837 research outputs found

    Another New Solvable Many-Body Model of Goldfish Type

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    A new solvable many-body problem is identified. It is characterized by nonlinear Newtonian equations of motion ("acceleration equal force") featuring one-body and two-body velocity-dependent forces "of goldfish type" which determine the motion of an arbitrary number NN of unit-mass point-particles in a plane. The NN (generally complex) values zn(t)z_{n}(t) at time tt of the NN coordinates of these moving particles are given by the NN eigenvalues of a time-dependent N×NN\times N matrix U(t)U(t) explicitly known in terms of the 2N initial data zn(0)z_{n}(0) and z˙n(0)\dot{z}_{n}(0). This model comes in two different variants, one featuring 3 arbitrary coupling constants, the other only 2; for special values of these parameters all solutions are completely periodic with the same period independent of the initial data ("isochrony"); for other special values of these parameters this property holds up to corrections vanishing exponentially as tt\rightarrow \infty ("asymptotic isochrony"). Other isochronous variants of these models are also reported. Alternative formulations, obtained by changing the dependent variables from the NN zeros of a monic polynomial of degree NN to its NN coefficients, are also exhibited. Some mathematical findings implied by some of these results - such as Diophantine properties of the zeros of certain polynomials - are outlined, but their analysis is postponed to a separate paper

    Isochronous solutions of Einstein's equations and their Newtonian limit

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    It has been recently demonstrated that it is possible to construct isochronous cosmologies, extending to general relativity a result valid for non-relativistic Hamiltonian systems. In this paper we review these findings and we discuss the Newtonian limit of these isochronous spacetimes, showing that it reproduces the analogous findings in the context of non-relativistic dynamics.Comment: arXiv admin note: text overlap with arXiv:1406.715

    Solvable Nonlinear Evolution PDEs in Multidimensional Space

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    A class of solvable (systems of) nonlinear evolution PDEs in multidimensional space is discussed. We focus on a rotation-invariant system of PDEs of Schr\"odinger type and on a relativistically-invariant system of PDEs of Klein-Gordon type. Isochronous variants of these evolution PDEs are also considered.Comment: This is a contribution to the Vadim Kuznetsov Memorial Issue on Integrable Systems and Related Topics, published in SIGMA (Symmetry, Integrability and Geometry: Methods and Applications) at http://www.emis.de/journals/SIGMA

    Isochronous Spacetimes

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    The possibility has been recently demonstrated to manufacture (nonrelativistic, Hamiltonian) many-body problems which feature an isochronous time evolution with an arbitrarily assigned period TT yet mimic with good approximation, or even exactly, any given many-body problem (within a quite large class, encompassing most of nonrelativistic physics) over times T~\tilde{T} which may also be arbitrarily large (but of course such that T~<T\tilde{T}<T). In this paper we review and further explore the possibility to extend this finding to a general relativity context, so that it becomes relevant for cosmology.Comment: Submitted to Acta Appl. Mat
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