Null SuperP-Branes Quantum Theory in 4-Dimensional Space-Time

1993 ◽  
Vol 41 (7) ◽  
pp. 619-676 ◽  
Author(s):  
I. A. Bandos ◽  
A. A. Zheltukhin
2019 ◽  
Author(s):  
Vitaly Kuyukov

Many approaches to quantum gravity consider the revision of the space-time geometry and the structure of elementary particles. One of the main candidates is string theory. It is possible that this theory will be able to describe the problem of hierarchy, provided that there is an appropriate Calabi-Yau geometry. In this paper we will proceed from the traditional view on the structure of elementary particles in the usual four-dimensional space-time. The only condition is that quarks and leptons should have a common emerging structure. When a new formula for the mass of the hierarchy is obtained, this structure arises from topological quantum theory and a suitable choice of dimensional units.


1991 ◽  
Vol 06 (14) ◽  
pp. 2497-2517 ◽  
Author(s):  
M.S. PLYUSHCHAY

The quantization of the massless Brink-Schwarz superparticle in four-dimensional space-time in terms of independent variables and by the Gupta-Bleuler method is developed. The connection between these two approaches to quantization of the model is retraced and covariantization of the latter one is realized. The properties of the system under spatial inversion are explored and the quantum theory which is invariant with respect to it is constructed.


1993 ◽  
Vol 41 (7) ◽  
pp. 619-676 ◽  
Author(s):  
I. A. Bandos ◽  
A. A. Zheltukhin

2019 ◽  
Vol 34 (08) ◽  
pp. 1950035
Author(s):  
Chun Yong Chew ◽  
Yong Kheng Goh

We study the electromagnetic Casimir interaction energy between two parallel concentric cylinders in [Formula: see text]-dimensional Minkowski space–time for different combinations of perfectly conducting boundary condition and infinitely permeable boundary condition. We consider two cases where one cylinder is outside each other and where one is inside the other. By solving the equation of motion and computing the TGTG formulas, explicit formulas for the Casimir interaction energy can be derived and asymptotic behavior of the Casimir interaction energy in the nanoregime is calculated by using perturbation technique. We computed the interaction energy analytically up to next-to-leading order term.


2008 ◽  
Vol 17 (08) ◽  
pp. 1179-1196 ◽  
Author(s):  
MARTÍN G. RICHARTE ◽  
CLAUDIO SIMEONE

We study spherically symmetric thin shell wormholes in a string cloud background in (3 + 1)-dimensional space–time. The amount of exotic matter required for the construction, the traversability and the stability of such wormholes under radial perturbations are analyzed as functions of the parameters of the model. In addition, in the appendices a nonperturbative approach to the dynamics and a possible extension of the analysis to a related model are briefly discussed.


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