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      Particle-without-Particle: a practical pseudospectral collocation method for numerical differential equations with distributional sources

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          Abstract

          Differential equations with distributional sources---in particular, involving delta distributions and/or derivatives thereof---have become increasingly ubiquitous in numerous areas of physics and applied mathematics. It is often of considerable interest to obtain numerical solutions for such equations, but the singular ("point-like") modeling of the sources in these problems typically introduces nontrivial obstacles for devising a satisfactory numerical implementation. A common method to circumvent these is through some form of delta function approximation procedure on the computational grid, yet this strategy often carries significant limitations. In this paper, we present an alternative technique for tackling such equations: the "Particle-without-Particle" method. Previously introduced in the context of the self-force problem in gravitational physics, the idea is to discretize the computational domain into two (or more) disjoint pseudospectral (Chebyshev-Lobatto) grids in such a way that the "particle" (the singular source location) is always at the interface between them; in this way, one only needs to solve homogeneous equations in each domain, with the source effectively replaced by jump (boundary) conditions thereon. We prove here that this method is applicable to any linear PDE (of arbitrary order) the source of which is a linear combination of one-dimensional delta distributions and derivatives thereof supported at an arbitrary number of particles. We furthermore apply this method to obtain numerical solutions for various types of distributionally-sourced PDEs: we consider first-order hyperbolic equations with applications to neuroscience models (describing neural populations), parabolic equations with applications to financial models (describing price formation), second-order hyperbolic equations with applications to wave acoustics, and finally elliptic (Poisson) equations.

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          Strings and other distributional sources in general relativity

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            Gravitational Radiation Reaction to a Particle Motion

            In this paper, we discuss the leading order correction to the equation of motion of the particle, which presumably describes the effect of gravitational radiation reaction. We derive the equation of motion in two different ways. The first one is an extension of the well-known formalism by DeWitt and Brehme developed for deriving the equation of motion of an electrically charged particle. In contrast to the electromagnetic case, in which there are two different charges, i.e., the electric charge and the mass, the gravitational counterpart has only one charge. This fact prevents us from using the same renormalization scheme that was used in the electromagnetic case. To make clear the subtlety in the first approach, we then consider the asymptotic matching of two different schemes, i.e., the internal scheme in which the small particle is represented by a spherically symmetric black hole with tidal perturbations and the external scheme in which the metric is given by small perturbations on the given background geometry. The equation of motion is obtained from the consistency condition of the matching. We find that in both ways the same equation of motion is obtained. The resulting equation of motion is analogous to that derived in the electromagnetic case. We discuss implications of this equation of motion.
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              A review on the products of distributions

              C. J. LI (2024)
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                Author and article information

                Journal
                09 February 2018
                Article
                1802.03405
                6f2f79d2-9a24-461b-bce4-06b13adf03d3

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

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                Custom metadata
                50 pages, 11 figures
                physics.comp-ph gr-qc math.NA q-bio.NC q-fin.CP

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