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Cosmological N-body Simulations [PDF]

open access: yesPramana, 2021
This article, published in 1997 is somewhat inaccessible; the present posting is the original ...
Bagla, J. S., Padmanabhan, T.
openaire   +3 more sources

Planetesimal Accretion at Short Orbital Periods

open access: yesThe Astrophysical Journal, 2023
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

Accelerating Polyhedral Discrete Element Method with CUDA

open access: yesThe Astronomical Journal, 2023
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

open access: yesUniverse, 2023
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

The Spherical Fast Multipole Method (sFMM) for Gravitational Lensing Simulation

open access: yesThe Astrophysical Journal, 2023
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

Triaxiality Inhibitors in N-body Simulations [PDF]

open access: yesThe Astrophysical Journal, 2018
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

Field-level Neural Network Emulator for Cosmological N-body Simulations

open access: yesThe Astrophysical Journal, 2023
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

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

Are long-term N-body simulations reliable? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT N-body integrations are used to model a wide range of astrophysical dynamics, but they suffer from errors which make their orbits diverge exponentially in time from the correct orbits. Over long time-scales, their reliability needs to be established. We address this reliability by running a three-body planetary system over about
Junichiro Makino   +2 more
openaire   +2 more sources

Confirming Resonance in Three Transiting Systems

open access: yesThe Astronomical Journal, 2023
Although resonant planets have orbital periods near commensurability, resonance is also dictated by other factors, such as the planets’ eccentricities and masses, and therefore must be confirmed through a study of the system’s dynamics.
Tyler Quinn, Mariah G. MacDonald
doaj   +1 more source

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