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A self-consistent general relativistic configuration describing a finite cross-section magnetic flux tube is constructed. The cosmic solenoid is modeled by an elastic superconductive surface which separates the Melvin core from the surrounding flat conic structure. We show that a given amount $Phi$ of magnetic flux cannot be confined within a cosmic solenoid of circumferential radius smaller than $frac{sqrt{3G}}{2pi c^2}Phi$ without creating a conic singularity. Gauss-Codazzi matching conditions are derived by means of a self-consistent action. The source term, representing the surface currents, is sandwiched between internal and external gravitational surface terms. Surface superconductivity is realized by means of a Higgs scalar minimally coupled to projective electromagnetism. Trading the magnetic London phase for a dual electric surface vector potential, the generalized quantization condition reads: $e/{hc} Phi + 1/e Q=n$ with $Q$ denoting some dual electric charge, thereby allowing for a non-trivial Aharonov-Bohm effect. Our conclusions persist for dilaton gravity provided the dilaton coupling is sub-critical.
We find a method to rewrite the equations of motion of scalar fields, generalized DBI field and quintessence, in the autonomous form foremph{arbitrary} scalar potentials. With the aid of this method, we explore the cosmic evolution of generalized DBI
Following the path of minimalism in alternative theories of gravity, we construct the Minimal Theory of Bigravity (MTBG), a theory of two interacting spin-2 fields that propagates only four local degrees of freedom instead of the usual seven ones and
Although the idea that there is a maximum force in nature seems untenable, we explore whether this concept can make sense in the restricted context of black holes. We discuss uniformly accelerated and cosmological black holes and we find that, althou
Gravitationally coupled scalar fields, originally introduced by Jordan, Brans and Dicke to account for a non constant gravitational coupling, are a prediction of many non-Einsteinian theories of gravity not excluding perturbative formulations of Stri
In this paper we consider spherically symmetric general fluids with heat flux, motivated by causal thermodynamics, and give the appropriate set of conditions that define separating shells defining the divide between expansion and collapse. To do so w