Papers › RelativisticDynamics.jl: Relativistic Spin-Orbital Dynamics in Julia
RelativisticDynamics.jl: Relativistic Spin-Orbital Dynamics in Julia
Tom Kimpson
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RelativisticDynamics.jl is an open-source Julia package for relativistic spin-orbital dynamics in the gravitational strong-field of a Kerr spacetime. Existing codes for modelling the dynamics of spinning objects like pulsars in the strong-field regime are generally lacking, since such systems occupy an intermediate regime that is generally overlooked. At the "low" end of this regime there are post-Newtonian descriptions which neglect the influence of the pulsar spin on the underlying spacetime metric ("spin-curvature" coupling). At the "high" end there are the full numerical relativity solutions which are primarily applicable toe two black holes with a mass ratio 𝒪(1), and are computationally intractable for pulsar systems observed over a large number of orbital cycles. RelativisticDynamics.jl aims to bridge this gap by providing a modern, fast code for accurate numerical evolution of spinning relativistic systems via the Mathisson-Papetrou-Dixon formalism. Julia is a modern language that solves the "two language problem", enabling fast dynamic typing and JIT compilation on conjunction with petaflop performance, comparable with numerical languages that are better known in the astrophysics community such as C or Fortran. RelativisticDynamics.jl is written to be fully type flexible, being able to support arbitrary number formats, and fully differentiable via automatic differentiation.
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