scholarly journals Self-consistent variational approach to the minimal left-right symmetric model of electroweak interactions

2006 ◽  
Vol 74 (11) ◽  
Author(s):  
Fabio Siringo ◽  
Luca Marotta
Keyword(s):  
Variational Approach ◽  
Symmetric Model ◽  
Electroweak Interactions ◽  
Self Consistent

scholarly journals Evolution of inhomogeneous condensates: Self-consistent variational approach

1998 ◽  
Vol 58 (2) ◽  
Author(s):  
D. Boyanovsky ◽  
F. Cooper ◽  
H. J. de Vega ◽  
P. Sodano
Keyword(s):  
Variational Approach ◽  
Self Consistent

scholarly journals HOT NUCLEAR MATTER: A VARIATIONAL APPROACH

1992 ◽  
Vol 01 (02) ◽  
pp. 405-419 ◽  
Author(s):  
H. MISHRA ◽  
S. P. MISRA ◽  
P. K. PANDA ◽  
B. K. PARIDA
Keyword(s):  
Field Theory ◽  
Transition Temperature ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Finite Temperature ◽  
Variational Approach ◽  
Mass Shell ◽  
Zero Temperature ◽  
Self Consistent ◽  
Consistent Manner

We develop a nonperturbative technique in field theory to study properties of infinite nuclear matter at zero temperature as well as at finite temperatures. Here we dress the nuclear matter with off–mass shell pions. The techniques of thermofield dynamics are used for finite temperature calculations. Equation of state is derived from the dynamics of the interacting system in a self consistent manner. The transition temperature for nuclear matter appears to be around 15 MeV.

scholarly journals Towards a Self-consistent Model of a Galaxy

1987 ◽  
Vol 127 ◽  
pp. 509-510
Author(s):  
W.J.L.V. Durodie ◽  
F.D. Kahn
Keyword(s):  
Stellar Dynamics ◽  
Time Development ◽  
Symmetric Model ◽  
Spherically Symmetric ◽  
Stellar Orbits ◽  
Consistent Model ◽  
Galactic System ◽  
Self Consistent ◽  
Functional Distribution ◽  
Fundamental Equations

Using a theoretical model for the functional distribution of stars in phase space in a spherically symmetric galactic system, it is found upon solving the fundamental equations of stellar dynamics that the rotation curves produced by the model are flat for large distances within the system. the properties of the stellar orbits within such systems are investigated and an N-ring axially and equatorially symmetric model for simulating its dynamics is presented. Poisson's equation is solved by expanding density and potential in Legendre polynomials (c.f. van Albada and van Gorkom, 1977). It is helped to follow the time development of such a system under various forces.

scholarly journals Self-consistent 1/Ncexpansion in the presence of electroweak interactions

1996 ◽  
Vol 53 (9) ◽  
pp. 5105-5107 ◽  
Author(s):  
Chi-Keung Chow ◽  
Tung-Mow Yan
Keyword(s):  
Electroweak Interactions ◽  
Self Consistent
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