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      Self-dual configurations in a generalized Abelian Chern-Simons-Higgs model with explicit breaking of the Lorentz covariance

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          Abstract

          We study a the existence of self-dual solitonic solutions in a generalization of the Abelian Chern-Simons-Higgs model. Such a generalization introduces two different nonnegative functions, \(\omega_1(|\phi|)\) and \(\omega(|\phi|)\), which split the kinetic term - \(|D_\mu\phi|^2 \rightarrow \omega_1 (|\phi|) |D_0\phi|^2-\omega(|\phi|) |D_k\phi|^2\) - of the Higgs field and break explicitly the Lorentz covariance. We have shown that a clean implementation of the Bogomolnyi procedure only can be implemented whether \(\omega \propto \beta |\phi|^{2\beta-2}\) with \(\beta\geq 1\). The self-dual or Bogomolnyi equations produce an infinity number of soliton solutions by choosing conveniently the generalizing function \(\omega_1(|\phi|)\) which must be able to provide a finite magnetic field. Among them we have selected the simplest ones which in some particular limits reproduce the Bogomolnyi equations of the Abelian Maxwell-Higgs and Chern-Simons-Higgs models. Finally, some new self-dual \(|\phi|^6\)-vortex solutions have been analyzed both from theoretical and numerical point of view.

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          Vortex-line models for dual strings

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            A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration

            Increasing evidence suggests that most of the energy density of the universe consists of a dark energy component with negative pressure, a ``cosmological constant" that causes the cosmic expansion to accelerate. In this paper, we address the puzzle of why this component comes to dominate the universe only recently rather than at some much earlier epoch. We present a class of theories based on an evolving scalar field where the explanation is based entirely on internal dynamical properties of the solutions. In the theories we consider, the dynamics causes the scalar field to lock automatically into a negative pressure state at the onset of matter-domination such that the present epoch is the earliest possible time, consistent with nucleosynthesis restrictions, when it can start to dominate.
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              Self-dual Chern-Simons vortices

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                Author and article information

                Journal
                2015-06-02
                2016-02-10
                Article
                10.1155/2016/5315649
                1506.01046
                4d346948-570d-4ad4-80b3-a1b087f08c8d

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Custom metadata
                7 pages, 5 .eps igures
                hep-th cond-mat.supr-con

                Condensed matter,High energy & Particle physics
                Condensed matter, High energy & Particle physics

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