Comparing Extended System Interactions with Motions in Softened Potentials
@article{Barnes2015ComparingES, title={Comparing Extended System Interactions with Motions in Softened Potentials}, author={Eric I. Barnes}, journal={arXiv: Instrumentation and Methods for Astrophysics}, year={2015} }
Using an $N$-body evolution code that does not rely on softened potentials, I have created a suite of unbound interacting cluster pair simulations. The motions of the centers of mass of the clusters have been tracked and compared to the trajectories of point masses interacting via one of four different softened potential prescriptions. I find that the relationship between the impact parameter of the cluster interaction and the point-mass softening length that best approximates each cluster's…
One Citation
Small-Scale Challenges to the ΛCDM Paradigm
- Physics
- 2017
The dark energy plus cold dark matter (ΛCDM) cosmological model has been a demonstrably successful framework for predicting and explaining the large-scale structure of the Universe and its evolution…
References
SHOWING 1-10 OF 18 REFERENCES
Optimal softening for force calculations in collisionless N-body simulations
- Physics
- 2000
In N-body simulations the force calculated between particles representing a given mass distribution is usually softened, to diminish the effect of graininess. In this paper we study the effect of…
Softening in N-body simulations of collisionless systems
- Physics
- 1993
The standard Plummer softening force law is physically inconsistent: the force on a particle is calculated as if it were a point mass, but its contribution to the gravitational field for other…
Tidal interactions between spherical galaxies
- Physics
- 1985
The impulse approximation and full N-body experiments are used to investigate the changes in mass and binding energy which result from gravitational encounters between spherical galaxies. Models with…
The Cosmological simulation code GADGET-2
- Physics
- 2005
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable of following a collisionless fluid with the N-body method, and an ideal gas by means of smoothed…
The inner structure of ΛCDM haloes – I. A numerical convergence study
- Physics
- 2002
We present a comprehensive set of convergence tests which explore the role of various numerical parameters on the equilibrium structure of a simulated dark matter halo. We report results obtained…
The dynamical fate of binary star clusters in the Galactic tidal field
- Physics
- 2016
Fragmentation and fission of giant molecular clouds occasionally results in a pair of gravitationally bound star clusters that orbit their mutual centre of mass for some time, under the influence of…
Gravitational softening as a smoothing operation
- Physics
- 2012
In self-consistent N-body simulations of collisionless systems, gravitational interactions are modified on small scales to remove singularities and simplify the task of numerically integrating the…
GADGET: a code for collisionless and gasdynamical cosmological simulations
- Physics, Computer Science
- 2001
TREESPH: A Unification of SPH with the Hierarchical Tree Method
- Physics
- 1989
A new, general-purpose code for evolving three-dimensional, self-gravitating fluids in astrophyics, both with and without collisionless matter, is described. In this TREESPH code, hydrodynamic…