Results 1 to 10 of about 141,991 (169)
N-body simulations for parametrized modified gravity [PDF]
ABSTRACT We present MG-evolution, an N-body code simulating the cosmological structure formation for parametrized modifications of gravity. It is built from the combination of parametrized linear theory with a parametrization of the deeply non-linear cosmological regime extrapolated from modified spherical collapse computations that ...
Lucas Lombriser, Farbod Hassani
exaly +4 more sources
Planetesimal Accretion at Short Orbital Periods
Formation models in which terrestrial bodies grow via the pairwise accretion of planetesimals have been reasonably successful at reproducing the general properties of the Solar System, including small-body populations. However, planetesimal accretion has
Spencer C. Wallace, Thomas R. Quinn
doaj +1 more source
On the reliability of N-body simulations [PDF]
AbstractThe general consensus in the N-body community is that statistical results of an ensemble of collisional N-body simulations are accurate, even though individual simulations are not. A way to test this hypothesis is to make a direct comparison of an ensemble of solutions obtained by conventional methods with an ensemble of true solutions.
Boekholt, T.C.N., Portegies Zwart, S.F.
openaire +3 more sources
Accelerating Polyhedral Discrete Element Method with CUDA
This paper presents an efficient CUDA-based implementation of a nonspherical discrete element method where irregular particles are described by using polyhedrons. Two strategies are employed to exploit the parallelism of the numerical method.
Tongge Wen, Xiangyuan Zeng
doaj +1 more source
Cosmological Neutrino N-Body Simulations of Dark Matter Halo
The study of massive neutrinos and their interactions is a critical aspect of contemporary cosmology. Recent advances in parallel computation and high-performance computing provide new opportunities for accurately constraining Large-Scale Structures (LSS)
Yu Chen +5 more
doaj +1 more source
Triaxiality Inhibitors in N-body Simulations [PDF]
Abstract Numerous previous studies have investigated the phenomenon wherein initially spherical N-body systems are distorted to triaxial shapes. We report on an investigation of a previously described orbital instability that should oppose triaxiality.
Eric I. Barnes, Evan Dowling
openaire +2 more sources
The Spherical Fast Multipole Method (sFMM) for Gravitational Lensing Simulation
In this paper, we present a spherical Fast Multipole Method (sFMM) for ray-tracing simulation of gravitational lensing on a curved sky. The sFMM is a nontrivial extension of the Fast Multiple Method to sphere ${{\mathbb{S}}}^{2}$ , and it can accurately ...
Xingpao Suo +3 more
doaj +1 more source
Experiences with parallel N-body simulation [PDF]
This paper describes our experiences developing high-performance code for astrophysical N-body simulations. Recent N-body methods are based on an adaptive tree structure. The tree must be built and maintained across physically distributed memory; moreover, the communication requirements are irregular and adaptive.
Pangfeng Liu, Sandeep N. Bhatt
openaire +1 more source
N-Body Simulation on Hybrid Architectures [PDF]
N-body codes are routinely used for simulation studies of physical systems, e.g. in the fields of computational astrophysics and molecular dynamics. Typically, they require only a moderate amount of run-time memory, but are very demanding in computational power.
Sloot, P.M.A. +2 more
openaire +2 more sources
Field-level Neural Network Emulator for Cosmological N-body Simulations
We build a field-level emulator for cosmic structure formation that is accurate in the nonlinear regime. Our emulator consists of two convolutional neural networks trained to output the nonlinear displacements and velocities of N -body simulation ...
Drew Jamieson +5 more
doaj +1 more source

