heyoka.py#
The heyókȟa […] is a kind of sacred clown in the culture of the Sioux (Lakota and Dakota people) of the Great Plains of North America. The heyoka is a contrarian, jester, and satirist, who speaks, moves and reacts in an opposite fashion to the people around them.
heyoka.py is a Python library for the integration of ordinary differential equations (ODEs) via Taylor’s method, based on automatic differentiation techniques and aggressive just-in-time compilation via LLVM. Notable features include:
support for single-precision, double-precision, extended-precision (80-bit and 128-bit), and arbitrary-precision floating-point types,
high-precision zero-cost dense output,
accurate and reliable event detection,
builtin support for analytical mechanics - bring your own Lagrangians/Hamiltonians and let heyoka.py formulate and solve the equations of motion,
builtin support for high-order variational equations - compute not only the solution, but also its partial derivatives,
builtin support for machine learning applications via neural network models,
the ability to maintain machine precision accuracy over tens of billions of timesteps,
batch mode integration to harness the power of modern SIMD instruction sets (including AVX/AVX2/AVX-512/Neon/VSX),
ensemble simulations and automatic parallelisation,
interoperability with SymPy.
heyoka.py is based on the heyoka C++ library.
If you are using heyoka.py as part of your research, teaching, or other activities, we would be grateful if you could star the repository and/or cite our work. For citation purposes, you can use the following BibTex entry, which refers to the heyoka.py paper (arXiv preprint):
@article{10.1093/mnras/stab1032,
author = {Biscani, Francesco and Izzo, Dario},
title = "{Revisiting high-order Taylor methods for astrodynamics and celestial mechanics}",
journal = {Monthly Notices of the Royal Astronomical Society},
volume = {504},
number = {2},
pages = {2614-2628},
year = {2021},
month = {04},
issn = {0035-8711},
doi = {10.1093/mnras/stab1032},
url = {https://doi.org/10.1093/mnras/stab1032},
eprint = {https://academic.oup.com/mnras/article-pdf/504/2/2614/37750349/stab1032.pdf}
}
heyoka.py’s novel event detection system is described in the following paper (arXiv preprint):
@article{10.1093/mnras/stac1092,
author = {Biscani, Francesco and Izzo, Dario},
title = "{Reliable event detection for Taylor methods in astrodynamics}",
journal = {Monthly Notices of the Royal Astronomical Society},
volume = {513},
number = {4},
pages = {4833-4844},
year = {2022},
month = {04},
issn = {0035-8711},
doi = {10.1093/mnras/stac1092},
url = {https://doi.org/10.1093/mnras/stac1092},
eprint = {https://academic.oup.com/mnras/article-pdf/513/4/4833/43796551/stac1092.pdf}
}
heyoka.py is released under the MPL-2.0 license. The authors are Francesco Biscani and Dario Izzo (European Space Agency).
- Celestial mechanics and astrodynamics
- The restricted three-body problem
- Continuation of Periodic Orbits in the CR3BP
- Pseudo arc-length continuation in the CR3BP
- Brouwer’s law in the outer Solar System
- Long term stability of N-body simulations: the case of Trappist-1
- Conserving first integrals via manifold projection
- Box control in satellite Formation Flying
- Comparing coordinate systems
- Inverting Kepler’s equation in ODEs
- Planetary embryos in the inner Solar System
- Mercury’s relativistic precession
- Calculating transit timing variations
- Introduction to the VSOP2013 planetary theory
- Introduction to the ELP2000 lunar theory
- Elastic tides
- Lagrange propagation and the state transition matrix
- Gravity-gradient stabilization
- A differentiable SGP4 propagator
- Event detection
- Machine Learning
- Variational equations
- Others