the combination of precise quantum Monte Carlo (QMC) methods with realistic nuclear interactions and consistent electroweak currents, in particular those constructed within effective field theories (EFTs), has led to new insights in light and medium-mass nuclei, neutron matter, and electroweak reactions. For example, with the same chiral interactions, QMC calculations can reproduce binding energies and radii for light nuclei, n–α scattering phase shifts, and the neutron matter equation of state. This compelling new body of work has been made possible both by advances in QMC methods for nuclear physics, which push the bounds of applicability to heavier nuclei and to asymmetric nuclear matter, and by the development of local chiral EFT interactions up to next-to-next-to-leading order and minimally nonlocal interactions including Δ degrees of freedom. In this review, we discuss these recent developments and give an overview of the exciting results for nuclei, neutron matter and neutron stars, and electroweak reactions.

scholarly journals Thermal Model Approach to Multisector Three-Phase Electrical Machines

2021 ◽  
Vol 68 (4) ◽  
pp. 2919-2930 ◽  
Author(s):  
Hengliang Zhang ◽  
Paolo Giangrande ◽  
Giacomo Sala ◽  
Zeyuan Xu ◽  
Wei Hua ◽  
...  
Keyword(s):  
Thermal Model ◽  
Electrical Machines ◽  
Three Phase ◽  
Model Approach

scholarly journals The search for the origin of the light nuclei Li, Be, B

2009 ◽  
Vol 5 (S268) ◽  
pp. 469-471
Author(s):  
Hubert Reeves
Keyword(s):  
Nuclear Interaction ◽  
Binding Energies ◽  
Light Nuclei ◽  
Major Influence ◽  
Magic Numbers ◽  
Light Elements ◽  
Closed Shells

AbstractMy aim is to show how the abundance ratios of the light elements (6 to 11) are related to the properties of the strong nuclear interaction and, in particular, to the major influence of closed shells of neutrons and protons, (the magic numbers : 2, 8, etc) on the binding energies of the nuclei.

LEVEL DENSITIES IN LIGHTER NUCLEI

1965 ◽  
Vol 43 (7) ◽  
pp. 1248-1258 ◽  
Author(s):  
A. Gilbert ◽  
F. S. Chen ◽  
A. G. W. Cameron
Keyword(s):  
Excitation Energy ◽  
Ground State ◽  
Shell Structure ◽  
Mass Number ◽  
State Energy ◽  
Binding Energies ◽  
Light Nuclei ◽  
Cumulative Number ◽  
Additional Consideration ◽  
Level Densities

There has been discussion in the literature as to whether the cumulative number of levels in light nuclei varies more nearly as exp(const. [Formula: see text]) or exp(const. E), where E is the excitation energy. The question is examined in this paper. It is found that if one constructs "step diagrams" by plotting the cumulative number versus the energy, both formulas represent the data almost equally well. However, additional consideration of levels counted above neutron and proton binding energies shows that exp(const. [Formula: see text]) fails badly to represent the data, whereas exp(const. E) continues to give good fits. In either case E may be measured above an arbitrary ground-state energy E0. If the satisfactory formula is written in the form exp(E–E0)/T, then it is found that the dependence of the slope on mass number may be expressed in approximately the form T−1 = 0.0165A MeV−1, but there are significant deviations from this relation apparently related to shell structure. The intercepts E0 are quite variable but are roughly clustered according to the oddness or evenness of the neutron and proton numbers of the nucleus.

On the Binding Energies of Light Nuclei

1951 ◽  
Vol 83 (3) ◽  
pp. 663-663 ◽  
Author(s):  
Jyumpei Sanada ◽  
Yasukazu Yoshizawa
Keyword(s):  
Binding Energies ◽  
Light Nuclei

scholarly journals On the Binding Energies of Very Light Nuclei

1955 ◽  
Vol 14 (5) ◽  
pp. 490-492
Author(s):  
Shôta Suekane ◽  
Wataro Watari
Keyword(s):  
Binding Energies ◽  
Light Nuclei
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