Abstract
A numerical algorithm capable of following the self-consistent, three-dimensional hydrodynamic evolution of gas in a multi-component universe is briefly described. The method is the merged product of a particle-particle partice-mesh (P3M) N-body scheme with a particle-based hydrodynamic approach known as smoothed particle hydrodynamics (SPH).
Keywords
- Dark Matter
- Smooth Particle Hydrodynamic
- Smooth Particle Hydrodynamic
- Smooth Particle Hydrodynamic Method
- Rich Cluster
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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References
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© 1988 Kluwer Academic Publishers
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Evrard, A.E. (1988). Extending N-Body Methods with SPH. In: Kaiser, N., Lasenby, A.N. (eds) The Post-Recombination Universe. NATO ASI Series, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3035-3_48
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DOI: https://doi.org/10.1007/978-94-009-3035-3_48
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7864-1
Online ISBN: 978-94-009-3035-3
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