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Monday, 07/24: Writing a pm-code - AIP

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dissipationless simulations 13<br />

Particle-Mesh (PM) technique: modern relevance<br />

• The popularity of PM in cosmology is due to<br />

⋆ its relative algorithmic simplicity,<br />

speed (the running time scales as ∝ O(N p )+O(N c ln N c ), where N p is the<br />

number of particles and N c is the number of grid cells; and low storage<br />

requirements;<br />

⋆ natural incorporation of periodic boundary conditions;<br />

• Today the PM technique is still very much relevant because<br />

⋆ Simplicity allows for efficient parallelization → and thus simulation on<br />

largest distributed architectures;<br />

⋆ low storage requirements allow simulation of a very large numbers of<br />

particles with relatively low resolution, suitable for some problems (e.g.,<br />

halo mass function). Papers based on pure PM simulations still appear.<br />

⋆ PM technique is used to solve for the large-scale potential and forces in<br />

many modern high-resolution methods (e.g., AP 3 M, ART, TreePM 4 ).<br />

4 now implemented inthe Gadget-2 <strong>code</strong>

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