Results 21 to 30 of about 17,955,789 (263)

The complexity of N-body simulation [PDF]

open access: yes, 1993
The n-body simulation problem is stated as follows: Given initial positions and velocities of n particles that have pair-wise force interactions, simulate the movement of these particles so as to determine the positions of the particles at a future time.
John H. Reif, Stephen R. Tate
openaire   +2 more sources

Investigating rotation in young massive clusters by means of hydrodynamical and direct N-body simulations [PDF]

open access: yes, 2022
One of the main open questions of star formation is the process of star clusters aggregation. In my thesis I investigate the kinematical features of embedded star clusters through hydrodynamical and N-body simulations.
Di Carlo, Ugo Niccolò
core  

Dynamical Analysis of the Maclaurin Disk with Velocity Dispersion and Its Influence on the Formation of the Bar

open access: yesThe Astrophysical Journal, 2023
We investigate the influence of Toomre’s Q parameter on the bar-forming dynamics of the Maclaurin disk using N -body simulations. According to Toomre’s criterion, the local velocity dispersion parametrized by Q ≥ 1 is required to suppress the local ...
T. Worrakitpoonpon
doaj   +1 more source

On Distributed Gravitational N-Body Simulations

open access: yesCoRR, 2022
The N-body problem is a classic problem involving a system of N discrete bodies mutually interacting in a dynamical system. At any moment in time there are N*(N - 1)/2 such interactions occurring. This scaling as N^2 leads to computational difficulties where simulations range from tens of thousands of bodies to many millions.
openaire   +2 more sources

Collisional Growth and Fragmentation of Dust Aggregates. II. Mass Distribution of Icy Fragments

open access: yesThe Astrophysical Journal, 2023
By performing N -body simulations, we investigated the fundamental processes of collisions between dust aggregates composed of submicron-sized icy dust monomers.
Yukihiko Hasegawa   +4 more
doaj   +1 more source

Halo modelling in chameleon theories [PDF]

open access: yes, 2014
We analyse modelling techniques for the large-scale structure formed in scalar-tensor theories of constant Brans-Dicke parameter which match the concordance model background expansion history and produce a chameleon suppression of the gravitational ...
Lombriser, Lucas   +5 more
core   +1 more source

Self-consistent Spin, Tidal, and Dynamical Equations of Motion in the REBOUNDx Framework

open access: yesThe Astrophysical Journal, 2023
We introduce self-consistent spin, tidal, and dynamical equations of motion into REBOUNDx , a library of additional effects for the popular N -body integrator REBOUND .
Tiger Lu   +6 more
doaj   +1 more source

A hybrid SPH/N-body method for star cluster simulations [PDF]

open access: yes, 2013
We present a new hybrid smoothed particle hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background.
Goodwin, S.P.   +3 more
core   +1 more source

N-Body Simulations of Elliptical Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1987
N-body simulations are a useful tool for constructing equilibrium models of elliptical galaxies and for the exploration of their kinematical properties, in particular the tumbling rate of the figure about some axis and the internal streaming. As yet little is known about these, except that there is a large variety of possible equilibrium models.
openaire   +2 more sources

An optimum time-stepping scheme for N-body simulations [PDF]

open access: yes, 2007
We present a new time-stepping criterion for N-body simulations that is based on the true dynamical time of a particle. This allows us to follow the orbits of particles correctly in all environments since it has better adaptivity than previous time ...
Moore, Ben   +4 more
core   +1 more source

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