scholarly journals Cosmological Formation of (2 + 1)-Dimensional Soliton Structures in Models Possessing Potentials with Local Peaks

Physics ◽  
2021 ◽  
Vol 3 (3) ◽  
pp. 563-568
Author(s):  
Boris S. Murygin ◽  
Alexander A. Kirillov ◽  
Valery V. Nikulin

Production of domain walls and string-like solitons in the model with two real scalar fields and potential with at least one saddle point and a local maximum is considered. The model is regarded as 2-dimensional spatial slices of 3-dimensional entire structures. It is shown that, in the early Universe, both types of solitons may appear. In addition, the qualitative estimate of the domain walls and strings formation probabilities is presented. It is found that the probability of the formation of string-like solitons is suppressed compared to that of domain walls.


2004 ◽  
Vol 19 (04) ◽  
pp. 575-592 ◽  
Author(s):  
D. BAZEIA ◽  
A. S. INÁCIO ◽  
L. LOSANO

We investigate several models described by real scalar fields, searching for topological defects, and investigating their linear stability. We also find bosonic zero modes and examine the thermal corrections at the one-loop level. The classical investigations are of direct interest to high energy physics and to applications in condensed matter, in particular to spatially extended systems where fronts and interfaces separating different phase states may appear. The thermal investigations show that the finite temperature corrections that appear in a specific model induce a second-order phase transition in the system, although the thermal effects do not suffice to fully restore the symmetry at high temperature.



Author(s):  
D. Bazeia ◽  
A. S. Lobão ◽  
L. Losano ◽  
R. Menezes


2002 ◽  
Vol 32 (4) ◽  
pp. 869-879 ◽  
Author(s):  
Dionisio Bazeia
Keyword(s):  


1999 ◽  
Vol 1999 (04) ◽  
pp. 028-028 ◽  
Author(s):  
Dionisio Bazeia ◽  
Henrique Boschi-Filho ◽  
Francisco A Brito
Keyword(s):  


Author(s):  
A. Cabo Montes de Oca ◽  
D. Suarez Fontanella

Static (not stationary) solutions of the Einstein–Klein–Gordon (EKG) equations including matter are obtained for real scalar fields. The scalar field interaction with matter is considered. The introduced coupling allows the existence of static solutions in contraposition with the case of the simpler EKG equations for real scalar fields and gravity. Surprisingly, when the considered matter is a photon-like gas, it turns out that the gravitational field intensity at large radial distances becomes nearly a constant, exerting an approximately fixed force to small bodies at any distance. The effect is clearly related with the massless character of the photon-like field. It is also argued that the gravitational field can generate a bounding attraction, that could avoid the unlimited increase in mass with the radius of the obtained here solution. This phenomenon, if verified, may furnish a possible mechanism for explaining how the increasing gravitational potential associated to dark matter, finally decays at large distances from the galaxies. A method for evaluating these photon bounding effects is just formulated in order to be further investigated.



2009 ◽  
Vol 79 (8) ◽  
Author(s):  
P. P. Avelino ◽  
D. Bazeia ◽  
R. Menezes ◽  
J. C. R. E. Oliveira
Keyword(s):  


2004 ◽  
Vol 19 (supp02) ◽  
pp. 82-91 ◽  
Author(s):  
P. BOWCOCK ◽  
E. CORRIGAN ◽  
C. ZAMBON

Some ideas and remarks are presented concerning a possible Lagrangian approach to the study of internal boundary conditions relating integrable fields at the junction of two domains. The main example given in the article concerns single real scalar fields in each domain and it is found that these may be free, of Liouville type, or of sinh-Gordon type.



2002 ◽  
Vol 17 (29) ◽  
pp. 1945-1953 ◽  
Author(s):  
D. BAZEIA ◽  
W. FREIRE ◽  
L. LOSANO ◽  
R. F. RIBEIRO

We deal with the presence of topological defects in models for two real scalar fields. We comment on defects hosting topological defects and search for explicit defect solutions using the trial orbit method. As we know, under certain circumstances the second-order equations of motion can be solved by solutions of first-order differential equations. In this case we show that the trial orbit method can be used very efficiently to obtain explicit solutions.



2004 ◽  
Vol 2004 (05) ◽  
pp. 004-004 ◽  
Author(s):  
David H Lyth ◽  
Takeo Moroi


1982 ◽  
Vol 48 (17) ◽  
pp. 1156-1159 ◽  
Author(s):  
P. Sikivie
Keyword(s):  


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