New lump-like structures in models with hyperbolic interactions

2019 ◽  
Vol 34 (01) ◽  
pp. 1950002
Author(s):  
D. A. Ferreira

We investigate lump-like solutions in models described by a single real scalar field with non-polynomial interactions in (1, 1) dimensions. We start with a model that supports kink-like solutions and then use the deformation procedure to obtain families of models with hyperbolic interactions. The results show that depending on the values of the parameters, the models can support lump-like and kink-like solutions. We illustrate our findings, constructing new models and examining their solutions, energy densities, stability potentials and zero modes.

2014 ◽  
Vol 29 (24) ◽  
pp. 1450141 ◽  
Author(s):  
Merab Gogberashvili ◽  
Pavle Midodashvili

In this paper, we investigate localization problem for spinor fields within the (5D) standing wave braneworld with the bulk real scalar field and show that there exist normalizable fermion field zero modes on the brane.


2020 ◽  
Vol 29 (11) ◽  
pp. 2041016
Author(s):  
Carlos Herdeiro ◽  
Eugen Radu

We review recent results on the existence of static black holes (BHs) without spatial isometries in four spacetime dimensions and propose a general framework for their study. These configurations are regular on and outside a horizon of spherical topology. Two different mechanisms allowing for their existence are identified. The first one relies on the presence of a solitonic limit of the BHs; when the solitons have no spatial isometries, the BHs, being a nonlinear bound state between the solitons and a horizon, inherit this property. The second one is related to BH scalarization, and the existence of zero modes of the scalar field without isometries around a spherical horizon. When the zero modes have no spatial isometries, the back-reaction of their nonlinear continuation makes the scalarized BHs inherit the absence of spatial continuous symmetries. A number of general features of the solutions are discussed together with possible generalizations.


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.


2013 ◽  
Vol 350 (1) ◽  
pp. 381-384 ◽  
Author(s):  
Murli Manohar Verma ◽  
Shankar Dayal Pathak

2005 ◽  
Vol 37 (7) ◽  
pp. 1323-1330 ◽  
Author(s):  
Guanghai Guo ◽  
Yuanxing Gui ◽  
Jianxiang Tian
Keyword(s):  
The Real ◽  

2005 ◽  
Vol 37 (1) ◽  
pp. 243-251 ◽  
Author(s):  
Zu-Yao Sun ◽  
You-Gen Shen
Keyword(s):  

1990 ◽  
Vol 330 (1) ◽  
pp. 225-260 ◽  
Author(s):  
I-Hsiu Lee ◽  
Junko Shigemitsu ◽  
Robert E. Shrock

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