1,720,964 research outputs found

    On non-topological solutions for planar Liouville Systems of Toda-type

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    Motivated by the study of non-abelian Chern Simons vor- tices of non-topological type in Gauge Field Theory we analyse the solvability of some Liouville-type system in presence of singular sources We identify necessary and sufficient conditions which ensure the radial solvability of this system.Non UBCUnreviewedAuthor affiliation: Ben Gurion UniversityFacult

    Upper bounds for a class of energies containing a non-local term

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    In this paper we construct upper bounds for families of functionals of the form Eε(ϕ):=Ω(εϕ2+1εW(ϕ))dx+1εRNHˉF(ϕ)2dx E_\varepsilon(\phi):=\int_\Omega\Big(\varepsilon |\nabla\phi|^2+\frac{1}{\varepsilon }W(\phi)\Big){\rm d}x+\frac{1}{\varepsilon }\int_{{\mathbb{R}}^N}|\nabla \bar H_{F(\phi)}|^2{\rm d}x where Δ Hˉu\bar H_u = div {χΩ\chi_\Omega u}. Particular cases of such functionals arise in Micromagnetics. We also use our technique to construct upper bounds for functionals that appear in a variational formulation of the method of vanishing viscosity for conservation laws

    Approximations in Besov Spaces and Jump Detection of Besov Functions with Bounded Variation

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    In this paper, we provide a proof that functions belonging to Besov spaces Bq,r(RN,Rd)B^{r}_{q,\infty}(\mathbb{R}^N,\mathbb{R}^d), q[1,)q\in [1,\infty), r(0,1)r\in(0,1), satisfy the following formula under a certain condition: \begin{equation} \label{eq:main result in abstract} \lim_{{\epsilon}\to 0^+}\frac{1}{|\ln{\epsilon}|}\left[u_{\epsilon}\right]^q_{W^{r,q}(\mathbb{R}^N,\mathbb{R}^d)}=N\lim_{{\epsilon}\to 0^+}\int_{\mathbb{R}^N}\frac{1}{{\epsilon}^N}\int_{B_{\epsilon}(x)}\frac{|u(x)-u(y)|^q}{|x-y|^{rq}}dydx. \end{equation} Here, []Wr,q\left[\cdot\right]_{W^{r,q}} represents the Gagliardo seminorm, and uϵu_{\epsilon} denotes the convolution of uu with a mollifier η(ϵ)(x):=1ϵNη(xϵ)\eta_{(\epsilon)}(x):=\frac{1}{\epsilon^N}\eta\left(\frac{x}{\epsilon}\right), ηW1,1(RN),RNη(z)dz=1\eta\in W^{1,1}(\mathbb{R}^N),\int_{\mathbb{R}^N}\eta(z)dz=1. Furthermore, we prove that every function uu in BV(RN,Rd)Bp,1/p(RN,Rd),p(1,),BV(\mathbb{R}^N,\mathbb{R}^d)\cap B^{1/p}_{p,\infty}(\mathbb{R}^N,\mathbb{R}^d),p\in(1,\infty), satisfies \begin{multline} \lim_{\epsilon\to 0^+}\frac{1}{|\ln{\epsilon}|}\left[u_{\epsilon}\right]^q_{W^{1/q,q}(\mathbb{R}^N,\mathbb{R}^d)}=N\lim_{{\epsilon}\to 0^+}\int_{\mathbb{R}^N}\frac{1}{{\epsilon}^N}\int_{B_{\epsilon}(x)}\frac{|u(x)-u(y)|^q}{|x-y|}dydx =\left(\int_{S^{N-1}}|z_1|~d\mathcal{H}^{N-1}(z)\right)\int_{\mathcal{J}_u} \Big|u^+(x)-u^-(x)\Big|^q d\mathcal{H}^{N-1}(x), \end{multline} for every 1<q<p1<q<p. Here u+,uu^+,u^- are the one-sided approximate limits of uu along the jump set Ju\mathcal{J}_u

    Non-relativistic model of the laws of gravity and electromagnetism, invariant under the change of inertial and non-inertial coordinate systems

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    Under the classical non-relativistic consideration of the space-time we propose the model of the laws of gravity and Electrodynamics, invariant under the galilean transformations and moreover, under every change of non-inertial cartesian coordinate system. Being in the frames of non-relativistic model of the space-time, we adopt some general ideas of the General Theory of Relativity, like the assumption of invariance of the most general physical laws in every inertial and non-inertial coordinate system and equivalence of factious forces in non-inertial coordinate systems and the force of gravity. Moreover, in the frames of our model, we obtain that the laws of Non-relativistic Quantum Mechanics also invariant under the change of inertial or non-inertial cartesian coordinate system.This is a preprint of the following work: Arkady Poliakovsky, The Laws of Gravity and Electromagnetism: A Non-relativistic Model Invariant Under the Change of Inertial and Non-inertial Coordinate Systems , 2024, Springer Cham, reproduced with permission of Springer Nature Switzerland AG 2024. The final authenticated version is available online at: https://doi.org/10.1007/978-3-031-61407-

    Lorentzian geometrical structures with global time, Gravity and Electrodynamics

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    We investigate Lorentzian structures in the four-dimensional space-time, supplemented either by a covector field of the time-direction or by a scalar field of the global time. Furthermore, we propose a new metrizable model of the gravity. In contrast to the usual Theory of General Relativity where all ten components of the symmetric pseudo-metrics are independent variables, the presented here model of the gravity essentially depend only on single four-covector field, restricted to have only three-independent components. However, we prove that the Gravitational field, ruled by the proposed model and generated by some massive body, resting and spherically symmetric in some coordinate system, is given by a pseudo-metrics {Kmn}m,n=0,1,2,3, which coincides with the well known Schwarzschild metric from the General Relativity. The Maxwell equations and Electrodynamics are also investigated in the frames of the proposed model. In particular, we derive the covariant formulation of Electrodynamics of moving dielectrics and para/diamagnetic mediums
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