Adaptive gravitational softening in gadget
Cosmological simulations of structure formation follow the collisionless evolution of dark matter starting from a nearly homogeneous field at early times down to the highly clustered configuration at redshift zero. The density field is sampled by a number of particles in number infinitely smaller th...
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Published in | Monthly notices of the Royal Astronomical Society Vol. 417; no. 4; pp. 2846 - 2859 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Oxford, UK
Blackwell Publishing Ltd
11.11.2011
Wiley-Blackwell Oxford University Press |
Subjects | |
Online Access | Get full text |
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