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      Ewald Sums for One Dimension

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          Abstract

          We derive analytic solutions for the potential and field in a one-dimensional system of masses or charges with periodic boundary conditions, in other words Ewald sums for one dimension. We also provide a set of tools for exploring the system evolution and show that it's possible to construct an efficient algorithm for carrying out simulations. In the cosmological setting we show that two approaches for satisfying periodic boundary conditions, one overly specified and the other completely general, provide a nearly identical clustering evolution until the number of clusters becomes small, at which time the influence of any size-dependent boundary cannot be ignored. Finally we compare the results with other recent work with the hope of providing clarification over differences these issues have induced. We explain that modern formulations of physics require a well defined potential which is not available if the forces are screened directly.

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          Statistical mechanics and dynamics of solvable models with long-range interactions

          The two-body potential of systems with long-range interactions decays at large distances as \(V(r)\sim 1/r^\alpha\), with \(\alpha\leq d\), where \(d\) is the space dimension. Examples are: gravitational systems, two-dimensional hydrodynamics, two-dimensional elasticity, charged and dipolar systems. Although such systems can be made extensive, they are intrinsically non additive. Moreover, the space of accessible macroscopic thermodynamic parameters might be non convex. The violation of these two basic properties is at the origin of ensemble inequivalence, which implies that specific heat can be negative in the microcanonical ensemble and temperature jumps can appear at microcanonical first order phase transitions. The lack of convexity implies that ergodicity may be generically broken. We present here a comprehensive review of the recent advances on the statistical mechanics and out-of-equilibrium dynamics of systems with long-range interactions. The core of the review consists in the detailed presentation of the concept of ensemble inequivalence, as exemplified by the exact solution, in the microcanonical and canonical ensembles, of mean-field type models. Relaxation towards thermodynamic equilibrium can be extremely slow and quasi-stationary states may be present. The understanding of such unusual relaxation process is obtained by the introduction of an appropriate kinetic theory based on the Vlasov equation.
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            SIMULATIONS OF STRUCTURE FORMATION IN THE UNIVERSE

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              One-Dimensional Plasma Model at Thermodynamic Equilibrium

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                Author and article information

                Journal
                18 July 2010
                2010-09-26
                Article
                10.1103/PhysRevE.82.066203
                1007.3055
                c103b20b-7142-415a-ab68-470255dac403

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

                History
                Custom metadata
                2 figures added references expanded discussion of algorithm corrected figures added discussion of screened force
                math-ph astro-ph.CO cond-mat.stat-mech math.MP

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